Exploring the observed properties of JWST Little Red Dots with cosmological simulations and dust radiative transfer

Alessia Tortosa; Fabio Di Mascia; Luca Zappacosta; Milena Valentini; Pierluigi Rinaldi; Roberta Tripodi; Saksham Chandna; Simona Gallerani; Stefano Carniani

REVIEW

Exploring the observed properties of JWST Little Red Dots with cosmological simulations and dust radiative transfer

Saksham Chandna, Fabio Di Mascia, Simona Gallerani, Stefano Carniani, Pierluigi Rinaldi, Roberta Tripodi, Milena Valentini, Alessia Tortosa

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Luca Zappacosta

Astrophysics of Galaxies · Submitted 28 Sep 2026 · 285 references

Pith's verdict: Solid, well-built forward-modeling paper that deserves referee time, but the Sec. 6 claim that LRDs are 'not a distinct class' is stated a notch too strongly for a demonstration resting on one halo and one narrow dust corner.

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arXiv ID2609.34903 (version 1)

Pith IDJ6OLJ6NK, Pith's permanent record of this paper and its review

CitationAlessia Tortosa, Fabio Di Mascia, Luca Zappacosta, Milena Valentini, Pierluigi Rinaldi, Roberta Tripodi, Saksham Chandna, Simona Gallerani, Stefano Carniani. "Exploring the observed properties of JWST Little Red Dots with cosmological simulations and dust radiative transfer." arXiv:2609.34903 (2026). https://pith.science/paper/J6OLJ6NK

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Bottom line: this deserves a serious referee, but soften the headline before publication. The abstract's 'do not necessarily represent a distinct class' is the defensible version; the Sec. 6 phrasing [b475] — 'do not constitute a fundamentally distinct class' — outruns the evidence on the table.

What's genuinely new is the pipeline: applying the full K25 photometric selection plus the Labbe compactness criterion to mock NIRCam images from a cosmological zoom-in, then decomposing the emergent SED into stellar and AGN contributions. The picture that comes out — rest-UV from the host, red optical from a dust-attenuated central AGN, compactness tracking the AGN-to-stellar flux ratio in F444W — is clean and internally consistent. The LRD/LBD continuity via dust geometry and AGN fraction is a useful framing. The mock-observation machinery (PSF convolution, native-pixel resampling, aperture extraction) is careful and follows standard practice.

Where it's soft. Table 2 is the load-bearing wall: 100% of LRD-selected sightlines use MW-type dust at fd = 0.05–0.1; SMC dust and fd = 0.3 give zero. The demonstration therefore lives in a narrow corner of parameter space, and the authors themselves call fd and grain size poorly constrained. Second, the red optical slope and compactness both require the unresolved AGN to suffer several magnitudes of extinction in the central ~60 pc octree cells — the least-resolved part of the domain — with no torus and no sub-grid clumping tested. Third, it's one halo with a ~1% selection fraction, and Sec. 5.4's own metallicity mismatch means the successful dust content isn't independently anchored to the observed population. The conclusion-level dependence on MW/low-fd dust and on 60 pc-resolved geometry deserves an explicit caveat in Sec. 6; right now it's only implicit.

That said, the gaps the authors do flag — torus, X-ray weakness, super-Eddington accretion, extreme Balmer breaks — are flagged honestly and point at the right next steps. This is not circular in a disqualifying way; choosing parameters in a forward model is standard. But the central claim should be matched to the evidence, and a robustness run with a different grain-size distribution or a second halo would materially strengthen it. Send it to review; a good referee will push on Table 2 and the resolution, and the paper will be better for it.

Referee report

Significance

If the result holds, the paper makes a substantial contribution: a careful forward-modelling pipeline demonstrates that a standard AGN-host framework, not built to make LRDs, recovers the V-shaped continuum, compact rest-optical morphology, UV luminosities, overmassive black holes, sub-Eddington ratios, and Balmer breaks (1–2) of most observed LRDs. The SFonly run failing the compactness criterion is a genuine discriminator, establishing that an obscured AGN is required within this framework. The methodology is transparent and reproducible: 22 documented runs, published selection criteria applied exactly, and a self-consistent spectral decomposition. The X-ray, torus, super-Eddington, and extreme-Balmer gaps are honestly flagged in Sec. 5. The central caveat is that the entire LRD-selected sample occupies one narrow corner of the explored parameter space (MW dust, fd=0.05–0.1; Sec. 4.2, Table 2), and the Sec. 6 conclusion does not condition on that fact.

Major objections (4)

[Sec. 5.4 and Sec. 2.2.1] Sec. 6 states unconditionally that LRDs 'do not constitute a fundamentally distinct class of objects', but the full LRD-selected sample in Table 2 consists of 100% MW WD01 dust at fd=0.05–0.1: SMC dust, the modified SMC with amin>0.1 µm, and fd=0.3 each contribute 0% of candidates (Sec. 4.2). The paper itself describes fd and grain size as 'poorly constrained' free parameters (Sec. 2.2.1) and cites high-z evidence favouring SMC-type extinction curves. The MW-only success is therefore a necessary precondition, not an emergent prediction; the defensible version of the conclusion is the abstract's 'not necessarily' formulation. I recommend either hedging the Sec. 6 claim to match the abstract, or providing an independent argument that massive z=6–9 AGN hosts genuinely have MW-like, metal-poor dust (for instance, consistency with the FIR dust-mass upper limits already used in App. C).
[Sec. 5.4 and Sec. 2.2.1] The dust content that produces LRD selection is not independently anchored to the observed population. Sec. 5.4 reports simulated gas metallicities Z~0.5–1 Z_sun, about an order of magnitude above values inferred for observed LRDs (0.05–0.15 Z_sun). Since fd is defined as M_dust/M_Z (Eq. 3), the successful low-fd values (0.05–0.1) can be read as compensating for the over-abundant metals in the simulation rather than as a physically preferred dust fraction; equivalently, the successful runs may represent MW dust at higher fd in lower-metallicity hosts. Because fd and the dust model jointly determine membership in the final sample (Table 2), this degeneracy is load-bearing for the central claim. A concrete check would be to rerun a subset of configurations with the gas metallicity scaled down by about 0.1 dex at fixed fd (or fd raised by about 10 at fixed metallicity) and verify that the V-shape and LRD selection survive.
[Sec. 4.2, Sec. 5.1, resolution] The red optical slope and compactness of the simulated LRDs require the unresolved AGN to be attenuated by several magnitudes inside the central ~60 pc octree cells — the least-resolved part of the computational domain — while the kiloparsec-scale stellar light remains largely unobscured (Sec. 2.2.1, Sec. 4.5). With the ≲10 pc torus absent (Sec. 5.1) and no sub-grid clumping factor tested, the differential attenuation that drives the V-shape is set at the resolution scale rather than at a converged physical scale. The paper acknowledges the torus limitation but does not address the resolution dependence of the ~1% selection fraction. A test varying the octree refinement depth, or introducing a clumping factor in the inner few hundred parsecs, would establish whether the LRD rate is robust to unresolved dust geometry; without such a test the Sec. 6 claim that these properties 'emerge from ... line-of-sight dust geometry' is weaker than stated.
[Sec. 4.5 and Sec. 6 (framing)] The V-shaped continuum is largely by construction: any configuration combining a blue, weakly attenuated stellar component with a red, dust-attenuated AGN will produce a V-shaped SED; the informative content is quantitative, namely which parameter combinations land inside the observed β_UV–β_opt windows and pass the compactness cut. The paper's own decomposition (Sec. 4.5, Fig. 10) makes this mechanism explicit, so this is not a circularity error, but it affects how the 'not a distinct class' conclusion should be read. I suggest that Sec. 4.5 and Sec. 6 separate, in one or two sentences, the by-construction elements (the two-component V-shape) from the genuinely emergent ones (the compactness–AGN linkage against the SFonly baseline, the M_UV–A_V locus, the sub-Eddington ratios, and the Balmer break range), so readers can weigh which parts of the claim rest on architecture versus on the specific dust configuration.

Minor objections (4)

[References] The reference list contains a duplicate: 'Labbé, I., Van Dokkum, P., Nelson, E., et al. 2023a' and '2023b' cite the same Nature article (616, 266). Several author names appear with a stray space (e.g., 'V olonteri'); these should be cleaned up.
[Sec. 4.2] The photometric cuts are applied to continuum-only photometry (no nebular lines), and the paper notes that observed photometry contains line contamination. A brief quantitative statement of how [O III]+Hβ and Hα+[N II] contamination might shift β_UV and β_opt for borderline candidates would strengthen the comparison with surveys.
[Sec. 4.2 (final paragraph)] The ~1% selection fraction is correctly described as a per-sightline selection probability for a single halo rather than a cosmic abundance; consider restating this scope guard in the Sec. 6 bullet list, since it is essential context for the population-level claim.
[Figs. 5 and A.1] The Gaussian noise is visually prominent in the short-wavelength stamps; stating the per-filter S/N thresholds used for each stamp in the captions would aid interpretation.

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The paper

The paper claims

This paper argues that JWST's Little Red Dots are not a fundamentally distinct class of object: their V-shaped colours, compact red cores, overmassive black holes and moderate Balmer breaks emerge naturally from an ordinary massive…

The reading

JWST's Little Red Dots—compact, V-shaped sources at redshifts 4 to 9—have resisted a single explanation because they show signs of black-hole activity alongside continua that look non-AGN. This paper asks which of their properties would emerge anyway from a standard cosmological simulation of a massive quasar-host galaxy, with no LRD-specific tuning. Post-processing the simulation with dust radiative transfer and mock JWST/NIRCam images, the authors find that the characteristic blue-UV/red-optical V-shape, the compact red core, overmassive black holes, sub-Eddington accretion, and Balmer breaks of about 1 to 2 all appear in roughly one percent of simulated sightlines. They conclude that LRDs need not be a fundamentally distinct class: the same galaxy looks like an LRD when its central AGN is hidden behind dense dust while extended stellar light dominates the UV, and looks like a Little Blue Dot when that dust is absent. If right, the puzzle shifts from what LRDs are to why so many high-redshift AGN are seen through just this kind of dust geometry.

What carries the argument

The load-bearing object is a pair of cosmological zoom-in simulations of the same massive halo ($M_{\\rm halo}\\sim10^{12}\\,M_\\odot$ at $z=6$), one including black-hole growth and AGN feedback (AGNfid) and one with only star formation (SFonly), post-processed with the SKIRT dust radiative transfer code. The mechanism that carries the argument is a spatial separation of light sources—stars spread over kiloparsecs versus a central AGN sitting where dust density peaks—which splits the SED naturally: stellar light dominates blueward of the Balmer break and the attenuated AGN redward of it, producing the V-shape. Around this sit the parameter controls that make or break the effect: dust model (Milky Way versus SMC), dust-to-metal ratio ($f_d=0.05$, 0.1, 0.3), and intrinsic AGN UV slope, filtered through mock NIRCam photometry with the Kocevski et al. (2025) colour criteria ($\\beta_{\\rm UV}<-0.37$, $\\beta_{\\rm opt}>0$) and the Labbé compactness ratio $\\kappa<1.7$ between 0.4 and 0.2 arcsecond apertures in F444W.

Extended reading notes

Core claim

The paper's central claim is that the defining observational package of Little Red Dots—the V-shaped continuum, the compact unresolved rest-optical core, UV luminosities in the range the observations show, overmassive black holes, sub-Eddington accretion, and Balmer break strengths $F_{4000}/F_{3600}\\sim1$–$2$—is reproduced by an ordinary massive AGN-host galaxy simulation that was never designed to make LRDs. Spectral decomposition shows why: the rest-frame UV is dominated by kiloparsec-scale stellar emission that escapes relatively unattenuated, while the rest-frame optical is the heavily dust-attenuated central AGN emerging through the densest gas. Compactness is controlled by the stellar-to-AGN flux ratio in the F444W band, and the AGN must dominate the rest-optical light for a source to pass the compactness criterion; star-formation-only galaxies show V-shaped colours but never the compact cores. The counterfactual dust runs are the sharpest part of the argument: only Milky-Way-type dust with a dust-to-metal ratio of 0.05 to 0.1 produces LRD candidates, while SMC-type dust reddens the UV too much and higher dust-to-metal ratios obscure the AGN entirely, so the result depends on high-redshift hosts having a particular, observationally motivated but unproven dust configuration.

Load-bearing premise

The result stands on the premise that real high-redshift LRD hosts carry Milky-Way-type dust with a low dust-to-metal ratio ($f_d\\sim0.05$–$0.1$) arranged as in a single simulated massive halo, because every other dust choice in the study—SMC-type dust, higher $f_d$, or a small-grain cutoff—fails to produce LRD candidates.

Editorial extensions

If this is right

LRDs and Little Blue Dots belong to one continuous population: the simulations reproduce the observed $L_{5100}$–$\\beta_{\\rm opt}$ trend across the $\\beta_{\\rm opt}=0$ boundary, with line-of-sight dust deciding which photometric label a source receives.
AGN variability and duty-cycle changes should appear in the rest-frame optical rather than the UV, because the UV continuum is anchored by the extended stellar host while the optical tracks the obscured, accreting black hole.
Extended rest-frame UV structures—host clumps, companions, and diffuse light—around a compact red core are the expected appearance of a large fraction of LRDs, not necessarily evidence of mergers or exotic formation physics.
The dust law of $z\\sim6$–$9$ galaxies is a controlling parameter: only Milky-Way-type dust at a dust-to-metal ratio of roughly 0.05 to 0.1 passes LRD selection, so direct measurements of LRD extinction curves sharply discriminate between viable and non-viable configurations.
LRD selection fractions near one percent of sightlines mean the observed abundance of LRDs encodes viewing geometry and evolutionary phase, so differing colour cuts across surveys translate directly into different apparent number densities.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

Editorial extension: if LRDs are a viewing geometry rather than an object class, their cosmic number-density evolution partly tracks how often massive hosts present the required sightline; the framework predicts LRD analogues at any redshift where obscured massive AGN hosts exist, and a systematic decline in V-shape fraction as hosts become more dust-rich, since $f_d=0.3$ extinguishes the selectio
Editorial extension: the sharpest population test is in the X-ray, because the simulation's own numbers imply that standard sub-Eddington AGN with Milky-Way-type dust shine 20 to 60 times brighter in hard X-rays than stacked LRD limits; if deep stacking rules out Compton-thick columns ($N_H\\sim5\\times10^{23}\\,\\mathrm{cm^{-2}}$) as the cause, the ordinary-AGN-host picture would have to lean on
Editorial extension: the framework's brightest simulated sources violate existing FIR upper limits, and only its least dusty systems comply, implying that observed LRDs may be systematically fainter or less dusty than the most massive simulated hosts; an abundance-matched sample comparing LRD UV luminosities to host dust masses would quantify this offset.
Editorial extension: the predicted monotonic relation between rest-optical compactness and the stellar-to-AGN flux ratio is testable with spatially resolved rest-frame near-IR imaging of the brightest LRDs, which would confirm or refute the claim that an AGN-dominated optical core is necessary for LRD morphology.

Original abstract

JWST has uncovered compact high-redshift (z>=4) sources, dubbed Little Red Dots (LRDs), characterised by a distinct V-shaped continuum. Their nature remains debated since broad-line AGN signatures coexist with non-AGN continua, marked by weak X-ray and mid-IR emission. We investigate which properties of LRDs naturally emerge within simulations of massive AGN host galaxies and which require additional physics. We post-process two cosmological zoom-in simulations of the same massive halo, one including black hole growth and AGN feedback (AGNfid) and the other with only star formation and stellar feedback (SFonly). We analyse snapshots spanning z=6-9 to probe different evolutionary stages. Using SKIRTv8, we develop a forward-modelling framework exploring various dust models, dust-to-metal ratios, and intrinsic AGN spectra. We generate mock spectra and images to apply JWST observational LRD selection criteria. Not designed to model LRDs, our AGNfid simulations naturally reproduce their properties: V-shaped continua, compact morphologies with rest-UV complexity, UV luminosities, attenuations, overmassive BHs, sub-Eddington accretion, and Balmer break strengths (~1-2) typical of most LRDs. Spectral decomposition reveals that the rest-UV continuum is dominated by stellar emission, whereas the optical continuum stems from a dust-attenuated AGN. Dust geometry and AGN-to-stellar contribution drive photometric differences between LRDs and Little Blue Dots. Our results suggest that LRDs do not necessarily represent a distinct class of objects. Instead, their defining properties can arise in massive AGN host galaxies from the interplay between stellar emission, an obscured central engine, and dust geometry. Super-Eddington accretion, dust-free gas columns, evolved stellar populations, and photoionisation modelling are required to test whether this framework reproduces the diversity of observed LRDs.

The compiled record

The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-29: 1 request, 9,668 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.95 · human participants 0.01 · controlled comparison 0.88 · randomized assignment 0.01 · states quantitative result 0.94 · compares with prior results 0.65 · mentions code or data availability 0.03.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; show every role.

JWST has uncovered compact high-redshift (z>=4) sources, dubbed Little Red Dots (LRDs), characterised by a distinct V-shaped continuum. Their nature remains debated since broad-line AGN signatures coexist with non-AGN continua, marked by weak X-ray and mid-IR emission. We investigate which properties of LRDs naturally emerge within simulations of massive AGN host galaxies and which require additional physics. We post-process two cosmological zoom-in simulations of the same massive halo, one including black hole growth and AGN feedback (AGNfid) and the other with only star formation and stellar feedback (SFonly). We analyse snapshots spanning z=6-9 to probe different evolutionary stages. Using SKIRTv8, we develop a forward-modelling framework exploring various dust models, dust-to-metal ratios, and intrinsic AGN spectra. We generate mock spectra and images to apply JWST observational LRD selection criteria. Not designed to model LRDs, our AGNfid simulations naturally reproduce their properties: V-shaped continua, compact morphologies with rest-UV complexity, UV luminosities, attenuations, overmassive BHs, sub-Eddington accretion, and Balmer break strengths (~1-2) typical of most LRDs. Spectral decomposition reveals that the rest-UV continuum is dominated by stellar emission, whereas the optical continuum stems from a dust-attenuated AGN. Dust geometry and AGN-to-stellar contribution drive photometric differences between LRDs and Little Blue Dots. Our results suggest that LRDs do not necessarily represent a distinct class of objects. Instead, their defining properties can arise in massive AGN host galaxies from the interplay between stellar emission, an obscured central engine, and dust geometry. Super-Eddington accretion, dust-free gas columns, evolved stellar populations, and photoionisation modelling are required to test whether this framework reproduces the diversity of observed LRDs.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	JWST has uncovered compact high-redshift (z>=4) sources, dubbed Little Red Dots (LRDs), characterised by a distinct V-shaped continuum.	background 1.00	0.08	0.02	asserted 1.00
s1	Their nature remains debated since broad-line AGN signatures coexist with non-AGN continua, marked by weak X-ray and mid-IR emission.	background 0.69	0.05	0.02	asserted 0.98
s2	We investigate which properties of LRDs naturally emerge within simulations of massive AGN host galaxies and which require additional physics.	contribution 0.94	0.52	0.03	unclear 0.59
s3	We post-process two cosmological zoom-in simulations of the same massive halo, one including black hole growth and AGN feedback (AGNfid) and the other with only star formation and stellar feedback (SFonly).	method 0.99	0.96	0.02	asserted 0.94
s4	We analyse snapshots spanning z=6-9 to probe different evolutionary stages.	method 0.99	0.90	0.01	asserted 0.78
s5	Using SKIRTv8, we develop a forward-modelling framework exploring various dust models, dust-to-metal ratios, and intrinsic AGN spectra.	method 1.00	0.95	0.02	asserted 0.99
s6	We generate mock spectra and images to apply JWST observational LRD selection criteria.	method 0.99	0.95	0.02	asserted 0.98
s7	Not designed to model LRDs, our AGNfid simulations naturally reproduce their properties: V-shaped continua, compact morphologies with rest-UV complexity, UV luminosities, attenuations, overmassive BHs, sub-Eddington accretion, and Balmer break strengths (~1-2) typical of most LRDs.	result 1.00	0.93	0.48	asserted 1.00
s8	Spectral decomposition reveals that the rest-UV continuum is dominated by stellar emission, whereas the optical continuum stems from a dust-attenuated AGN.	result 0.94	0.93	0.07	asserted 1.00
s9	Dust geometry and AGN-to-stellar contribution drive photometric differences between LRDs and Little Blue Dots.	result 0.66	0.82	0.06	asserted 1.00
s10	Our results suggest that LRDs do not necessarily represent a distinct class of objects.	interpretation 0.98	0.74	0.63	hedged possibility 0.98
s11	Instead, their defining properties can arise in massive AGN host galaxies from the interplay between stellar emission, an obscured central engine, and dust geometry.	interpretation 1.00	0.79	0.78	asserted 0.56
s12	Super-Eddington accretion, dust-free gas columns, evolved stellar populations, and photoionisation modelling are required to test whether this framework reproduces the diversity of observed LRDs.	future work 0.91	0.17	0.07	asserted 0.70

What kind of paper the classifier reports this is: simulation study 1.00 · evidence from simulation or computation 1.00.

What was examined, and what was not

sources read

arXiv listing abstract v1

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

not run

S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

Figures

**Figure 1.** Schematic overview of the pipeline used to produce mock photometric maps from the radiative transfer outputs. For visualisation, the colour scales are saturated above fixed fractions of the peak flux, such that all values exceeding the threshold are assigned the same colour. The intrinsic 2D maps are capped at 1% of the maximum flux, while the convolved and noise-added maps are capped at 50% of the maximum flux, improving the visibility of extended structures in the presence of bright central pixels. filter maps have a finer spatial sampling than the native NIRCam pixel scale…

**Figure 2.** shows the SEDs extracted using a Dap = 0.4 ′′ diameter aperture applied directly to the 3D spectral data cubes generated by our RT calculations (see Sec. 2.2). Each simulated object is observed along six perpendicular lines of sight, with each line of sight treated as an independent mock observation of an LRD candidate. The two panels show the results for the SFonly and AGNfid simulation suites separately. The SFonly and AGNfid suites exhibit comparable flux levels in the rest-frame UV (ranging from 10−3µJy to 0.5 − 1µJy), whereas the AGNfid spectra become systematically brighter…

**Figure 3.** Distribution of synthetic sources in the rest-frame spectral index plane (βUV vs. βopt) extracted from the AGNfid suite (left panel) and the SFonly suite (right panel). The horizontal dashed line at βopt = 0 separates sources with red optical continua (βopt > 0) from those with blue optical continua. The vertical dashed lines mark the boundaries of the rest-frame UV selection: βUV = −0.37 denotes the upper limit for blue UV colours, while βUV = −2.8 represents the lower cutoff adopted in empirical surveys to exclude Galactic brown dwarf contaminants. In both panels, star markers…

**Figure 5.** Mock JWST/NIRCam image stamps and corresponding three-colour RGB composites generated using the post-processing procedure described in Sec. 3 for a representative subset of the simulated LRDs selected in Sec. 4.2. The redshift of each source is indicated in the RGB panel. Each panel shows a 2′′ × 2 ′′ field of view (∼ 11 × 11 physical kpc at z = 6.4), centered on the most luminous source within the central massive halo in the NIRCam F444W band. The dashed white circle overplotted on each single-filter panel represents the 0.4 ′′ diameter photometric aperture (Dap = 0.4 ′′,…

**Figure 6.** Observed properties of our AGNfid sample. Star markers denote sources that are compact (κ < 1.7), whereas circles indicate extended sources. Red (pink) markers designate sources satisfying all LRD photometric selection criteria (simulated LRDs), blue (light-blue) markers signify sources that violate only the βopt cutoff (simulated LBDs), while green (light-green) markers identify sources that fail the rest-UV selection (βUV) for compact (extended) populations. Gray markers correspond to sources falling below the adopted detection threshold (Sec. 4.2). Marginal histograms along the…

**Figure 7.** Comparison of rest-frame SED shape for our simulated AGNfid sample against observational composite spectra from Pérez-González et al. 2026. Red (blue) dashed curves represent normalised SEDs for our simulated compact LRD (LBD) candidates, defined by their compactness and v-shape (blue optical slope, βopt < 0) criteria. For comparison, solid curves depict the empirical stacked spectra of xLRDs (magenta), +LRDs (yellow), −LRDs (lime), and bLRDs (cyan). All spectra are normalised to flux density at rest-frame λ = 0.55 µm. In agreement with data, our LRD candidates are systematically…

**Figure 8.** Intrinsic physical properties of the simulated sources in the AGNfid suite. Star markers denote sources that are compact, whereas circles indicate extended sources. Red (pink) markers designate sources satisfying all LRD photometric selection criteria, blue (light-blue) markers signify sources that violate only the βopt cutoff, while green (light-green) markers identify sources that fail the rest-UV selection (βUV) for compact (extended) populations. Gray markers correspond to sources falling below the adopted detection threshold. Left panel: Black hole mass (MBH) versus host galaxy…

**Figure 9.** Optical continuum slope (βopt) versus monochromatic luminosity at rest-frame 5100 Å (log10(L5100/erg s−1 )) for our simulated LRDs and LBDs. Red star markers denote simulated LRDs satisfying all LRD photometric criteria, whereas blue star markers designate simulated LBDs, which violate solely the optical slope selection (βopt < 0). For comparison, coloured pentagons indicate median values inferred from the stacked NIRSpec/PRISM spectra of four LRD subtypes (xLRD in magenta, +LRD in yellow, −LRD in green, and bLRD in cyan) from Pérez-González et al. 2026. The pink shaded region…

**Figure 11.** Compactness ratio (κ) as a function of the observed stellar-to-black hole flux ratio (f ⋆ 444/ f BH 444 ) in the JWST/NIRCam F444W bandpass. The dashed horizontal line denotes the threshold (κ = 1.7) separating extended systems from the compact region (shaded green area). Red (pink) markers designate sources satisfying all LRD photometric selection criteria, blue (lightblue) markers signify sources that violate only the βopt cutoff, while green (light-green) markers identify sources that fail the rest-UV selection (βUV) for compact (extended) populations. Gray markers correspond

Showing 9 of the paper's 11 figures. See all figures in the PDF ↗ Figures reproduced from arXiv:2609.34903 by the authors.

References

Works cited (285)

[1]

Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model. arXiv e-prints , keywords =. doi:10.48550/arXiv.2602.22386 , archivePrefix =. 2602.22386 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2602.22386
[2]

You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei. , keywords =. doi:10.1051/0004-6361/202659544 , adsurl =

View on Pith doi:10.1051/0004-6361/202659544
[3]

Ionizing Photon Production Efficiencies and Chemical Abundances at Cosmic Dawn Revealed by Ultradeep Rest-frame Optical Spectroscopy of JADES-GS-z14-0. , keywords =. doi:10.3847/2041-8213/ae7446 , archivePrefix =. 2512.19695 , primaryClass =

View on Pith arXiv
[4]

The Atmospheric Structure of the O-Type Giant Krzeminski's Star and the Mass of its Companion Neutron Star Centaurus X-3. , keywords =. doi:10.1086/165954 , adsurl =

View on Pith doi:10.1086/165954
[5]

Too many or too massive? Investigating the high-z demography of active SMBHs from JWST. , keywords =. doi:10.1093/mnras/stag223 , archivePrefix =. 2601.23250 , primaryClass =

View on Pith arXiv
[6]

A Selection Aware View of Black Hole-Galaxy Coevolution at High Redshift. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.04358 , archivePrefix =. 2603.04358 , primaryClass =

View on Pith doi:10.48550/arxiv.2603.04358
[7]

Active galactic nuclei-heated dust revealed in ``little red dots''. , keywords =. doi:10.1051/0004-6361/202557164 , archivePrefix =. 2509.07100 , primaryClass =

View on Pith arXiv
[8]

What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots. , keywords =. doi:10.3847/1538-4357/ae1836 , archivePrefix =. 2509.05434 , primaryClass =

View on Pith Pith review arXiv
[9]

From ``The Cliff'' to ``Virgil'': Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec. , keywords =. doi:10.3847/1538-4357/ae5d2c , archivePrefix =. 2512.15853 , primaryClass =

View on Pith arXiv
[10]

Radiative Transfer in Circumstellar Dust Clouds. Interstellar Dust and Related Topics , year = 1973, editor =

View on Pith 1973
[11]

Astrophysics of gaseous nebulae and active galactic nuclei

View on Pith
[12]

Analytical Approximations for Calculating the Escape and Absorption of Radiation in Clumpy Dusty Environments. , keywords =. doi:10.1086/307729 , archivePrefix =. astro-ph/9905029 , primaryClass =

View on Pith Pith review arXiv
[13]

'Little red dots' cannot reside in the same dark matter haloes as comparably luminous unobscured quasars. , keywords =. doi:10.1093/mnras/staf660 , archivePrefix =. 2409.18208 , primaryClass =

View on Pith Pith review arXiv
[14]

Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe. arXiv e-prints , keywords =. doi:10.48550/arXiv.2402.18773 , archivePrefix =. 2402.18773 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2402.18773
[15]

Seeking the growth of the first black hole seeds with JWST. , keywords =. doi:10.1093/mnras/stac3768 , archivePrefix =. 2211.01389 , primaryClass =

View on Pith Pith review arXiv
[16]

Comparing Single-epoch Virial Black Hole Mass Estimators for Luminous Quasars. , keywords =. doi:10.1088/0004-637X/753/2/125 , archivePrefix =. 1203.0601 , primaryClass =

View on Pith Pith review arXiv
[17]

A small and vigorous black hole in the early Universe. arXiv e-prints , keywords =. doi:10.48550/arXiv.2305.12492 , archivePrefix =. 2305.12492 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2305.12492
[18]

Sustained super-Eddington accretion in high-redshift quasars. arXiv e-prints , keywords =. doi:10.48550/arXiv.2312.08422 , archivePrefix =. 2312.08422 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2312.08422
[19]

XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch. , keywords =. doi:10.1093/mnras/stad1468 , archivePrefix =. 2305.05053 , primaryClass =

View on Pith Pith review arXiv
[20]

The growth efficiency of high-redshift black holes. , keywords =. doi:10.1093/mnras/stv1465 , archivePrefix =. 1506.04750 , primaryClass =

View on Pith Pith review arXiv
[21]

Super-Eddington growth of the first black holes. , keywords =. doi:10.1093/mnras/stw505 , archivePrefix =. 1603.00475 , primaryClass =

View on Pith Pith review arXiv
[22]

Mass Functions of the Active Black Holes in Distant Quasars from the Large Bright Quasar Survey, the Bright Quasar Survey, and the Color-selected Sample of the SDSS Fall Equatorial Stripe. , keywords =. doi:10.1088/0004-637X/699/1/800 , archivePrefix =. 0904.3348 , primaryClass =

View on Pith Pith review arXiv
[23]

A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 7. , keywords =. doi:10.1088/0067-0049/194/2/45 , archivePrefix =. 1006.5178 , primaryClass =

View on Pith Pith review arXiv
[24]

The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars. , keywords =. doi:10.3847/1538-4357/ac9626 , archivePrefix =. 2207.05113 , primaryClass =

View on Pith Pith review arXiv
[25]

Galactic winds in cosmological simulations of the circumgalactic medium. , keywords =. doi:10.1093/mnras/stt125 , archivePrefix =. 1210.3582 , primaryClass =

View on Pith Pith review arXiv
[26]

Host galaxies of high-redshift quasars: SMBH growth and feedback. , keywords =. doi:10.1093/mnras/stab1992 , archivePrefix =. 2107.05638 , primaryClass =

View on Pith Pith review arXiv
[27]

On spherically symmetrical accretion. , year = 1952, month = jan, volume =. doi:10.1093/mnras/112.2.195 , adsurl =

View on Pith doi:10.1093/mnras/112.2.195 1952
[28]

JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr after the Big Bang. , keywords =. doi:10.3847/1538-4357/acdbc6 , archivePrefix =. 2302.07234 , primaryClass =

View on Pith Pith review arXiv
[29]

Statistics of extremes , author=. 1958 , publisher=

View on Pith 1958
[30]

Extreme value distributions: theory and applications , author=. 2000 , publisher=

View on Pith 2000
[31]

Table for estimating the goodness of fit of empirical distributions , author=. The annals of mathematical statistics , volume=. 1948 , publisher=

View on Pith 1948
[32]

Two Remarkably Luminous Galaxy Candidates at z 10-12 Revealed by JWST. , keywords =. doi:10.3847/2041-8213/ac9b22 , archivePrefix =. 2207.09434 , primaryClass =

View on Pith Pith review arXiv
[33]

Large-scale bias and the peak background split. , keywords =. doi:10.1046/j.1365-8711.1999.02692.x , archivePrefix =. astro-ph/9901122 , primaryClass =

View on Pith arXiv 1999
[34]

JADES NIRSpec Spectroscopy of GN-z11: Lyman- emission and possible enhanced nitrogen abundance in a z = 10.60 luminous galaxy. , keywords =. doi:10.1051/0004-6361/202346159 , archivePrefix =. 2302.07256 , primaryClass =

View on Pith Pith review arXiv
[35]

Planck 2018 results. VI. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201833910 , archivePrefix =. 1807.06209 , primaryClass =

View on Pith Pith review arXiv 2018
[36]

On the stunning abundance of super-early, luminous galaxies revealed by JWST. , keywords =. doi:10.1093/mnras/stad1095 , archivePrefix =. 2208.00720 , primaryClass =

View on Pith Pith review arXiv
[37]

Essential physics of early galaxy formation. , keywords =. doi:10.1093/mnras/stu1848 , archivePrefix =. 1405.4862 , primaryClass =

View on Pith Pith review arXiv
[38]

How the super-Eddington regime regulates black hole growth in high-redshift galaxies. , keywords =. doi:10.1051/0004-6361/202243170 , archivePrefix =. 2201.08766 , primaryClass =

View on Pith Pith review arXiv
[39]

XQR-30: Black hole masses and accretion rates of 42 z 6 quasars. , keywords =. doi:10.1051/0004-6361/202346317 , archivePrefix =. 2306.16474 , primaryClass =

View on Pith Pith review arXiv
[40]

The Internal Constitution of the Stars

View on Pith
[41]

Euclid preparation. V. Predicted yield of redshift 7 < z < 9 quasars from the wide survey. , keywords =. doi:10.1051/0004-6361/201936427 , archivePrefix =. 1908.04310 , primaryClass =

View on Pith Pith review arXiv 1908
[42]

Kinetic and radiative power from optically thin accretion flows. , keywords =. doi:10.1093/mnras/stx543 , archivePrefix =. 1701.07033 , primaryClass =

View on Pith Pith review arXiv
[43]

Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time. , keywords =. doi:10.1093/mnras/stz3131 , archivePrefix =. 1911.02572 , primaryClass =

View on Pith Pith review arXiv 1911
[45]

A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations. , keywords =. doi:10.1093/mnras/stv072 , archivePrefix =. 1409.3221 , primaryClass =

View on Pith Pith review arXiv
[47]

SKIRT: An advanced dust radiative transfer code with a user-friendly architecture. Astronomy and Computing , keywords =. doi:10.1016/j.ascom.2014.10.004 , archivePrefix =. 1410.1629 , primaryClass =

View on Pith Pith review arXiv 2014
[48]

The EAGLE project: simulating the evolution and assembly of galaxies and their environments. , keywords =. doi:10.1093/mnras/stu2058 , archivePrefix =. 1407.7040 , primaryClass =

View on Pith Pith review arXiv
[52]

Simulating galaxy formation with the IllustrisTNG model. , keywords =. doi:10.1093/mnras/stx2656 , archivePrefix =. 1703.02970 , primaryClass =

View on Pith Pith review arXiv
[53]

Simulating galaxy formation with black hole driven thermal and kinetic feedback. , keywords =. doi:10.1093/mnras/stw2944 , archivePrefix =. 1607.03486 , primaryClass =

View on Pith Pith review arXiv
[54]

Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships. , keywords =. doi:10.1086/500572 , archivePrefix =. astro-ph/0601303 , primaryClass =

View on Pith Pith review arXiv
[55]

A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy. , keywords =. doi:10.3847/0004-637X/819/2/129 , archivePrefix =. 1603.00461 , primaryClass =

View on Pith Pith review arXiv
[56]

In the beginning: the first sources of light and the reionization of the universe. , keywords =. doi:10.1016/S0370-1573(01)00019-9 , archivePrefix =. astro-ph/0010468 , primaryClass =

View on Pith Pith review arXiv
[57]

Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with CDM?. , keywords =. doi:10.1093/mnras/stac3224 , archivePrefix =. 2208.10479 , primaryClass =

View on Pith Pith review arXiv
[58]

On the abundance of extreme voids. , keywords =. doi:10.1088/1475-7516/2015/05/062 , archivePrefix =. 1502.07705 , primaryClass =

View on Pith Pith review arXiv 2015
[59]

Cluster-Void Degeneracy Breaking: Dark Energy, Planck, and the Largest Cluster and Void. , keywords =. doi:10.3847/2041-8205/820/1/L7 , archivePrefix =. 1511.04075 , primaryClass =

View on Pith Pith review arXiv
[60]

Exact extreme value statistics and the halo mass function. , keywords =. doi:10.1111/j.1745-3933.2011.01134.x , archivePrefix =. 1108.1358 , primaryClass =

View on Pith arXiv 2011
[62]

Primordial non-Gaussianity and extreme-value statistics of galaxy clusters. , keywords =. doi:10.1103/PhysRevD.85.063508 , archivePrefix =. 1107.5617 , primaryClass =

View on Pith Pith review arXiv
[63]

Extreme-value statistics of the spin of primordial black holes. , keywords =. doi:10.1103/PhysRevD.104.083018 , archivePrefix =. 2109.12268 , primaryClass =

View on Pith Pith review arXiv
[67]

Quasars and the Intergalactic Medium at Cosmic Dawn. , keywords =. doi:10.1146/annurev-astro-052920-102455 , archivePrefix =. 2212.06907 , primaryClass =

View on Pith Pith review arXiv
[68]

A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey. I. Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z -0.5ex 6. , keywords =. doi:10.1086/324111 , archivePrefix =. astro-ph/0108063 , primaryClass =

View on Pith Pith review arXiv
[69]

A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey. II. Discovery of Three Additional Quasars at z>6. , keywords =. doi:10.1086/368246 , archivePrefix =. astro-ph/0301135 , primaryClass =

View on Pith Pith review arXiv
[70]

A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey. IV. Discovery of Seven Additional Quasars. , keywords =. doi:10.1086/500296 , archivePrefix =. astro-ph/0512080 , primaryClass =

View on Pith Pith review arXiv
[71]

First Results from the Canada-France High-z Quasar Survey: Constraints on the z = 6 Quasar Luminosity Function and the Quasar Contribution to Reionization. , keywords =. doi:10.1086/462408 , archivePrefix =. astro-ph/0507183 , primaryClass =

View on Pith Pith review arXiv
[72]

Six More Quasars at Redshift 6 Discovered by the Canada-France High-z Quasar Survey. , keywords =. doi:10.1088/0004-6256/137/3/3541 , archivePrefix =. 0901.0565 , primaryClass =

View on Pith Pith review arXiv
[73]

The Canada-France High-z Quasar Survey: Nine New Quasars and the Luminosity Function at Redshift 6. , keywords =. doi:10.1088/0004-6256/139/3/906 , archivePrefix =. 0912.0281 , primaryClass =

View on Pith Pith review arXiv
[74]

Discovery of Three z > 6.5 Quasars in the VISTA Kilo-Degree Infrared Galaxy (VIKING) Survey. , keywords =. doi:10.1088/0004-637X/779/1/24 , archivePrefix =. 1311.3666 , primaryClass =

View on Pith Pith review arXiv
[75]

First discoveries of z 6 quasars with the Kilo-Degree Survey and VISTA Kilo-Degree Infrared Galaxy survey. , keywords =. doi:10.1093/mnras/stv1774 , archivePrefix =. 1507.00726 , primaryClass =

View on Pith Pith review arXiv
[76]

The Assembly of the First Massive Black Holes. , keywords =. doi:10.1146/annurev-astro-120419-014455 , archivePrefix =. 1911.05791 , primaryClass =

View on Pith Pith review arXiv 1911
[77]

z -0.5ex 7 Galaxy Candidates from NICMOS Observations Over the HDF-South and the CDF-South and HDF-North Goods Fields. , keywords =. doi:10.1088/0004-637X/725/2/1587 , archivePrefix =. 1003.1706 , primaryClass =

View on Pith Pith review arXiv
[78]

Overview of the JWST Advanced Deep Extragalactic Survey (JADES). arXiv e-prints , keywords =. doi:10.48550/arXiv.2306.02465 , archivePrefix =. 2306.02465 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2306.02465
[79]

Black holes in the early Universe. Reports on Progress in Physics , keywords =. doi:10.1088/0034-4885/75/12/124901 , archivePrefix =. 1209.2243 , primaryClass =

View on Pith Pith review arXiv
[80]

The origins of massive black holes. Nature Reviews Physics , keywords =. doi:10.1038/s42254-021-00364-9 , archivePrefix =. 2110.10175 , primaryClass =

View on Pith Pith review arXiv
[82]

The First Massive Black Hole Seeds and Their Hosts. , keywords =. doi:10.1088/0004-637X/742/1/13 , archivePrefix =. 1104.3858 , primaryClass =

View on Pith Pith review arXiv
[83]

Formation of Supermassive Black Hole Seeds. , keywords =. doi:10.1017/pasa.2016.41 , archivePrefix =. 1605.07391 , primaryClass =

View on Pith Pith review arXiv 2016
[84]

Feedback-regulated supermassive black hole seed formation. , keywords =. doi:10.1093/mnras/stu1007 , archivePrefix =. 1405.6743 , primaryClass =

View on Pith Pith review arXiv
[85]

The formation of the first quasars: the black hole seeds, accretion, and feedback models. , keywords =. doi:10.1093/mnras/stac1556 , archivePrefix =. 2012.01458 , primaryClass =

View on Pith Pith review arXiv 2012
[86]

Sulla determinazione empirica di una lgge di distribuzione , author=. Inst. Ital. Attuari, Giorn. , volume=

View on Pith
[87]

Star Formation. doi:10.1142/10091 , adsurl =

View on Pith doi:10.1142/10091
[88]

Nuclear activity versus star formation: emission-line diagnostics at ultraviolet and optical wavelengths. , keywords =. doi:10.1093/mnras/stv2794 , archivePrefix =. 1511.08217 , primaryClass =

View on Pith Pith review arXiv
[89]

Multiline Assessment of Narrow-line Regions in z 3 Radio Galaxies. , keywords =. doi:10.3847/1538-4357/ac5b71 , archivePrefix =. 2203.03390 , primaryClass =

View on Pith Pith review arXiv
[90]

The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]- 1908 A emission 10.8 to 12.5 Gyr ago. , keywords =. doi:10.1051/0004-6361/201732197 , archivePrefix =. 1710.10715 , primaryClass =

View on Pith Pith review arXiv 1908
[91]

High velocity outflows in quasars

View on Pith
[92]

Statistical analysis of Al III and C III] emission lines as virial black hole mass estimators in quasars. , keywords =. doi:10.1051/0004-6361/202244177 , archivePrefix =. 2209.05526 , primaryClass =

View on Pith Pith review arXiv
[93]

The formation of supermassive black holes from Population III.1 seeds. I. Cosmic formation histories and clustering properties. , keywords =. doi:10.1093/mnras/sty3298 , archivePrefix =. 1608.04421 , primaryClass =

View on Pith Pith review arXiv
[94]

The formation of supermassive black holes from Population III.1 seeds. II. Evolution to the local universe. , keywords =. doi:10.1093/mnras/stad2346 , archivePrefix =. 2301.11464 , primaryClass =

View on Pith Pith review arXiv
[95]

Conditions for Optimal Growth of Black Hole Seeds. , keywords =. doi:10.3847/2041-8213/aa9aea , archivePrefix =. 1710.09375 , primaryClass =

View on Pith Pith review arXiv
[96]

The growth of black holes from Population III remnants in the Renaissance simulations. , keywords =. doi:10.1093/mnras/sty2103 , archivePrefix =. 1804.06477 , primaryClass =

View on Pith Pith review arXiv
[97]

Diagnostics for PopIII galaxies and direct collapse black holes in the early universe. , keywords =. doi:10.1093/mnras/stac1242 , archivePrefix =. 2204.11870 , primaryClass =

View on Pith Pith review arXiv
[98]

The characteristic black hole mass resulting from direct collapse in the early Universe. , keywords =. doi:10.1093/mnras/stt1786 , archivePrefix =. 1309.1097 , primaryClass =

View on Pith Pith review arXiv
[99]

Formation of the First Nuclear Clusters and Massive Black Holes at High Redshift. , keywords =. doi:10.1088/0004-637X/694/1/302 , archivePrefix =. 0810.1057 , primaryClass =

View on Pith Pith review arXiv
[100]

Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes. , keywords =. doi:10.1046/j.1365-8711.2001.04006.x , archivePrefix =. astro-ph/9907024 , primaryClass =

View on Pith arXiv 2001
[101]

HMFcalc: An online tool for calculating dark matter halo mass functions. Astronomy and Computing , keywords =. doi:10.1016/j.ascom.2013.11.001 , archivePrefix =. 1306.6721 , primaryClass =

View on Pith Pith review arXiv 2013
[102]

Growing massive black holes through supercritical accretion of stellar-mass seeds. , keywords =. doi:10.1093/mnras/stv2877 , archivePrefix =. 1512.02651 , primaryClass =

View on Pith Pith review arXiv
[103]

Supermassive black holes in cosmological simulations I: M _ BH - M _ relation and black hole mass function. , keywords =. doi:10.1093/mnras/stab496 , archivePrefix =. 2006.10094 , primaryClass =

View on Pith Pith review arXiv 2006
[104]

Supermassive black holes in cosmological simulations - II: the AGN population and predictions for upcoming X-ray missions. , keywords =. doi:10.1093/mnras/stab3147 , archivePrefix =. 2111.01802 , primaryClass =

View on Pith Pith review arXiv
[105]

Simulating the growth of Intermediate Mass Black Holes. , keywords =. doi:10.1093/mnras/stv018 , archivePrefix =. 1501.00989 , primaryClass =

View on Pith Pith review arXiv
[106]

Super-critical Growth of Massive Black Holes from Stellar-mass Seeds. , keywords =. doi:10.1088/2041-8205/784/2/L38 , archivePrefix =. 1402.6995 , primaryClass =

View on Pith Pith review arXiv
[107]

Slim Disks Around Kerr Black Holes Revisited. , keywords =. doi:10.1088/0067-0049/183/2/171 , archivePrefix =. 0906.0355 , primaryClass =

View on Pith Pith review arXiv
[108]

Growth problems of stellar black holes in early galaxies. , keywords =. doi:10.1093/mnras/sty1482 , archivePrefix =. 1807.05760 , primaryClass =

View on Pith Pith review arXiv
[109]

The sustainable growth of the first black holes. , keywords =. doi:10.1093/mnras/stx1640 , archivePrefix =. 1706.06592 , primaryClass =

View on Pith Pith review arXiv
[110]

Relations between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe. , keywords =. doi:10.1088/0004-637X/813/2/82 , archivePrefix =. 1508.06274 , primaryClass =

View on Pith Pith review arXiv
[111]

The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies. , keywords =. doi:10.1051/0004-6361/201936634 , archivePrefix =. 2002.00958 , primaryClass =

View on Pith Pith review arXiv 2002
[112]

JWST CEERS and JADES Active Galaxies at z = 4-7 Violate the Local M _ -M _ Relation at >3 : Implications for Low-mass Black Holes and Seeding Models. , keywords =. doi:10.3847/2041-8213/ad0158 , archivePrefix =. 2308.12331 , primaryClass =

View on Pith Pith review arXiv
[113]

GN-z11: The environment of an AGN at z= 10.603. arXiv e-prints , keywords =. doi:10.48550/arXiv.2306.09142 , archivePrefix =. 2306.09142 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2306.09142
[114]

Kiloparsec-scale ALMA Imaging of [C II] and Dust Continuum Emission of 27 Quasar Host Galaxies at z 6. , keywords =. doi:10.3847/1538-4357/abc563 , archivePrefix =. 2010.14874 , primaryClass =

View on Pith Pith review arXiv 2010
[115]

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-luminosity Quasar at z = 7.07 on the Local Black Hole to Host Mass Relation. , keywords =. doi:10.3847/1538-4357/abf6dc , archivePrefix =. 2104.05738 , primaryClass =

View on Pith Pith review arXiv
[116]

Intermediate-Mass Black Holes. , keywords =. doi:10.1146/annurev-astro-032620-021835 , archivePrefix =. 1911.09678 , primaryClass =

View on Pith Pith review arXiv 1911
[117]

The formation of nuclei in newly formed galaxies and the evolution of the quasar population. , keywords =. doi:10.1093/mnras/263.1.168 , adsurl =

View on Pith doi:10.1093/mnras/263.1.168
[119]

Massive Black Holes as Population III Remnants. , keywords =. doi:10.1086/319848 , archivePrefix =. astro-ph/0101223 , primaryClass =

View on Pith Pith review arXiv
[120]

Initial mass function of intermediate-mass black hole seeds. , keywords =. doi:10.1093/mnras/stu1280 , archivePrefix =. 1406.6685 , primaryClass =

View on Pith Pith review arXiv
[121]

A Snapshot Survey for Gravitational Lenses among z>=4.0 Quasars. II. Constraints on the 4.0<z<5.4 Quasar Population. , keywords =. doi:10.1086/498063 , archivePrefix =. astro-ph/0509135 , primaryClass =

View on Pith Pith review arXiv
[123]

Physical Properties of the First Quasars. , keywords =. doi:10.1017/pasa.2017.14 , archivePrefix =. 1702.06123 , primaryClass =

View on Pith Pith review arXiv 2017
[124]

Correcting C IV-based virial black hole masses. , keywords =. doi:10.1093/mnras/stw2797 , archivePrefix =. 1610.08977 , primaryClass =

View on Pith Pith review arXiv
[125]

Detecting and Characterizing Young Quasars. II. Four Quasars at z 6 with Lifetimes < 10 ^ 4 Yr. , keywords =. doi:10.3847/1538-4357/ac0a76 , archivePrefix =. 2106.04586 , primaryClass =

View on Pith Pith review arXiv
[126]

An ALMA [C II] Survey of 27 Quasars at z > 5.94. , keywords =. doi:10.3847/1538-4357/aaa5aa , archivePrefix =. 1801.02641 , primaryClass =

View on Pith Pith review arXiv
[127]

Probing the Interstellar Medium and Star Formation of the Most Luminous Quasar at z = 6.3. , keywords =. doi:10.3847/0004-637X/830/1/53 , archivePrefix =. 1606.09634 , primaryClass =

View on Pith Pith review arXiv
[128]

Molecular gas in z 6 quasar host galaxies. , keywords =. doi:10.1051/0004-6361/202142871 , archivePrefix =. 2203.03658 , primaryClass =

View on Pith Pith review arXiv
[129]

Copious Amounts of Dust and Gas in a z = 7.5 Quasar Host Galaxy. , keywords =. doi:10.3847/2041-8213/aa943a , archivePrefix =. 1712.01886 , primaryClass =

View on Pith Pith review arXiv
[130]

On the effect of galactic outflows in cosmological simulations of disc galaxies. , keywords =. doi:10.1093/mnras/stx1352 , archivePrefix =. 1705.10325 , primaryClass =

View on Pith Pith review arXiv
[131]

Colour-magnitude diagram in simulations of galaxy formation. , keywords =. doi:10.1093/mnras/sty1896 , archivePrefix =. 1805.00028 , primaryClass =

View on Pith Pith review arXiv
[132]

Chemical evolution of disc galaxies from cosmological simulations. , keywords =. doi:10.1093/mnras/stz492 , archivePrefix =. 1902.05955 , primaryClass =

View on Pith Pith review arXiv 1902
[134]

Simulating realistic disc galaxies with a novel sub-resolution ISM model. , keywords =. doi:10.1093/mnras/stu2400 , adsurl =

View on Pith doi:10.1093/mnras/stu2400
[135]

A JWST/NIRSpec First Census of Broad-line AGNs at z = 4-7: Detection of 10 Faint AGNs with M _ BH 10 ^ 6 - 10 ^ 8 M _ and Their Host Galaxy Properties. , keywords =. doi:10.3847/1538-4357/ad029e , archivePrefix =. 2303.11946 , primaryClass =

View on Pith Pith review arXiv
[136]

A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of z > 6.5 Quasars Using JWST. , keywords =. doi:10.3847/2041-8213/acc9c8 , archivePrefix =. 2304.09888 , primaryClass =

View on Pith Pith review arXiv
[137]

On the physics of dust grains in hot gas. , keywords =. doi:10.1086/157165 , adsurl =

View on Pith doi:10.1086/157165
[138]

Asplund, Martin and Grevesse, Nicolas and Sauval, A. Jacques and Scott, Pat , year=. The Chemical Composition of the Sun , volume=. Annual Review of Astronomy and Astrophysics , publisher=. doi:10.1146/annurev.astro.46.060407.145222 , number=

View on Pith arXiv
[139]

The route to massive black hole formation via merger-driven direct collapse: a review. Reports on Progress in Physics , keywords =. doi:10.1088/1361-6633/aad6a5 , archivePrefix =. 1803.06391 , primaryClass =

View on Pith Pith review arXiv
[141]

Evidence for Low Radiative Efficiency or Highly Obscured Growth of z > 7 Quasars. , keywords =. doi:10.3847/2041-8213/ab42e3 , archivePrefix =. 1906.10130 , primaryClass =

View on Pith Pith review arXiv 1906
[142]

Revealing the Accretion Physics of Supermassive Black Holes at Redshift z 7 with Chandra and Infrared Observations. , keywords =. doi:10.3847/1538-4357/abcc5e , archivePrefix =. 2011.12458 , primaryClass =

View on Pith Pith review arXiv 2011
[143]

An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5. , keywords =. doi:10.1038/nature25180 , archivePrefix =. 1712.01860 , primaryClass =

View on Pith Pith review arXiv
[144]

P \= o niu \= a 'ena: A Luminous z = 7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole. , keywords =. doi:10.3847/2041-8213/ab9c26 , archivePrefix =. 2006.13452 , primaryClass =

View on Pith Pith review arXiv 2006
[145]

A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars. , keywords =. doi:10.3847/2041-8213/ace619 , archivePrefix =. 2303.08918 , primaryClass =

View on Pith Pith review arXiv
[146]

First rest-frame infrared spectrum of a z>7 quasar: JWST/MRS observations of J1120+0641. arXiv e-prints , keywords =. doi:10.48550/arXiv.2307.14414 , archivePrefix =. 2307.14414 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2307.14414
[147]

UNCOVER: The Growth of the First Massive Black Holes from JWST/NIRSpec-Spectroscopic Redshift Confirmation of an X-Ray Luminous AGN at z = 10.1. , keywords =. doi:10.3847/2041-8213/acf7c5 , archivePrefix =. 2308.02750 , primaryClass =

View on Pith Pith review arXiv
[148]

A supermassive black hole in the early universe growing in the shadows. arXiv e-prints , keywords =. doi:10.48550/arXiv.2308.05735 , archivePrefix =. 2308.05735 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2308.05735
[149]

Are we surprised to find SMBHs with JWST at z 9?. , keywords =. doi:10.1093/mnras/stad2503 , archivePrefix =. 2305.12504 , primaryClass =

View on Pith Pith review arXiv
[150]

Exploring the nature of UV-bright z rsim 10 galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?. arXiv e-prints , keywords =. doi:10.48550/arXiv.2305.04944 , archivePrefix =. 2305.04944 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2305.04944
[151]

Very high redshift quasars and the rapid emergence of supermassive black holes. , keywords =. doi:10.1093/mnras/staa2276 , archivePrefix =. 2007.14402 , primaryClass =

View on Pith Pith review arXiv 2007
[152]

The low-end of the black hole mass function at cosmic dawn. , keywords =. doi:10.1093/mnras/stac062 , archivePrefix =. 2201.02630 , primaryClass =

View on Pith Pith review arXiv
[153]

The Rise of Faint, Red Active Galactic Nuclei at z > 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields. , keywords =. doi:10.3847/1538-4357/adbc7d , archivePrefix =. 2404.03576 , primaryClass =

View on Pith Pith review arXiv
[154]

Casey, Caitlin M. and Akins, Hollis B. and Kokorev, Vasily and McKinney, Jed and Cooper, Olivia R. and Long, Arianna S. and Franco, Maximilien and Manning, Sinclaire M. , month = sep, year =. Dust in. doi:10.48550/arXiv.2407.05094 , abstract =

View on Pith Pith review arXiv doi:10.48550/arxiv.2407.05094
[155]

An Upper Limit of 10 ^ 6 M _ in Dust from ALMA Observations in 60 Little Red Dots. , keywords =. doi:10.3847/2041-8213/adfa91 , archivePrefix =. 2505.18873 , primaryClass =

View on Pith Pith review arXiv
[156]

Exploring active galactic nuclei and little red dots with the Obelisk simulation. , keywords =. doi:10.1051/0004-6361/202451963 , archivePrefix =. 2408.12854 , primaryClass =

View on Pith Pith review arXiv
[157]

Little. , author =. 2024 , pages =. doi:10.3847/1538-4357/ad2345 , abstract =

View on Pith doi:10.3847/1538-4357/ad2345 2024
[158]

A population of red candidate massive galaxies. Nature , author =. 2023 , pages =. doi:10.1038/s41586-023-05786-2 , language =

View on Pith doi:10.1038/s41586-023-05786-2 2023
[159]

Labbe, Ivo and Greene, Jenny E. and Bezanson, Rachel and Fujimoto, Seiji and Furtak, Lukas J. and Goulding, Andy D. and Matthee, Jorryt and Naidu, Rohan P. and Oesch, Pascal A. and Atek, Hakim and Brammer, Gabriel and Chemerynska, Iryna and Coe, Dan and Cutler, Sam E. and Dayal, Pratika and Feldmann, Robert and Franx, Marijn and Glazebrook, Karl and Leja,...

View on Pith 2024
[160]

Camps, P. and Baes, M. , urldate =. doi:10.1016/j.ascom.2020.100381 , shorttitle =

View on Pith arXiv 2020
[161]

Baes, M. and Camps, P. , urldate =. doi:10.1016/j.ascom.2015.05.006 , shorttitle =

View on Pith doi:10.1016/j.ascom.2015.05.006 2015
[162]

Camps, P. and Baes, M. , urldate =. doi:10.1016/j.ascom.2014.10.004 , shorttitle =

View on Pith doi:10.1016/j.ascom.2014.10.004 2014
[163]

Infrared emission of z 6 galaxies: AGN imprints. , keywords =. doi:10.1093/mnras/stab528 , archivePrefix =. 2102.08956 , primaryClass =

View on Pith Pith review arXiv
[164]

The dust attenuation law in z 6 quasars. , keywords =. doi:10.1093/mnras/stab1876 , archivePrefix =. 2106.15625 , primaryClass =

View on Pith Pith review arXiv
[165]

Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample. , keywords =. doi:10.1086/518306 , archivePrefix =. astro-ph/0703213 , primaryClass =

View on Pith Pith review arXiv
[166]

Dust Grain-Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud. , keywords =. doi:10.1086/318651 , archivePrefix =. astro-ph/0008146 , primaryClass =

View on Pith Pith review arXiv
[167]

Planck 2015 results. XIII. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201525830 , archivePrefix =. 1502.01589 , primaryClass =

View on Pith Pith review arXiv 2015
[168]

The effect of interstellar matter on climatic variation. Proceedings of the Cambridge Philosophical Society , year = 1939, month = jan, volume =. doi:10.1017/S0305004100021150 , adsurl =

View on Pith doi:10.1017/s0305004100021150 1939
[169]

On the mechanism of accretion by stars. , year = 1944, month = jan, volume =. doi:10.1093/mnras/104.5.273 , adsurl =

View on Pith doi:10.1093/mnras/104.5.273 1944
[171]

Another view into JWST-discovered X-ray weak AGNs via radiative dusty feedback. , keywords =. doi:10.1093/mnras/staf1439 , archivePrefix =. 2509.05423 , primaryClass =

View on Pith Pith review arXiv
[172]

Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion , author=. 2025 , eprint=

View on Pith 2025
[173]

AGN obscuration in optical and X-rays: Host properties and the interplay of nuclear and galactic gas and dust in a combined SDSS–XMM sample , DOI= "10.1051/0004-6361/202558424", url= "https://doi.org/10.1051/0004-6361/202558424", journal =

View on Pith doi:10.1051/0004-6361/202558424
[174]

Bornancini, C. G. and Oio, G. A. and Coldwell, G. , year=. Obscured and unobscured X-ray active galactic nuclei: I. Host-galaxy properties , volume=. doi:10.1051/0004-6361/202554599 , journal=

View on Pith doi:10.1051/0004-6361/202554599
[175]

Chandra Rules Out Super-Eddington Accretion Models for Little Red Dots. , keywords =. doi:10.3847/2041-8213/adf5c8 , archivePrefix =. 2505.09669 , primaryClass =

View on Pith Pith review arXiv
[176]

The X-ray weakness of little red dots and JWST-selected AGN: Comparison with local AGN in different accretion regimes. , keywords =. doi:10.1051/0004-6361/202557444 , archivePrefix =. 2603.10162 , primaryClass =

View on Pith Pith review arXiv
[177]

The X-Ray Dot: Exotic Dust or a Late-stage Little Red Dot?. , keywords =. doi:10.3847/2041-8213/ae4c88 , archivePrefix =. 2601.09778 , primaryClass =

View on Pith arXiv
[178]

Discovery of two little red dots transitioning into quasars , author=. 2025 , eprint=

View on Pith 2025
[179]

Estimating Black Hole Masses in Active Galaxies Using the H Emission Line. , keywords =. doi:10.1086/431897 , archivePrefix =. astro-ph/0508335 , primaryClass =

View on Pith Pith review arXiv
[180]

Type 1 AGN at low z- I. Emission properties. , keywords =. doi:10.1111/j.1365-2966.2012.20901.x , archivePrefix =. 1203.3158 , primaryClass =

View on Pith arXiv 2012
[181]

Richards, Gordon T. and Lacy, Mark and Storrie‐Lombardi, Lisa J. and Hall, Patrick B. and Gallagher, S. C. and Hines, Dean C. and Fan, Xiaohui and Papovich, Casey and Vanden Berk, Daniel E. and Trammell, George B. and Schneider, Donald P. and Vestergaard, Marianne and York, Donald G. and Jester, Sebastian and Anderson, Scott F. and Budavari, Tamas and Sza...

View on Pith doi:10.1086/5
[182]

Dong, Xiaobo and Wang, Tinggui and Wang, Jianguo and Yuan, Weimin and Zhou, Hongyan and Dai, Haifeng and Zhang, Kai , title =. , volume =. 2007 , month =. doi:10.1111/j.1365-2966.2007.12560.x , url =

View on Pith arXiv 2007
[183]

Springel, Volker and di Matteo, Tiziana and Hernquist, Lars , title =. , volume =. 2005 , month =. doi:10.1111/j.1365-2966.2005.09238.x , url =

View on Pith arXiv 2005
[184]

Springel, Volker and Hernquist, Lars , title =. , volume =. 2003 , month =. doi:10.1046/j.1365-8711.2003.06206.x , url =

View on Pith arXiv 2003
[185]

Galactic Stellar and Substellar Initial Mass Function. , keywords =. doi:10.1086/376392 , archivePrefix =. astro-ph/0304382 , primaryClass =

View on Pith Pith review arXiv
[186]

Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs. , keywords =. doi:10.1051/0004-6361/201629228 , archivePrefix =. 1607.00288 , primaryClass =

View on Pith Pith review arXiv
[187]

Nozawa, Takaya and Asano, Ryosuke S. and Hirashita, Hiroyuki and Takeuchi, Tsutomu T. , title =. Monthly Notices of the Royal Astronomical Society: Letters , volume =. 2015 , month =. doi:10.1093/mnrasl/slu175 , url =

View on Pith doi:10.1093/mnrasl/slu175 2015
[188]

Asano, Ryosuke S. and Takeuchi, Tsutomu T. and Hirashita, Hiroyuki and Inoue, Akio K. , title=. Earth, Planets and Space , year=. doi:10.5047/eps.2012.04.014 , url=

View on Pith doi:10.5047/eps.2012.04.014 2012
[189]

Galaxy simulation with dust formation and destruction. , keywords =. doi:10.1093/mnras/stw3061 , archivePrefix =. 1609.07547 , primaryClass =

View on Pith Pith review arXiv
[190]

Ferrara, A. and Viti, S. and Ceccarelli, C. , title =. Monthly Notices of the Royal Astronomical Society: Letters , volume =. 2016 , month =. doi:10.1093/mnrasl/slw165 , url =

View on Pith doi:10.1093/mnrasl/slw165 2016
[191]

No [C II] or dust detection in two Little Red Dots at z _ spec > 7. , keywords =. doi:10.1051/0004-6361/202554361 , archivePrefix =. 2503.01945 , primaryClass =

View on Pith Pith review arXiv
[192]

Evidence of violation of Case B recombination in Little Red Dots. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.06362 , archivePrefix =. 2510.06362 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2510.06362
[193]

Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.00101 , archivePrefix =. 2510.00101 , primaryClass =

View on Pith doi:10.48550/arxiv.2510.00101
[194]

Ji, Xihan and D’Eugenio, Francesco and Juodžbalis, Ignas and Walton, Dominic J and Fabian, Andrew C and Maiolino, Roberto and Ramos Almeida, Cristina and Acosta Pulido, Jose A and Belokurov, Vasily A and Isobe, Yuki and Jones, Gareth and Maraston, Claudia and Scholtz, Jan and Simmonds, Charlotte and Tacchella, Sandro and Terlevich, Elena and Terlevich, Ro...

View on Pith doi:10.1093/mnras/staf2235 2026
[195]

The Discovery of Little Red Dots in the Local Universe: Signatures of Cool Gas Envelopes. , keywords =. doi:10.3847/1538-4357/ae2bdf , archivePrefix =. 2507.10659 , primaryClass =

View on Pith arXiv
[196]

The Cliff: a metal-poor little red dot hosting an overmassive black hole at z = 3.55. , keywords =. doi:10.1093/mnras/stag1220 , archivePrefix =. 2604.09177 , primaryClass =

View on Pith Pith review arXiv
[197]

Is GRB 050904 at z = 6.3 absorbed by dust? , DOI= "10.1051/0004-6361/201016414", url= "https://doi.org/10.1051/0004-6361/201016414", journal =

View on Pith doi:10.1051/0004-6361/201016414
[198]

Hirashita, Hiroyuki and Aoyama, Shohei , title =. , volume =. 2019 , month =. doi:10.1093/mnras/sty2838 , url =

View on Pith doi:10.1093/mnras/sty2838 2019
[199]

Hirashita, Hiroyuki and Nozawa, Takaya and Villaume, Alexa and Srinivasan, Sundar , title =. , volume =. 2015 , month =. doi:10.1093/mnras/stv2095 , url =

View on Pith Pith review doi:10.1093/mnras/stv2095 2015
[200]

What determines the grain size distribution in galaxies?. , keywords =. doi:10.1093/mnras/stt506 , archivePrefix =. 1303.5528 , primaryClass =

View on Pith Pith review arXiv
[201]

Stellar sources of dust in the high-redshift Universe. , keywords =. doi:10.1111/j.1365-2966.2009.15076.x , archivePrefix =. 0905.1691 , primaryClass =

View on Pith arXiv 2009
[202]

Hjorth, Jens and Vreeswijk, Paul M. and Gall, Christa and Watson, Darach , title =. , abstract =. 2013 , month =. doi:10.1088/0004-637X/768/2/173 , url =

View on Pith doi:10.1088/0004-637x/768/2/173 2013
[203]

Zafar, T and Møller, P and Watson, D and Lattanzio, J and Hopkins, A M and Karakas, A and Fynbo, J P U and Tanvir, N R and Selsing, J and Jakobsson, P and Heintz, K E and Kann, D A and Groves, B and Kulkarni, V and Covino, S and D’Elia, V and Japelj, J and Corre, D and Vergani, S , title =. , volume =. 2018 , month =. doi:10.1093/mnras/sty1876 , url =

View on Pith doi:10.1093/mnras/sty1876 2018
[204]

Zafar, T. and Watson, D. and Fynbo, J. P. U. and Malesani, D. and Jakobsson, P. and de Ugarte Postigo, A. , year=. The extinction curves of star-forming regions from<i>z</i> = 0.1 to 6.7 using GRB afterglow spectroscopy , volume=. doi:10.1051/0004-6361/201116663 , journal=

View on Pith doi:10.1051/0004-6361/201116663
[205]

Li, Zhengrong and Inayoshi, Kohei and Chen, Kejian and Ichikawa, Kohei and Ho, Luis C. , title =. , abstract =. 2025 , month =. doi:10.3847/1538-4357/ada5fb , url =

View on Pith doi:10.3847/1538-4357/ada5fb 2025
[206]

Chen, Kejian and Li, Zhengrong and Inayoshi, Kohei and Ho, Luis C. , title =. , abstract =. 2025 , month =. doi:10.3847/2041-8213/ae1955 , url =

View on Pith doi:10.3847/2041-8213/ae1955 2025
[207]

Extinction due to amorphous carbon grains in red quasars from the Sloan Digital Sky Survey. , keywords =. doi:10.1111/j.1365-2966.2004.07590.x , archivePrefix =. astro-ph/0401158 , primaryClass =

View on Pith arXiv 2004
[208]

Gaskell, C. Martin and Goosmann, René W. and Antonucci, Robert R. J. and Whysong, David H. , title =. , abstract =. 2004 , month =. doi:10.1086/423885 , url =

View on Pith doi:10.1086/423885 2004
[209]

Gallerani, S. and Maiolino, R. and Juarez, Y. and Nagao, T. and Marconi, A. and Bianchi, S. and Schneider, R. and Mannucci, F. and Oliva, T. and Willott, C. J. and Jiang, L. and Fan, X. , year=. The extinction law at high redshift and its implications , volume=. doi:10.1051/0004-6361/201014721 , journal=

View on Pith doi:10.1051/0004-6361/201014721
[210]

What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition. , keywords =. doi:10.3847/1538-4357/ad38bb , archivePrefix =. 2401.08782 , primaryClass =

View on Pith Pith review arXiv
[211]

COSMOS-Web: The Overabundance and Physical Nature of ``Little Red Dots'' Implications for Early Galaxy and SMBH Assembly. , keywords =. doi:10.3847/1538-4357/ade984 , archivePrefix =. 2406.10341 , primaryClass =

View on Pith Pith review arXiv
[212]

The Galaxies Missed by Hubble and ALMA: The Contribution of Extremely Red Galaxies to the Cosmic Census at 3 < z < 8. , keywords =. doi:10.3847/1538-4357/ad3f17 , archivePrefix =. 2311.07483 , primaryClass =

View on Pith Pith review arXiv
[213]

Exploring the Nature of Little Red Dots: Constraints on Active Galactic Nucleus and Stellar Contributions from PRIMER MIRI Imaging. , keywords =. doi:10.3847/1538-4357/adfcce , archivePrefix =. 2411.12005 , primaryClass =

View on Pith Pith review arXiv
[214]

RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow. , keywords =. doi:10.3847/1538-4357/adc1ca , archivePrefix =. 2403.02304 , primaryClass =

View on Pith Pith review arXiv
[215]

MIDIS: MIRI Uncovers Virgil, the First Little Red Dot with Clear Detection of Its Host Galaxy at z ≃ 6.6. , keywords =. doi:10.3847/1538-4357/ade5a6 , archivePrefix =. 2406.18207 , primaryClass =

View on Pith Pith review arXiv
[216]

Setton, David J. and Greene, Jenny E. and Spilker, Justin S. and Williams, Christina C. and Labbé, Ivo and Ma, Yilun and Wang, Bingjie and Whitaker, Katherine E. and Leja, Joel and de Graaff, Anna and Alberts, Stacey and Bezanson, Rachel and Boogaard, Leindert A. and Brammer, Gabriel and Cutler, Sam E. and Cleri, Nikko J. and Cooper, Olivia R. and Dayal, ...

View on Pith 2025
[217]

A Comprehensive Photometric Selection of ``Little Red Dots'' in MIRI Fields: An Infrared-Bright Little Red Dot at z = 3.1386 with Warm Dust Emission. , keywords =. doi:10.3847/1538-4357/ae0704 , archivePrefix =. 2412.01887 , primaryClass =

View on Pith Pith review arXiv
[218]

Hviding, Raphael E. and de Graaff, Anna and Miller, Tim B. and Setton, David J. and Greene, Jenny E. and Labbé, Ivo and Brammer, Gabriel and Bezanson, Rachel and Boogaard, Leindert A. and Cleri, Nikko J. and Leja, Joel and Maseda, Michael V. and McConachie, Ian and Matthee, Jorryt and Naidu, Rohan P. and Oesch, Pascal A. and Wang, Bingjie and Whitaker, Ka...

View on Pith
[219]

A. , author =. 2024 , note =. doi:10.3847/1538-4357/ad4265 , abstract =

View on Pith doi:10.3847/1538-4357/ad4265 2024
[220]

, author =. 2024 , note =. doi:10.3847/1538-4357/ad1e5f , abstract =

View on Pith doi:10.3847/1538-4357/ad1e5f 2024
[221]

A remarkable ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a little red dot at z = 3.5. , keywords =. doi:10.1051/0004-6361/202554681 , archivePrefix =. 2503.16600 , primaryClass =

View on Pith Pith review arXiv
[222]

The Engine and its Flows: Little Red Dot spectra are shaped by the column densities of their gas envelopes. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.17667 , archivePrefix =. 2603.17667 , primaryClass =

View on Pith doi:10.48550/arxiv.2603.17667
[223]

UNCOVER: 404 Error Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1. , keywords =. doi:10.3847/1538-4357/ada613 , archivePrefix =. 2410.06257 , primaryClass =

View on Pith Pith review arXiv
[224]

RUBIES: Evolved Stellar Populations with Extended Formation Histories at z 7─8 in Candidate Massive Galaxies Identified with JWST/NIRSpec. , keywords =. doi:10.3847/2041-8213/ad55f7 , archivePrefix =. 2405.01473 , primaryClass =

View on Pith Pith review arXiv
[225]

Ji, Xihan and Maiolino, Roberto and Übler, Hannah and Scholtz, Jan and D’Eugenio, Francesco and Sun, Fengwu and Perna, Michele and Turner, Hannah and Carniani, Stefano and Arribas, Santiago and Bennett, Jake S and Bunker, Andrew and Charlot, Stéphane and Cresci, Giovanni and Curti, Mirko and Egami, Eiichi and Fabian, Andy and Inayoshi, Kohei and Isobe, Yu...

View on Pith 2025
[226]

A gas-enshrouded and gas-reddened black hole at cosmic dawn. , keywords =. doi:10.1038/s41586-026-10846-4 , archivePrefix =. 2503.16596 , primaryClass =

View on Pith Pith review arXiv
[227]

Extremely. , author =. 2025 , note =. doi:10.3847/2041-8213/adaebd , abstract =

View on Pith doi:10.3847/2041-8213/adaebd 2025
[228]

An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy. arXiv e-prints , keywords =. doi:10.48550/arXiv.2412.04557 , archivePrefix =. 2412.04557 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2412.04557
[229]

Setton, David J. and Greene, Jenny E. and de Graaff, Anna and Ma, Yilun and Leja, Joel and Matthee, Jorryt and Bezanson, Rachel and Boogaard, Leindert A. and Cleri, Nikko J. and Katz, Harley and Labbe, Ivo and Maseda, Michael V. and McConachie, Ian and Miller, Tim B. and Price, Sedona H. and Suess, Katherine A. and van Dokkum, Pieter and Wang, Bingjie and...

View on Pith doi:10.3847/1538-4357/ae1500 2025
[230]

Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies. , keywords =. doi:10.1146/annurev-astro-082708-101811 , archivePrefix =. 1304.7762 , primaryClass =

View on Pith Pith review arXiv
[231]

GA-NIFS: A massive black hole in a low-metallicity AGN at z 5.55 revealed by JWST/NIRSpec IFS. , keywords =. doi:10.1051/0004-6361/202346137 , archivePrefix =. 2302.06647 , primaryClass =

View on Pith Pith review arXiv
[232]

Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS. , keywords =. doi:10.3847/2041-8213/ace5a0 , archivePrefix =. 2302.00012 , primaryClass =

View on Pith Pith review arXiv
[233]

Little Red and Blue Dots: simply stratified Broad Line Regions. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.22277 , archivePrefix =. 2603.22277 , primaryClass =

View on Pith doi:10.48550/arxiv.2603.22277
[234]

Rinaldi, P. and Bonaventura, N. and Rieke, G. H. and Alberts, S. and Caputi, K. I. and Baker, W. M. and Baum, S. and Bhatawdekar, R. and Bunker, A. J. and Carniani, S. and Curtis-Lake, E. and D’Eugenio, F. and Egami, E. and Ji, Z. and Johnson, B. D. and Hainline, K. and Helton, J. M. and Lin, X. and Lyu, J. and Ma, Z. and Maiolino, R. and Pérez-González, ...

View on Pith 2025
[235]

The Small Sizes and High Implied Densities of ``Little Red Dots'' with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus. , keywords =. doi:10.3847/2041-8213/ad90b8 , archivePrefix =. 2408.07745 , primaryClass =

View on Pith Pith review arXiv
[236]

Hidden in Pixels. I. Discovery of dual ``little red dots'' indicates excess clustering on kilo-parsec scales. arXiv e-prints , keywords =. doi:10.48550/arXiv.2412.14246 , archivePrefix =. 2412.14246 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2412.14246
[237]

Sizes and Mass Profiles of Candidate Massive Galaxies Discovered by JWST at 7 < z < 9: Evidence for Very Early Formation of the Central 100 pc of Present-day Ellipticals. , keywords =. doi:10.3847/2041-8213/acf5ef , archivePrefix =. 2305.17162 , primaryClass =

View on Pith Pith review arXiv
[238]

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383. , keywords =. doi:10.3847/2041-8213/ae82fe , archivePrefix =. 2512.03239 , primaryClass =

View on Pith Pith review arXiv
[239]

Possible environmental quenching in an interacting little red dot pair at z 7. , keywords =. doi:10.1051/0004-6361/202553943 , archivePrefix =. 2501.17925 , primaryClass =

View on Pith Pith review arXiv
[240]

A Deep Dive down the Broad-line Region: Permitted O I, Ca II, and Fe II Emission in an Active Galactic Nucleus Little Red Dot at z = 5.3. , keywords =. doi:10.3847/2041-8213/ae13a9 , archivePrefix =. 2507.20684 , primaryClass =

View on Pith arXiv
[241]

A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling. arXiv e-prints , keywords =. doi:10.48550/arXiv.2605.30414 , archivePrefix =. 2605.30414 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2605.30414
[242]

Extreme properties of a compact and massive accreting black hole host in the first 500 Myr. Nature Communications , keywords =. doi:10.1038/s41467-025-65070-x , archivePrefix =. 2412.04983 , primaryClass =

View on Pith Pith review arXiv
[243]

JADES and BlackTHUNDER: rest-frame Balmer-line absorption and the local environment in a Little Red Dot at z = 5. , keywords =. doi:10.1093/mnras/staf2117 , archivePrefix =. 2506.14870 , primaryClass =

View on Pith arXiv
[244]

A weak Ly halo for an extremely bright little red dot: Indications of enshrouded supermassive black hole growth. , keywords =. doi:10.1051/0004-6361/202555596 , archivePrefix =. 2505.09542 , primaryClass =

View on Pith arXiv
[245]

VENUS: Two Faint Little Red Dots Separated by 70\,pc Hidden in a Single Lensed Galaxy at z 7. arXiv e-prints , keywords =. doi:10.48550/arXiv.2601.06015 , archivePrefix =. 2601.06015 , primaryClass =

View on Pith doi:10.48550/arxiv.2601.06015
[246]

Connecting the Dots: UV-bright Companions of Little Red Dots as Lyman─Werner Sources Enabling Direct-collapse Black Hole Formation. , keywords =. doi:10.3847/2041-8213/ae58a5 , archivePrefix =. 2602.02702 , primaryClass =

View on Pith Pith review arXiv
[247]

Beyond the Dot: An LRD-like Nucleus at the Heart of an IR-bright Galaxy and its Implications for High-redshift LRDs. , keywords =. doi:10.3847/1538-4357/ae80cd , archivePrefix =. 2507.17738 , primaryClass =

View on Pith Pith review arXiv
[248]

A high black-hole-to-host mass ratio in a lensed AGN in the early Universe. , keywords =. doi:10.1038/s41586-024-07184-8 , archivePrefix =. 2308.05735 , primaryClass =

View on Pith Pith review arXiv
[249]

Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13. , keywords =. doi:10.3847/1538-4357/ad7d03 , archivePrefix =. 2407.20320 , primaryClass =

View on Pith Pith review arXiv
[250]

Juodžbalis, Ignas and Marconcini, Cosimo and D’Eugenio, Francesco and Maiolino, Roberto and Marconi, Alessandro and Übler, Hannah and Scholtz, Jan and Ji, Xihan and Jones, Gareth C. and Perna, Michele and Arribas, Santiago and Bennett, Jake S. and Bromm, Volker and Bunker, Andrew J. and Carniani, Stefano and Charlot, Stéphane and Cresci, Giovanni and Daya...

View on Pith
[251]

Pacucci, Fabio and Narayan, Ramesh , year=. Mildly Super-Eddington Accretion onto Slowly Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots , volume=. , publisher=. doi:10.3847/1538-4357/ad84f7 , number=

View on Pith doi:10.3847/1538-4357/ad84f7
[252]

On the quenching of LRD X-ray emission by both Compton-thick gas and high accretion rates , author=. 2026 , eprint=

View on Pith 2026
[253]

Stacking. , author =. 2024 , note =. doi:10.3847/2041-8213/ad7eba , abstract =

View on Pith doi:10.3847/2041-8213/ad7eba 2024
[254]

Preparing Red-Green-Blue Images from CCD Data. , keywords =. doi:10.1086/382245 , archivePrefix =. astro-ph/0312483 , primaryClass =

View on Pith Pith review arXiv
[255]

JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe. , keywords =. doi:10.1093/mnras/staf359 , archivePrefix =. 2405.00504 , primaryClass =

View on Pith Pith review arXiv
[256]

X-Ray Weak Active Galactic Nuclei from Super-Eddington Accretion onto Infant Black Holes. , keywords =. doi:10.3847/2041-8213/ad90e1 , archivePrefix =. 2410.00417 , primaryClass =

View on Pith Pith review arXiv
[257]

Do little red dots really form a distinct class of astronomical objects?. arXiv e-prints , keywords =. doi:10.48550/arXiv.2604.11677 , archivePrefix =. 2604.11677 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2604.11677
[258]

Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST. , keywords =. doi:10.3847/1538-4357/acef21 , archivePrefix =. 2304.12347 , primaryClass =

View on Pith Pith review arXiv
[259]

UNCOVER: A NIRSpec Identification of a Broad-line AGN at z = 8.50. , keywords =. doi:10.3847/2041-8213/ad037a , archivePrefix =. 2308.11610 , primaryClass =

View on Pith Pith review arXiv
[260]

Extremely Red Galaxies at z = 5─9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?. , keywords =. doi:10.3847/1538-4357/ad167e , archivePrefix =. 2305.14418 , primaryClass =

View on Pith Pith review arXiv
[261]

A. , author =. 2023 , note =. doi:10.3847/2041-8213/aca9d3 , abstract =

View on Pith doi:10.3847/2041-8213/aca9d3 2023
[262]

JWST UNCOVER: Extremely Red and Compact Object at z _ phot ≃ 7.6 Triply Imaged by A2744. , keywords =. doi:10.3847/1538-4357/acdc9d , archivePrefix =. 2212.10531 , primaryClass =

View on Pith Pith review arXiv
[263]

Counting Little Red Dots at z < 4 with Ground-based Surveys and Spectroscopic Follow-up. , keywords =. doi:10.3847/1538-4357/ae4596 , archivePrefix =. 2504.08032 , primaryClass =

View on Pith Pith review arXiv
[264]

Super-Eddington Accretion of Black Holes in Early Nuclear Bursts Gives Birth to Little Red Dots. , keywords =. doi:10.3847/2041-8213/ae909e , archivePrefix =. 2605.31077 , primaryClass =

View on Pith Pith review arXiv
[265]

Zhuang, Ming-Yang and Li, Junyao and Shen, Yue and Lin, Xiaojing and Shapley, Alice E. and Wang, Feige and Wu, Qiaoya and Yang, Qian , title =. , abstract =. 2026 , month =. doi:10.3847/1538-4357/ae3612 , url =

View on Pith doi:10.3847/1538-4357/ae3612 2026
[266]

Discovery of a Little Red Dot candidate at z 10 in COSMOS-Web based on MIRI-NIRCam selection , author=. 2025 , eprint=

View on Pith 2025
[267]

The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time. arXiv e-prints , keywords =. doi:10.48550/arXiv.2604.07138 , archivePrefix =. 2604.07138 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2604.07138
[268]

(LRDs) ^2 : The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample. arXiv e-prints , keywords =. doi:10.48550/arXiv.2605.21574 , archivePrefix =. 2605.21574 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2605.21574
[269]

Little Red Dots as the Very First Activity of Black Hole Growth. , keywords =. doi:10.3847/2041-8213/adea66 , archivePrefix =. 2503.05537 , primaryClass =

View on Pith Pith review arXiv
[270]

X-Ray View of Little Red Dots: Do They Host Supermassive Black Holes?. , keywords =. doi:10.3847/2041-8213/ad5669 , archivePrefix =. 2404.19010 , primaryClass =

View on Pith Pith review arXiv
[271]

Furtak, Lukas J. and Secunda, Amy R. and Greene, Jenny E. and Zitrin, Adi and Labbé, Ivo and Golubchik, Miriam and Bezanson, Rachel and Kokorev, Vasily and Atek, Hakim and Brammer, Gabriel B. and Chemerynska, Iryna and Cutler, Sam E. and Dayal, Pratika and Feldmann, Robert and Fujimoto, Seiji and Glazebrook, Karl and Leja, Joel and Ma, Yilun and Matthee, ...

View on Pith
[272]

Kokubo, Mitsuru and Harikane, Yuichi , title =. , abstract =. 2025 , month =. doi:10.3847/1538-4357/ae119e , url =

View on Pith doi:10.3847/1538-4357/ae119e 2025
[273]

The GlimmIr: Spectroscopic Variability in a z 7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions , author=. 2026 , eprint=

View on Pith 2026
[274]

Zhang, Zijian and Jiang, Linhua and Liu, Weiyang and Ho, Luis C. , title =. , abstract =. 2025 , month =. doi:10.3847/1538-4357/adcb3e , url =

View on Pith doi:10.3847/1538-4357/adcb3e 2025
[275]

Jiang, Linhua and Fan, Xiaohui and Brandt, W. N. and Carilli, Chris L. and Egami, Eiichi and Hines, Dean C. and Kurk, Jaron D. and Richards, Gordon T. and Shen, Yue and Strauss, Michael A. and Vestergaard, Marianne and Walter, Fabian , year=. Dust-free quasars in the early Universe , volume=. Nature , publisher=. doi:10.1038/nature08877 , number=

View on Pith doi:10.1038/nature08877
[276]

Lyu, Jianwei and Rieke, G. H. and Shi, Yong , title =. , abstract =. 2017 , month =. doi:10.3847/1538-4357/835/2/257 , url =

View on Pith doi:10.3847/1538-4357/835/2/257 2017
[277]

The spectral energy distributions of active galactic nuclei. , keywords =. doi:10.1093/mnras/stz2324 , archivePrefix =. 1908.03720 , primaryClass =

View on Pith Pith review arXiv 1908
[278]

Son, Suyeon and Kim, Minjin and Ho, Luis C. , title =. , abstract =. 2023 , month =. doi:10.3847/1538-4357/ace165 , url =

View on Pith doi:10.3847/1538-4357/ace165 2023
[279]

Lyu, Jianwei and Rieke, George , year=. Infrared Spectral Energy Distribution and Variability of Active Galactic Nuclei: Clues to the Structure of Circumnuclear Material , volume=. Universe , publisher=. doi:10.3390/universe8060304 , number=

View on Pith doi:10.3390/universe8060304
[280]

FORGE'd in FIRE: Resolving the End of Star Formation and Structure of AGN Accretion Disks from Cosmological Initial Conditions. The Open Journal of Astrophysics , keywords =. doi:10.21105/astro.2309.13115 , archivePrefix =. 2309.13115 , primaryClass =

View on Pith arXiv
[281]

High-redshift clumpy discs and bulges in cosmological simulations. , keywords =. doi:10.1111/j.1365-2966.2010.16433.x , archivePrefix =. 0907.3271 , primaryClass =

View on Pith arXiv 2010
[282]

Hot-dust-poor Type 1 Active Galactic Nuclei in the COSMOS Survey. , keywords =. doi:10.1088/2041-8205/724/1/L59 , archivePrefix =. 1009.3276 , primaryClass =

View on Pith Pith review arXiv
[283]

Lyu, Jianwei and Alberts, Stacey and Rieke, George H. and Shivaei, Irene and Pérez-González, Pablo G. and Sun, Fengwu and Hainline, Kevin N. and Baum, Stefi and Bonaventura, Nina and Bunker, Andrew J. and Egami, Eiichi and Eisenstein, Daniel J. and Florian, Michael and Ji, Zhiyuan and Johnson, Benjamin D. and Morrison, Jane and Rieke, Marcia and Robertson...

View on Pith 2024
[284]

Molecular Gas in z -0.5ex 6 Quasar Host Galaxies. , keywords =. doi:10.1088/0004-637X/714/1/699 , archivePrefix =. 1002.1561 , primaryClass =

View on Pith Pith review arXiv
[285]

Enhanced star formation in z 6 quasar companions. , keywords =. doi:10.1093/mnras/stac978 , archivePrefix =. 2204.03658 , primaryClass =

View on Pith Pith review arXiv
[286]

HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars. , keywords =. doi:10.1051/0004-6361/202346795 , archivePrefix =. 2305.02347 , primaryClass =

View on Pith Pith review arXiv
[287]

HYPERION. Shedding light on the first luminous quasars: A correlation between UV disc winds and X-ray continuum. , keywords =. doi:10.1051/0004-6361/202449662 , archivePrefix =. 2410.12786 , primaryClass =

View on Pith arXiv
[288]

Systematic broad-band X-ray study of super-Eddington accretion on to supermassive black holes - I. X-ray continuum. , keywords =. doi:10.1093/mnras/stac3590 , archivePrefix =. 2212.06183 , primaryClass =

View on Pith Pith review arXiv
[289]

The extreme properties of the nearby hyper-Eddington accreting active galactic nucleus in IRAS 04416+1215. , keywords =. doi:10.1093/mnras/stab3152 , archivePrefix =. 2109.02573 , primaryClass =

View on Pith Pith review arXiv
[290]

An Investigation into the Selection and Colors of Little Red Dots and Active Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/ad9920 , archivePrefix =. 2410.00100 , primaryClass =

View on Pith Pith review arXiv
[291]

Tee, Wei Leong and Fan, Xiaohui and Wang, Feige and Yang, Jinyi , title =. , abstract =. 2025 , month =. doi:10.3847/2041-8213/adc5e3 , url =

View on Pith doi:10.3847/2041-8213/adc5e3 2025
[292]

The Sloan Digital Sky Survey: Technical Summary. , keywords =. doi:10.1086/301513 , archivePrefix =. astro-ph/0006396 , primaryClass =

View on Pith Pith review arXiv
[293]

Composite Quasar Spectra from the Sloan Digital Sky Survey. , keywords =. doi:10.1086/321167 , archivePrefix =. astro-ph/0105231 , primaryClass =

View on Pith Pith review arXiv
[294]

Glikman, Eilat and Helfand, David J. and White, Richard L. , title =. , abstract =. 2006 , month =. doi:10.1086/500098 , url =

View on Pith doi:10.1086/500098 2006
[295]

CIGALE: a python Code Investigating GALaxy Emission⋆ , DOI= "10.1051/0004-6361/201834156", url= "https://doi.org/10.1051/0004-6361/201834156", journal =

View on Pith Pith review doi:10.1051/0004-6361/201834156
[296]

Fitting AGN/Galaxy X-Ray-to-radio SEDs with CIGALE and Improvement of the Code. , keywords =. doi:10.3847/1538-4357/ac4971 , archivePrefix =. 2201.03718 , primaryClass =

View on Pith Pith review arXiv
[297]

Yang(杨光), G and Boquien, M and Buat, V and Burgarella, D and Ciesla, L and Duras, F and Stalevski, M and Brandt, W N and Papovich, C , title =. , volume =. 2020 , month =. doi:10.1093/mnras/stz3001 , url =

View on Pith Pith review doi:10.1093/mnras/stz3001 2020
[298]

Stalevski, Marko and Fritz, Jacopo and Baes, Maarten and Nakos, Theodoros and Popovi. 3D radiative transfer modelling of the dusty tori around active galactic nuclei as a clumpy two-phase medium , journal =. 2012 , month =. doi:10.1111/j.1365-2966.2011.19775.x , url =

View on Pith arXiv 2012
[299]

Stalevski, Marko and Ricci, Claudio and Ueda, Yoshihiro and Lira, Paulina and Fritz, Jacopo and Baes, Maarten , title =. , volume =. 2016 , month =. doi:10.1093/mnras/stw444 , url =

View on Pith doi:10.1093/mnras/stw444 2016
[300]

The first billion years according to JWST. Nature Astronomy , keywords =. doi:10.1038/s41550-025-02624-5 , archivePrefix =. 2405.21054 , primaryClass =

View on Pith Pith review arXiv

Discussion

Disagree with the review, or know something it missed? Leave a comment, highlight any passage above to comment on it, or challenge this review formally.

[1] [1]

Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model. arXiv e-prints , keywords =. doi:10.48550/arXiv.2602.22386 , archivePrefix =. 2602.22386 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2602.22386

[2] [2]

You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei. , keywords =. doi:10.1051/0004-6361/202659544 , adsurl =

View on Pith doi:10.1051/0004-6361/202659544

[3] [3]

Ionizing Photon Production Efficiencies and Chemical Abundances at Cosmic Dawn Revealed by Ultradeep Rest-frame Optical Spectroscopy of JADES-GS-z14-0. , keywords =. doi:10.3847/2041-8213/ae7446 , archivePrefix =. 2512.19695 , primaryClass =

View on Pith arXiv

[4] [4]

The Atmospheric Structure of the O-Type Giant Krzeminski's Star and the Mass of its Companion Neutron Star Centaurus X-3. , keywords =. doi:10.1086/165954 , adsurl =

View on Pith doi:10.1086/165954

[5] [5]

Too many or too massive? Investigating the high-z demography of active SMBHs from JWST. , keywords =. doi:10.1093/mnras/stag223 , archivePrefix =. 2601.23250 , primaryClass =

View on Pith arXiv

[6] [6]

A Selection Aware View of Black Hole-Galaxy Coevolution at High Redshift. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.04358 , archivePrefix =. 2603.04358 , primaryClass =

View on Pith doi:10.48550/arxiv.2603.04358

[7] [7]

Active galactic nuclei-heated dust revealed in ``little red dots''. , keywords =. doi:10.1051/0004-6361/202557164 , archivePrefix =. 2509.07100 , primaryClass =

View on Pith arXiv

[8] [8]

What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots. , keywords =. doi:10.3847/1538-4357/ae1836 , archivePrefix =. 2509.05434 , primaryClass =

View on Pith Pith review arXiv

[9] [9]

From ``The Cliff'' to ``Virgil'': Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec. , keywords =. doi:10.3847/1538-4357/ae5d2c , archivePrefix =. 2512.15853 , primaryClass =

View on Pith arXiv

[10] [10]

Radiative Transfer in Circumstellar Dust Clouds. Interstellar Dust and Related Topics , year = 1973, editor =

View on Pith 1973

[11] [11]

Astrophysics of gaseous nebulae and active galactic nuclei

View on Pith

[12] [12]

Analytical Approximations for Calculating the Escape and Absorption of Radiation in Clumpy Dusty Environments. , keywords =. doi:10.1086/307729 , archivePrefix =. astro-ph/9905029 , primaryClass =

View on Pith Pith review arXiv

[13] [13]

'Little red dots' cannot reside in the same dark matter haloes as comparably luminous unobscured quasars. , keywords =. doi:10.1093/mnras/staf660 , archivePrefix =. 2409.18208 , primaryClass =

View on Pith Pith review arXiv

[14] [14]

Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe. arXiv e-prints , keywords =. doi:10.48550/arXiv.2402.18773 , archivePrefix =. 2402.18773 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2402.18773

[15] [15]

Seeking the growth of the first black hole seeds with JWST. , keywords =. doi:10.1093/mnras/stac3768 , archivePrefix =. 2211.01389 , primaryClass =

View on Pith Pith review arXiv

[16] [16]

Comparing Single-epoch Virial Black Hole Mass Estimators for Luminous Quasars. , keywords =. doi:10.1088/0004-637X/753/2/125 , archivePrefix =. 1203.0601 , primaryClass =

View on Pith Pith review arXiv

[17] [17]

A small and vigorous black hole in the early Universe. arXiv e-prints , keywords =. doi:10.48550/arXiv.2305.12492 , archivePrefix =. 2305.12492 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2305.12492

[18] [18]

Sustained super-Eddington accretion in high-redshift quasars. arXiv e-prints , keywords =. doi:10.48550/arXiv.2312.08422 , archivePrefix =. 2312.08422 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2312.08422

[19] [19]

XQR-30: The ultimate XSHOOTER quasar sample at the reionization epoch. , keywords =. doi:10.1093/mnras/stad1468 , archivePrefix =. 2305.05053 , primaryClass =

View on Pith Pith review arXiv

[20] [20]

The growth efficiency of high-redshift black holes. , keywords =. doi:10.1093/mnras/stv1465 , archivePrefix =. 1506.04750 , primaryClass =

View on Pith Pith review arXiv

[21] [21]

Super-Eddington growth of the first black holes. , keywords =. doi:10.1093/mnras/stw505 , archivePrefix =. 1603.00475 , primaryClass =

View on Pith Pith review arXiv

[22] [22]

Mass Functions of the Active Black Holes in Distant Quasars from the Large Bright Quasar Survey, the Bright Quasar Survey, and the Color-selected Sample of the SDSS Fall Equatorial Stripe. , keywords =. doi:10.1088/0004-637X/699/1/800 , archivePrefix =. 0904.3348 , primaryClass =

View on Pith Pith review arXiv

[23] [23]

A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 7. , keywords =. doi:10.1088/0067-0049/194/2/45 , archivePrefix =. 1006.5178 , primaryClass =

View on Pith Pith review arXiv

[24] [24]

The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars. , keywords =. doi:10.3847/1538-4357/ac9626 , archivePrefix =. 2207.05113 , primaryClass =

View on Pith Pith review arXiv

[25] [25]

Galactic winds in cosmological simulations of the circumgalactic medium. , keywords =. doi:10.1093/mnras/stt125 , archivePrefix =. 1210.3582 , primaryClass =

View on Pith Pith review arXiv

[26] [26]

Host galaxies of high-redshift quasars: SMBH growth and feedback. , keywords =. doi:10.1093/mnras/stab1992 , archivePrefix =. 2107.05638 , primaryClass =

View on Pith Pith review arXiv

[27] [27]

On spherically symmetrical accretion. , year = 1952, month = jan, volume =. doi:10.1093/mnras/112.2.195 , adsurl =

View on Pith doi:10.1093/mnras/112.2.195 1952

[28] [28]

JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr after the Big Bang. , keywords =. doi:10.3847/1538-4357/acdbc6 , archivePrefix =. 2302.07234 , primaryClass =

View on Pith Pith review arXiv

[29] [29]

Statistics of extremes , author=. 1958 , publisher=

View on Pith 1958

[30] [30]

Extreme value distributions: theory and applications , author=. 2000 , publisher=

View on Pith 2000

[31] [31]

Table for estimating the goodness of fit of empirical distributions , author=. The annals of mathematical statistics , volume=. 1948 , publisher=

View on Pith 1948

[32] [32]

Two Remarkably Luminous Galaxy Candidates at z 10-12 Revealed by JWST. , keywords =. doi:10.3847/2041-8213/ac9b22 , archivePrefix =. 2207.09434 , primaryClass =

View on Pith Pith review arXiv

[33] [33]

Large-scale bias and the peak background split. , keywords =. doi:10.1046/j.1365-8711.1999.02692.x , archivePrefix =. astro-ph/9901122 , primaryClass =

View on Pith arXiv 1999

[34] [34]

JADES NIRSpec Spectroscopy of GN-z11: Lyman- emission and possible enhanced nitrogen abundance in a z = 10.60 luminous galaxy. , keywords =. doi:10.1051/0004-6361/202346159 , archivePrefix =. 2302.07256 , primaryClass =

View on Pith Pith review arXiv

[35] [35]

Planck 2018 results. VI. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201833910 , archivePrefix =. 1807.06209 , primaryClass =

View on Pith Pith review arXiv 2018

[36] [36]

On the stunning abundance of super-early, luminous galaxies revealed by JWST. , keywords =. doi:10.1093/mnras/stad1095 , archivePrefix =. 2208.00720 , primaryClass =

View on Pith Pith review arXiv

[37] [37]

Essential physics of early galaxy formation. , keywords =. doi:10.1093/mnras/stu1848 , archivePrefix =. 1405.4862 , primaryClass =

View on Pith Pith review arXiv

[38] [38]

How the super-Eddington regime regulates black hole growth in high-redshift galaxies. , keywords =. doi:10.1051/0004-6361/202243170 , archivePrefix =. 2201.08766 , primaryClass =

View on Pith Pith review arXiv

[39] [39]

XQR-30: Black hole masses and accretion rates of 42 z 6 quasars. , keywords =. doi:10.1051/0004-6361/202346317 , archivePrefix =. 2306.16474 , primaryClass =

View on Pith Pith review arXiv

[40] [40]

The Internal Constitution of the Stars

View on Pith

[41] [41]

Euclid preparation. V. Predicted yield of redshift 7 < z < 9 quasars from the wide survey. , keywords =. doi:10.1051/0004-6361/201936427 , archivePrefix =. 1908.04310 , primaryClass =

View on Pith Pith review arXiv 1908

[42] [42]

Kinetic and radiative power from optically thin accretion flows. , keywords =. doi:10.1093/mnras/stx543 , archivePrefix =. 1701.07033 , primaryClass =

View on Pith Pith review arXiv

[43] [43]

Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time. , keywords =. doi:10.1093/mnras/stz3131 , archivePrefix =. 1911.02572 , primaryClass =

View on Pith Pith review arXiv 1911

[44] [45]

A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations. , keywords =. doi:10.1093/mnras/stv072 , archivePrefix =. 1409.3221 , primaryClass =

View on Pith Pith review arXiv

[45] [47]

SKIRT: An advanced dust radiative transfer code with a user-friendly architecture. Astronomy and Computing , keywords =. doi:10.1016/j.ascom.2014.10.004 , archivePrefix =. 1410.1629 , primaryClass =

View on Pith Pith review arXiv 2014

[46] [48]

The EAGLE project: simulating the evolution and assembly of galaxies and their environments. , keywords =. doi:10.1093/mnras/stu2058 , archivePrefix =. 1407.7040 , primaryClass =

View on Pith Pith review arXiv

[47] [52]

Simulating galaxy formation with the IllustrisTNG model. , keywords =. doi:10.1093/mnras/stx2656 , archivePrefix =. 1703.02970 , primaryClass =

View on Pith Pith review arXiv

[48] [53]

Simulating galaxy formation with black hole driven thermal and kinetic feedback. , keywords =. doi:10.1093/mnras/stw2944 , archivePrefix =. 1607.03486 , primaryClass =

View on Pith Pith review arXiv

[49] [54]

Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships. , keywords =. doi:10.1086/500572 , archivePrefix =. astro-ph/0601303 , primaryClass =

View on Pith Pith review arXiv

[50] [55]

A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy. , keywords =. doi:10.3847/0004-637X/819/2/129 , archivePrefix =. 1603.00461 , primaryClass =

View on Pith Pith review arXiv

[51] [56]

In the beginning: the first sources of light and the reionization of the universe. , keywords =. doi:10.1016/S0370-1573(01)00019-9 , archivePrefix =. astro-ph/0010468 , primaryClass =

View on Pith Pith review arXiv

[52] [57]

Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with CDM?. , keywords =. doi:10.1093/mnras/stac3224 , archivePrefix =. 2208.10479 , primaryClass =

View on Pith Pith review arXiv

[53] [58]

On the abundance of extreme voids. , keywords =. doi:10.1088/1475-7516/2015/05/062 , archivePrefix =. 1502.07705 , primaryClass =

View on Pith Pith review arXiv 2015

[54] [59]

Cluster-Void Degeneracy Breaking: Dark Energy, Planck, and the Largest Cluster and Void. , keywords =. doi:10.3847/2041-8205/820/1/L7 , archivePrefix =. 1511.04075 , primaryClass =

View on Pith Pith review arXiv

[55] [60]

Exact extreme value statistics and the halo mass function. , keywords =. doi:10.1111/j.1745-3933.2011.01134.x , archivePrefix =. 1108.1358 , primaryClass =

View on Pith arXiv 2011

[56] [62]

Primordial non-Gaussianity and extreme-value statistics of galaxy clusters. , keywords =. doi:10.1103/PhysRevD.85.063508 , archivePrefix =. 1107.5617 , primaryClass =

View on Pith Pith review arXiv

[57] [63]

Extreme-value statistics of the spin of primordial black holes. , keywords =. doi:10.1103/PhysRevD.104.083018 , archivePrefix =. 2109.12268 , primaryClass =

View on Pith Pith review arXiv

[58] [67]

Quasars and the Intergalactic Medium at Cosmic Dawn. , keywords =. doi:10.1146/annurev-astro-052920-102455 , archivePrefix =. 2212.06907 , primaryClass =

View on Pith Pith review arXiv

[59] [68]

A Survey of z>5.8 Quasars in the Sloan Digital Sky Survey. I. Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z -0.5ex 6. , keywords =. doi:10.1086/324111 , archivePrefix =. astro-ph/0108063 , primaryClass =

View on Pith Pith review arXiv

[60] [69]

A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey. II. Discovery of Three Additional Quasars at z>6. , keywords =. doi:10.1086/368246 , archivePrefix =. astro-ph/0301135 , primaryClass =

View on Pith Pith review arXiv

[61] [70]

A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey. IV. Discovery of Seven Additional Quasars. , keywords =. doi:10.1086/500296 , archivePrefix =. astro-ph/0512080 , primaryClass =

View on Pith Pith review arXiv

[62] [71]

First Results from the Canada-France High-z Quasar Survey: Constraints on the z = 6 Quasar Luminosity Function and the Quasar Contribution to Reionization. , keywords =. doi:10.1086/462408 , archivePrefix =. astro-ph/0507183 , primaryClass =

View on Pith Pith review arXiv

[63] [72]

Six More Quasars at Redshift 6 Discovered by the Canada-France High-z Quasar Survey. , keywords =. doi:10.1088/0004-6256/137/3/3541 , archivePrefix =. 0901.0565 , primaryClass =

View on Pith Pith review arXiv

[64] [73]

The Canada-France High-z Quasar Survey: Nine New Quasars and the Luminosity Function at Redshift 6. , keywords =. doi:10.1088/0004-6256/139/3/906 , archivePrefix =. 0912.0281 , primaryClass =

View on Pith Pith review arXiv

[65] [74]

Discovery of Three z > 6.5 Quasars in the VISTA Kilo-Degree Infrared Galaxy (VIKING) Survey. , keywords =. doi:10.1088/0004-637X/779/1/24 , archivePrefix =. 1311.3666 , primaryClass =

View on Pith Pith review arXiv

[66] [75]

First discoveries of z 6 quasars with the Kilo-Degree Survey and VISTA Kilo-Degree Infrared Galaxy survey. , keywords =. doi:10.1093/mnras/stv1774 , archivePrefix =. 1507.00726 , primaryClass =

View on Pith Pith review arXiv

[67] [76]

The Assembly of the First Massive Black Holes. , keywords =. doi:10.1146/annurev-astro-120419-014455 , archivePrefix =. 1911.05791 , primaryClass =

View on Pith Pith review arXiv 1911

[68] [77]

z -0.5ex 7 Galaxy Candidates from NICMOS Observations Over the HDF-South and the CDF-South and HDF-North Goods Fields. , keywords =. doi:10.1088/0004-637X/725/2/1587 , archivePrefix =. 1003.1706 , primaryClass =

View on Pith Pith review arXiv

[69] [78]

Overview of the JWST Advanced Deep Extragalactic Survey (JADES). arXiv e-prints , keywords =. doi:10.48550/arXiv.2306.02465 , archivePrefix =. 2306.02465 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2306.02465

[70] [79]

Black holes in the early Universe. Reports on Progress in Physics , keywords =. doi:10.1088/0034-4885/75/12/124901 , archivePrefix =. 1209.2243 , primaryClass =

View on Pith Pith review arXiv

[71] [80]

The origins of massive black holes. Nature Reviews Physics , keywords =. doi:10.1038/s42254-021-00364-9 , archivePrefix =. 2110.10175 , primaryClass =

View on Pith Pith review arXiv

[72] [82]

The First Massive Black Hole Seeds and Their Hosts. , keywords =. doi:10.1088/0004-637X/742/1/13 , archivePrefix =. 1104.3858 , primaryClass =

View on Pith Pith review arXiv

[73] [83]

Formation of Supermassive Black Hole Seeds. , keywords =. doi:10.1017/pasa.2016.41 , archivePrefix =. 1605.07391 , primaryClass =

View on Pith Pith review arXiv 2016

[74] [84]

Feedback-regulated supermassive black hole seed formation. , keywords =. doi:10.1093/mnras/stu1007 , archivePrefix =. 1405.6743 , primaryClass =

View on Pith Pith review arXiv

[75] [85]

The formation of the first quasars: the black hole seeds, accretion, and feedback models. , keywords =. doi:10.1093/mnras/stac1556 , archivePrefix =. 2012.01458 , primaryClass =

View on Pith Pith review arXiv 2012

[76] [86]

Sulla determinazione empirica di una lgge di distribuzione , author=. Inst. Ital. Attuari, Giorn. , volume=

View on Pith

[77] [87]

Star Formation. doi:10.1142/10091 , adsurl =

View on Pith doi:10.1142/10091

[78] [88]

Nuclear activity versus star formation: emission-line diagnostics at ultraviolet and optical wavelengths. , keywords =. doi:10.1093/mnras/stv2794 , archivePrefix =. 1511.08217 , primaryClass =

View on Pith Pith review arXiv

[79] [89]

Multiline Assessment of Narrow-line Regions in z 3 Radio Galaxies. , keywords =. doi:10.3847/1538-4357/ac5b71 , archivePrefix =. 2203.03390 , primaryClass =

View on Pith Pith review arXiv

[80] [90]

The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]- 1908 A emission 10.8 to 12.5 Gyr ago. , keywords =. doi:10.1051/0004-6361/201732197 , archivePrefix =. 1710.10715 , primaryClass =

View on Pith Pith review arXiv 1908

[81] [91]

High velocity outflows in quasars

View on Pith

[82] [92]

Statistical analysis of Al III and C III] emission lines as virial black hole mass estimators in quasars. , keywords =. doi:10.1051/0004-6361/202244177 , archivePrefix =. 2209.05526 , primaryClass =

View on Pith Pith review arXiv

[83] [93]

The formation of supermassive black holes from Population III.1 seeds. I. Cosmic formation histories and clustering properties. , keywords =. doi:10.1093/mnras/sty3298 , archivePrefix =. 1608.04421 , primaryClass =

View on Pith Pith review arXiv

[84] [94]

The formation of supermassive black holes from Population III.1 seeds. II. Evolution to the local universe. , keywords =. doi:10.1093/mnras/stad2346 , archivePrefix =. 2301.11464 , primaryClass =

View on Pith Pith review arXiv

[85] [95]

Conditions for Optimal Growth of Black Hole Seeds. , keywords =. doi:10.3847/2041-8213/aa9aea , archivePrefix =. 1710.09375 , primaryClass =

View on Pith Pith review arXiv

[86] [96]

The growth of black holes from Population III remnants in the Renaissance simulations. , keywords =. doi:10.1093/mnras/sty2103 , archivePrefix =. 1804.06477 , primaryClass =

View on Pith Pith review arXiv

[87] [97]

Diagnostics for PopIII galaxies and direct collapse black holes in the early universe. , keywords =. doi:10.1093/mnras/stac1242 , archivePrefix =. 2204.11870 , primaryClass =

View on Pith Pith review arXiv

[88] [98]

The characteristic black hole mass resulting from direct collapse in the early Universe. , keywords =. doi:10.1093/mnras/stt1786 , archivePrefix =. 1309.1097 , primaryClass =

View on Pith Pith review arXiv

[89] [99]

Formation of the First Nuclear Clusters and Massive Black Holes at High Redshift. , keywords =. doi:10.1088/0004-637X/694/1/302 , archivePrefix =. 0810.1057 , primaryClass =

View on Pith Pith review arXiv

[90] [100]

Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes. , keywords =. doi:10.1046/j.1365-8711.2001.04006.x , archivePrefix =. astro-ph/9907024 , primaryClass =

View on Pith arXiv 2001

[91] [101]

HMFcalc: An online tool for calculating dark matter halo mass functions. Astronomy and Computing , keywords =. doi:10.1016/j.ascom.2013.11.001 , archivePrefix =. 1306.6721 , primaryClass =

View on Pith Pith review arXiv 2013

[92] [102]

Growing massive black holes through supercritical accretion of stellar-mass seeds. , keywords =. doi:10.1093/mnras/stv2877 , archivePrefix =. 1512.02651 , primaryClass =

View on Pith Pith review arXiv

[93] [103]

Supermassive black holes in cosmological simulations I: M _ BH - M _ relation and black hole mass function. , keywords =. doi:10.1093/mnras/stab496 , archivePrefix =. 2006.10094 , primaryClass =

View on Pith Pith review arXiv 2006

[94] [104]

Supermassive black holes in cosmological simulations - II: the AGN population and predictions for upcoming X-ray missions. , keywords =. doi:10.1093/mnras/stab3147 , archivePrefix =. 2111.01802 , primaryClass =

View on Pith Pith review arXiv

[95] [105]

Simulating the growth of Intermediate Mass Black Holes. , keywords =. doi:10.1093/mnras/stv018 , archivePrefix =. 1501.00989 , primaryClass =

View on Pith Pith review arXiv

[96] [106]

Super-critical Growth of Massive Black Holes from Stellar-mass Seeds. , keywords =. doi:10.1088/2041-8205/784/2/L38 , archivePrefix =. 1402.6995 , primaryClass =

View on Pith Pith review arXiv

[97] [107]

Slim Disks Around Kerr Black Holes Revisited. , keywords =. doi:10.1088/0067-0049/183/2/171 , archivePrefix =. 0906.0355 , primaryClass =

View on Pith Pith review arXiv

[98] [108]

Growth problems of stellar black holes in early galaxies. , keywords =. doi:10.1093/mnras/sty1482 , archivePrefix =. 1807.05760 , primaryClass =

View on Pith Pith review arXiv

[99] [109]

The sustainable growth of the first black holes. , keywords =. doi:10.1093/mnras/stx1640 , archivePrefix =. 1706.06592 , primaryClass =

View on Pith Pith review arXiv

[100] [110]

Relations between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe. , keywords =. doi:10.1088/0004-637X/813/2/82 , archivePrefix =. 1508.06274 , primaryClass =

View on Pith Pith review arXiv

[101] [111]

The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies. , keywords =. doi:10.1051/0004-6361/201936634 , archivePrefix =. 2002.00958 , primaryClass =

View on Pith Pith review arXiv 2002

[102] [112]

JWST CEERS and JADES Active Galaxies at z = 4-7 Violate the Local M _ -M _ Relation at >3 : Implications for Low-mass Black Holes and Seeding Models. , keywords =. doi:10.3847/2041-8213/ad0158 , archivePrefix =. 2308.12331 , primaryClass =

View on Pith Pith review arXiv

[103] [113]

GN-z11: The environment of an AGN at z= 10.603. arXiv e-prints , keywords =. doi:10.48550/arXiv.2306.09142 , archivePrefix =. 2306.09142 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2306.09142

[104] [114]

Kiloparsec-scale ALMA Imaging of [C II] and Dust Continuum Emission of 27 Quasar Host Galaxies at z 6. , keywords =. doi:10.3847/1538-4357/abc563 , archivePrefix =. 2010.14874 , primaryClass =

View on Pith Pith review arXiv 2010

[105] [115]

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-luminosity Quasar at z = 7.07 on the Local Black Hole to Host Mass Relation. , keywords =. doi:10.3847/1538-4357/abf6dc , archivePrefix =. 2104.05738 , primaryClass =

View on Pith Pith review arXiv

[106] [116]

Intermediate-Mass Black Holes. , keywords =. doi:10.1146/annurev-astro-032620-021835 , archivePrefix =. 1911.09678 , primaryClass =

View on Pith Pith review arXiv 1911

[107] [117]

The formation of nuclei in newly formed galaxies and the evolution of the quasar population. , keywords =. doi:10.1093/mnras/263.1.168 , adsurl =

View on Pith doi:10.1093/mnras/263.1.168

[108] [119]

Massive Black Holes as Population III Remnants. , keywords =. doi:10.1086/319848 , archivePrefix =. astro-ph/0101223 , primaryClass =

View on Pith Pith review arXiv

[109] [120]

Initial mass function of intermediate-mass black hole seeds. , keywords =. doi:10.1093/mnras/stu1280 , archivePrefix =. 1406.6685 , primaryClass =

View on Pith Pith review arXiv

[110] [121]

A Snapshot Survey for Gravitational Lenses among z>=4.0 Quasars. II. Constraints on the 4.0<z<5.4 Quasar Population. , keywords =. doi:10.1086/498063 , archivePrefix =. astro-ph/0509135 , primaryClass =

View on Pith Pith review arXiv

[111] [123]

Physical Properties of the First Quasars. , keywords =. doi:10.1017/pasa.2017.14 , archivePrefix =. 1702.06123 , primaryClass =

View on Pith Pith review arXiv 2017

[112] [124]

Correcting C IV-based virial black hole masses. , keywords =. doi:10.1093/mnras/stw2797 , archivePrefix =. 1610.08977 , primaryClass =

View on Pith Pith review arXiv

[113] [125]

Detecting and Characterizing Young Quasars. II. Four Quasars at z 6 with Lifetimes < 10 ^ 4 Yr. , keywords =. doi:10.3847/1538-4357/ac0a76 , archivePrefix =. 2106.04586 , primaryClass =

View on Pith Pith review arXiv

[114] [126]

An ALMA [C II] Survey of 27 Quasars at z > 5.94. , keywords =. doi:10.3847/1538-4357/aaa5aa , archivePrefix =. 1801.02641 , primaryClass =

View on Pith Pith review arXiv

[115] [127]

Probing the Interstellar Medium and Star Formation of the Most Luminous Quasar at z = 6.3. , keywords =. doi:10.3847/0004-637X/830/1/53 , archivePrefix =. 1606.09634 , primaryClass =

View on Pith Pith review arXiv

[116] [128]

Molecular gas in z 6 quasar host galaxies. , keywords =. doi:10.1051/0004-6361/202142871 , archivePrefix =. 2203.03658 , primaryClass =

View on Pith Pith review arXiv

[117] [129]

Copious Amounts of Dust and Gas in a z = 7.5 Quasar Host Galaxy. , keywords =. doi:10.3847/2041-8213/aa943a , archivePrefix =. 1712.01886 , primaryClass =

View on Pith Pith review arXiv

[118] [130]

On the effect of galactic outflows in cosmological simulations of disc galaxies. , keywords =. doi:10.1093/mnras/stx1352 , archivePrefix =. 1705.10325 , primaryClass =

View on Pith Pith review arXiv

[119] [131]

Colour-magnitude diagram in simulations of galaxy formation. , keywords =. doi:10.1093/mnras/sty1896 , archivePrefix =. 1805.00028 , primaryClass =

View on Pith Pith review arXiv

[120] [132]

Chemical evolution of disc galaxies from cosmological simulations. , keywords =. doi:10.1093/mnras/stz492 , archivePrefix =. 1902.05955 , primaryClass =

View on Pith Pith review arXiv 1902

[121] [134]

Simulating realistic disc galaxies with a novel sub-resolution ISM model. , keywords =. doi:10.1093/mnras/stu2400 , adsurl =

View on Pith doi:10.1093/mnras/stu2400

[122] [135]

A JWST/NIRSpec First Census of Broad-line AGNs at z = 4-7: Detection of 10 Faint AGNs with M _ BH 10 ^ 6 - 10 ^ 8 M _ and Their Host Galaxy Properties. , keywords =. doi:10.3847/1538-4357/ad029e , archivePrefix =. 2303.11946 , primaryClass =

View on Pith Pith review arXiv

[123] [136]

A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of z > 6.5 Quasars Using JWST. , keywords =. doi:10.3847/2041-8213/acc9c8 , archivePrefix =. 2304.09888 , primaryClass =

View on Pith Pith review arXiv

[124] [137]

On the physics of dust grains in hot gas. , keywords =. doi:10.1086/157165 , adsurl =

View on Pith doi:10.1086/157165

[125] [138]

Asplund, Martin and Grevesse, Nicolas and Sauval, A. Jacques and Scott, Pat , year=. The Chemical Composition of the Sun , volume=. Annual Review of Astronomy and Astrophysics , publisher=. doi:10.1146/annurev.astro.46.060407.145222 , number=

View on Pith arXiv

[126] [139]

The route to massive black hole formation via merger-driven direct collapse: a review. Reports on Progress in Physics , keywords =. doi:10.1088/1361-6633/aad6a5 , archivePrefix =. 1803.06391 , primaryClass =

View on Pith Pith review arXiv

[127] [141]

Evidence for Low Radiative Efficiency or Highly Obscured Growth of z > 7 Quasars. , keywords =. doi:10.3847/2041-8213/ab42e3 , archivePrefix =. 1906.10130 , primaryClass =

View on Pith Pith review arXiv 1906

[128] [142]

Revealing the Accretion Physics of Supermassive Black Holes at Redshift z 7 with Chandra and Infrared Observations. , keywords =. doi:10.3847/1538-4357/abcc5e , archivePrefix =. 2011.12458 , primaryClass =

View on Pith Pith review arXiv 2011

[129] [143]

An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5. , keywords =. doi:10.1038/nature25180 , archivePrefix =. 1712.01860 , primaryClass =

View on Pith Pith review arXiv

[130] [144]

P \= o niu \= a 'ena: A Luminous z = 7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole. , keywords =. doi:10.3847/2041-8213/ab9c26 , archivePrefix =. 2006.13452 , primaryClass =

View on Pith Pith review arXiv 2006

[131] [145]

A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars. , keywords =. doi:10.3847/2041-8213/ace619 , archivePrefix =. 2303.08918 , primaryClass =

View on Pith Pith review arXiv

[132] [146]

First rest-frame infrared spectrum of a z>7 quasar: JWST/MRS observations of J1120+0641. arXiv e-prints , keywords =. doi:10.48550/arXiv.2307.14414 , archivePrefix =. 2307.14414 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2307.14414

[133] [147]

UNCOVER: The Growth of the First Massive Black Holes from JWST/NIRSpec-Spectroscopic Redshift Confirmation of an X-Ray Luminous AGN at z = 10.1. , keywords =. doi:10.3847/2041-8213/acf7c5 , archivePrefix =. 2308.02750 , primaryClass =

View on Pith Pith review arXiv

[134] [148]

A supermassive black hole in the early universe growing in the shadows. arXiv e-prints , keywords =. doi:10.48550/arXiv.2308.05735 , archivePrefix =. 2308.05735 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2308.05735

[135] [149]

Are we surprised to find SMBHs with JWST at z 9?. , keywords =. doi:10.1093/mnras/stad2503 , archivePrefix =. 2305.12504 , primaryClass =

View on Pith Pith review arXiv

[136] [150]

Exploring the nature of UV-bright z rsim 10 galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?. arXiv e-prints , keywords =. doi:10.48550/arXiv.2305.04944 , archivePrefix =. 2305.04944 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2305.04944

[137] [151]

Very high redshift quasars and the rapid emergence of supermassive black holes. , keywords =. doi:10.1093/mnras/staa2276 , archivePrefix =. 2007.14402 , primaryClass =

View on Pith Pith review arXiv 2007

[138] [152]

The low-end of the black hole mass function at cosmic dawn. , keywords =. doi:10.1093/mnras/stac062 , archivePrefix =. 2201.02630 , primaryClass =

View on Pith Pith review arXiv

[139] [153]

The Rise of Faint, Red Active Galactic Nuclei at z > 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields. , keywords =. doi:10.3847/1538-4357/adbc7d , archivePrefix =. 2404.03576 , primaryClass =

View on Pith Pith review arXiv

[140] [154]

Casey, Caitlin M. and Akins, Hollis B. and Kokorev, Vasily and McKinney, Jed and Cooper, Olivia R. and Long, Arianna S. and Franco, Maximilien and Manning, Sinclaire M. , month = sep, year =. Dust in. doi:10.48550/arXiv.2407.05094 , abstract =

View on Pith Pith review arXiv doi:10.48550/arxiv.2407.05094

[141] [155]

An Upper Limit of 10 ^ 6 M _ in Dust from ALMA Observations in 60 Little Red Dots. , keywords =. doi:10.3847/2041-8213/adfa91 , archivePrefix =. 2505.18873 , primaryClass =

View on Pith Pith review arXiv

[142] [156]

Exploring active galactic nuclei and little red dots with the Obelisk simulation. , keywords =. doi:10.1051/0004-6361/202451963 , archivePrefix =. 2408.12854 , primaryClass =

View on Pith Pith review arXiv

[143] [157]

Little. , author =. 2024 , pages =. doi:10.3847/1538-4357/ad2345 , abstract =

View on Pith doi:10.3847/1538-4357/ad2345 2024

[144] [158]

A population of red candidate massive galaxies. Nature , author =. 2023 , pages =. doi:10.1038/s41586-023-05786-2 , language =

View on Pith doi:10.1038/s41586-023-05786-2 2023

[145] [159]

Labbe, Ivo and Greene, Jenny E. and Bezanson, Rachel and Fujimoto, Seiji and Furtak, Lukas J. and Goulding, Andy D. and Matthee, Jorryt and Naidu, Rohan P. and Oesch, Pascal A. and Atek, Hakim and Brammer, Gabriel and Chemerynska, Iryna and Coe, Dan and Cutler, Sam E. and Dayal, Pratika and Feldmann, Robert and Franx, Marijn and Glazebrook, Karl and Leja,...

View on Pith 2024

[146] [160]

Camps, P. and Baes, M. , urldate =. doi:10.1016/j.ascom.2020.100381 , shorttitle =

View on Pith arXiv 2020

[147] [161]

Baes, M. and Camps, P. , urldate =. doi:10.1016/j.ascom.2015.05.006 , shorttitle =

View on Pith doi:10.1016/j.ascom.2015.05.006 2015

[148] [162]

Camps, P. and Baes, M. , urldate =. doi:10.1016/j.ascom.2014.10.004 , shorttitle =

View on Pith doi:10.1016/j.ascom.2014.10.004 2014

[149] [163]

Infrared emission of z 6 galaxies: AGN imprints. , keywords =. doi:10.1093/mnras/stab528 , archivePrefix =. 2102.08956 , primaryClass =

View on Pith Pith review arXiv

[150] [164]

The dust attenuation law in z 6 quasars. , keywords =. doi:10.1093/mnras/stab1876 , archivePrefix =. 2106.15625 , primaryClass =

View on Pith Pith review arXiv

[151] [165]

Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample. , keywords =. doi:10.1086/518306 , archivePrefix =. astro-ph/0703213 , primaryClass =

View on Pith Pith review arXiv

[152] [166]

Dust Grain-Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud. , keywords =. doi:10.1086/318651 , archivePrefix =. astro-ph/0008146 , primaryClass =

View on Pith Pith review arXiv

[153] [167]

Planck 2015 results. XIII. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201525830 , archivePrefix =. 1502.01589 , primaryClass =

View on Pith Pith review arXiv 2015

[154] [168]

The effect of interstellar matter on climatic variation. Proceedings of the Cambridge Philosophical Society , year = 1939, month = jan, volume =. doi:10.1017/S0305004100021150 , adsurl =

View on Pith doi:10.1017/s0305004100021150 1939

[155] [169]

On the mechanism of accretion by stars. , year = 1944, month = jan, volume =. doi:10.1093/mnras/104.5.273 , adsurl =

View on Pith doi:10.1093/mnras/104.5.273 1944

[156] [171]

Another view into JWST-discovered X-ray weak AGNs via radiative dusty feedback. , keywords =. doi:10.1093/mnras/staf1439 , archivePrefix =. 2509.05423 , primaryClass =

View on Pith Pith review arXiv

[157] [172]

Weakness of X-rays and Variability in High-redshift AGNs with Super-Eddington Accretion , author=. 2025 , eprint=

View on Pith 2025

[158] [173]

AGN obscuration in optical and X-rays: Host properties and the interplay of nuclear and galactic gas and dust in a combined SDSS–XMM sample , DOI= "10.1051/0004-6361/202558424", url= "https://doi.org/10.1051/0004-6361/202558424", journal =

View on Pith doi:10.1051/0004-6361/202558424

[159] [174]

Bornancini, C. G. and Oio, G. A. and Coldwell, G. , year=. Obscured and unobscured X-ray active galactic nuclei: I. Host-galaxy properties , volume=. doi:10.1051/0004-6361/202554599 , journal=

View on Pith doi:10.1051/0004-6361/202554599

[160] [175]

Chandra Rules Out Super-Eddington Accretion Models for Little Red Dots. , keywords =. doi:10.3847/2041-8213/adf5c8 , archivePrefix =. 2505.09669 , primaryClass =

View on Pith Pith review arXiv

[161] [176]

The X-ray weakness of little red dots and JWST-selected AGN: Comparison with local AGN in different accretion regimes. , keywords =. doi:10.1051/0004-6361/202557444 , archivePrefix =. 2603.10162 , primaryClass =

View on Pith Pith review arXiv

[162] [177]

The X-Ray Dot: Exotic Dust or a Late-stage Little Red Dot?. , keywords =. doi:10.3847/2041-8213/ae4c88 , archivePrefix =. 2601.09778 , primaryClass =

View on Pith arXiv

[163] [178]

Discovery of two little red dots transitioning into quasars , author=. 2025 , eprint=

View on Pith 2025

[164] [179]

Estimating Black Hole Masses in Active Galaxies Using the H Emission Line. , keywords =. doi:10.1086/431897 , archivePrefix =. astro-ph/0508335 , primaryClass =

View on Pith Pith review arXiv

[165] [180]

Type 1 AGN at low z- I. Emission properties. , keywords =. doi:10.1111/j.1365-2966.2012.20901.x , archivePrefix =. 1203.3158 , primaryClass =

View on Pith arXiv 2012

[166] [181]

Richards, Gordon T. and Lacy, Mark and Storrie‐Lombardi, Lisa J. and Hall, Patrick B. and Gallagher, S. C. and Hines, Dean C. and Fan, Xiaohui and Papovich, Casey and Vanden Berk, Daniel E. and Trammell, George B. and Schneider, Donald P. and Vestergaard, Marianne and York, Donald G. and Jester, Sebastian and Anderson, Scott F. and Budavari, Tamas and Sza...

View on Pith doi:10.1086/5

[167] [182]

Dong, Xiaobo and Wang, Tinggui and Wang, Jianguo and Yuan, Weimin and Zhou, Hongyan and Dai, Haifeng and Zhang, Kai , title =. , volume =. 2007 , month =. doi:10.1111/j.1365-2966.2007.12560.x , url =

View on Pith arXiv 2007

[168] [183]

Springel, Volker and di Matteo, Tiziana and Hernquist, Lars , title =. , volume =. 2005 , month =. doi:10.1111/j.1365-2966.2005.09238.x , url =

View on Pith arXiv 2005

[169] [184]

Springel, Volker and Hernquist, Lars , title =. , volume =. 2003 , month =. doi:10.1046/j.1365-8711.2003.06206.x , url =

View on Pith arXiv 2003

[170] [185]

Galactic Stellar and Substellar Initial Mass Function. , keywords =. doi:10.1086/376392 , archivePrefix =. astro-ph/0304382 , primaryClass =

View on Pith Pith review arXiv

[171] [186]

Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs. , keywords =. doi:10.1051/0004-6361/201629228 , archivePrefix =. 1607.00288 , primaryClass =

View on Pith Pith review arXiv

[172] [187]

Nozawa, Takaya and Asano, Ryosuke S. and Hirashita, Hiroyuki and Takeuchi, Tsutomu T. , title =. Monthly Notices of the Royal Astronomical Society: Letters , volume =. 2015 , month =. doi:10.1093/mnrasl/slu175 , url =

View on Pith doi:10.1093/mnrasl/slu175 2015

[173] [188]

Asano, Ryosuke S. and Takeuchi, Tsutomu T. and Hirashita, Hiroyuki and Inoue, Akio K. , title=. Earth, Planets and Space , year=. doi:10.5047/eps.2012.04.014 , url=

View on Pith doi:10.5047/eps.2012.04.014 2012

[174] [189]

Galaxy simulation with dust formation and destruction. , keywords =. doi:10.1093/mnras/stw3061 , archivePrefix =. 1609.07547 , primaryClass =

View on Pith Pith review arXiv

[175] [190]

Ferrara, A. and Viti, S. and Ceccarelli, C. , title =. Monthly Notices of the Royal Astronomical Society: Letters , volume =. 2016 , month =. doi:10.1093/mnrasl/slw165 , url =

View on Pith doi:10.1093/mnrasl/slw165 2016

[176] [191]

No [C II] or dust detection in two Little Red Dots at z _ spec > 7. , keywords =. doi:10.1051/0004-6361/202554361 , archivePrefix =. 2503.01945 , primaryClass =

View on Pith Pith review arXiv

[177] [192]

Evidence of violation of Case B recombination in Little Red Dots. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.06362 , archivePrefix =. 2510.06362 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2510.06362

[178] [193]

Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption. arXiv e-prints , keywords =. doi:10.48550/arXiv.2510.00101 , archivePrefix =. 2510.00101 , primaryClass =

View on Pith doi:10.48550/arxiv.2510.00101

[179] [194]

Ji, Xihan and D’Eugenio, Francesco and Juodžbalis, Ignas and Walton, Dominic J and Fabian, Andrew C and Maiolino, Roberto and Ramos Almeida, Cristina and Acosta Pulido, Jose A and Belokurov, Vasily A and Isobe, Yuki and Jones, Gareth and Maraston, Claudia and Scholtz, Jan and Simmonds, Charlotte and Tacchella, Sandro and Terlevich, Elena and Terlevich, Ro...

View on Pith doi:10.1093/mnras/staf2235 2026

[180] [195]

The Discovery of Little Red Dots in the Local Universe: Signatures of Cool Gas Envelopes. , keywords =. doi:10.3847/1538-4357/ae2bdf , archivePrefix =. 2507.10659 , primaryClass =

View on Pith arXiv

[181] [196]

The Cliff: a metal-poor little red dot hosting an overmassive black hole at z = 3.55. , keywords =. doi:10.1093/mnras/stag1220 , archivePrefix =. 2604.09177 , primaryClass =

View on Pith Pith review arXiv

[182] [197]

Is GRB 050904 at z = 6.3 absorbed by dust? , DOI= "10.1051/0004-6361/201016414", url= "https://doi.org/10.1051/0004-6361/201016414", journal =

View on Pith doi:10.1051/0004-6361/201016414

[183] [198]

Hirashita, Hiroyuki and Aoyama, Shohei , title =. , volume =. 2019 , month =. doi:10.1093/mnras/sty2838 , url =

View on Pith doi:10.1093/mnras/sty2838 2019

[184] [199]

Hirashita, Hiroyuki and Nozawa, Takaya and Villaume, Alexa and Srinivasan, Sundar , title =. , volume =. 2015 , month =. doi:10.1093/mnras/stv2095 , url =

View on Pith Pith review doi:10.1093/mnras/stv2095 2015

[185] [200]

What determines the grain size distribution in galaxies?. , keywords =. doi:10.1093/mnras/stt506 , archivePrefix =. 1303.5528 , primaryClass =

View on Pith Pith review arXiv

[186] [201]

Stellar sources of dust in the high-redshift Universe. , keywords =. doi:10.1111/j.1365-2966.2009.15076.x , archivePrefix =. 0905.1691 , primaryClass =

View on Pith arXiv 2009

[187] [202]

Hjorth, Jens and Vreeswijk, Paul M. and Gall, Christa and Watson, Darach , title =. , abstract =. 2013 , month =. doi:10.1088/0004-637X/768/2/173 , url =

View on Pith doi:10.1088/0004-637x/768/2/173 2013

[188] [203]

Zafar, T and Møller, P and Watson, D and Lattanzio, J and Hopkins, A M and Karakas, A and Fynbo, J P U and Tanvir, N R and Selsing, J and Jakobsson, P and Heintz, K E and Kann, D A and Groves, B and Kulkarni, V and Covino, S and D’Elia, V and Japelj, J and Corre, D and Vergani, S , title =. , volume =. 2018 , month =. doi:10.1093/mnras/sty1876 , url =

View on Pith doi:10.1093/mnras/sty1876 2018

[189] [204]

Zafar, T. and Watson, D. and Fynbo, J. P. U. and Malesani, D. and Jakobsson, P. and de Ugarte Postigo, A. , year=. The extinction curves of star-forming regions from<i>z</i> = 0.1 to 6.7 using GRB afterglow spectroscopy , volume=. doi:10.1051/0004-6361/201116663 , journal=

View on Pith doi:10.1051/0004-6361/201116663

[190] [205]

Li, Zhengrong and Inayoshi, Kohei and Chen, Kejian and Ichikawa, Kohei and Ho, Luis C. , title =. , abstract =. 2025 , month =. doi:10.3847/1538-4357/ada5fb , url =

View on Pith doi:10.3847/1538-4357/ada5fb 2025

[191] [206]

Chen, Kejian and Li, Zhengrong and Inayoshi, Kohei and Ho, Luis C. , title =. , abstract =. 2025 , month =. doi:10.3847/2041-8213/ae1955 , url =

View on Pith doi:10.3847/2041-8213/ae1955 2025

[192] [207]

Extinction due to amorphous carbon grains in red quasars from the Sloan Digital Sky Survey. , keywords =. doi:10.1111/j.1365-2966.2004.07590.x , archivePrefix =. astro-ph/0401158 , primaryClass =

View on Pith arXiv 2004

[193] [208]

Gaskell, C. Martin and Goosmann, René W. and Antonucci, Robert R. J. and Whysong, David H. , title =. , abstract =. 2004 , month =. doi:10.1086/423885 , url =

View on Pith doi:10.1086/423885 2004

[194] [209]

Gallerani, S. and Maiolino, R. and Juarez, Y. and Nagao, T. and Marconi, A. and Bianchi, S. and Schneider, R. and Mannucci, F. and Oliva, T. and Willott, C. J. and Jiang, L. and Fan, X. , year=. The extinction law at high redshift and its implications , volume=. doi:10.1051/0004-6361/201014721 , journal=

View on Pith doi:10.1051/0004-6361/201014721

[195] [210]

What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition. , keywords =. doi:10.3847/1538-4357/ad38bb , archivePrefix =. 2401.08782 , primaryClass =

View on Pith Pith review arXiv

[196] [211]

COSMOS-Web: The Overabundance and Physical Nature of ``Little Red Dots'' Implications for Early Galaxy and SMBH Assembly. , keywords =. doi:10.3847/1538-4357/ade984 , archivePrefix =. 2406.10341 , primaryClass =

View on Pith Pith review arXiv

[197] [212]

The Galaxies Missed by Hubble and ALMA: The Contribution of Extremely Red Galaxies to the Cosmic Census at 3 < z < 8. , keywords =. doi:10.3847/1538-4357/ad3f17 , archivePrefix =. 2311.07483 , primaryClass =

View on Pith Pith review arXiv

[198] [213]

Exploring the Nature of Little Red Dots: Constraints on Active Galactic Nucleus and Stellar Contributions from PRIMER MIRI Imaging. , keywords =. doi:10.3847/1538-4357/adfcce , archivePrefix =. 2411.12005 , primaryClass =

View on Pith Pith review arXiv

[199] [214]

RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow. , keywords =. doi:10.3847/1538-4357/adc1ca , archivePrefix =. 2403.02304 , primaryClass =

View on Pith Pith review arXiv

[200] [215]

MIDIS: MIRI Uncovers Virgil, the First Little Red Dot with Clear Detection of Its Host Galaxy at z ≃ 6.6. , keywords =. doi:10.3847/1538-4357/ade5a6 , archivePrefix =. 2406.18207 , primaryClass =

View on Pith Pith review arXiv

[201] [216]

Setton, David J. and Greene, Jenny E. and Spilker, Justin S. and Williams, Christina C. and Labbé, Ivo and Ma, Yilun and Wang, Bingjie and Whitaker, Katherine E. and Leja, Joel and de Graaff, Anna and Alberts, Stacey and Bezanson, Rachel and Boogaard, Leindert A. and Brammer, Gabriel and Cutler, Sam E. and Cleri, Nikko J. and Cooper, Olivia R. and Dayal, ...

View on Pith 2025

[202] [217]

A Comprehensive Photometric Selection of ``Little Red Dots'' in MIRI Fields: An Infrared-Bright Little Red Dot at z = 3.1386 with Warm Dust Emission. , keywords =. doi:10.3847/1538-4357/ae0704 , archivePrefix =. 2412.01887 , primaryClass =

View on Pith Pith review arXiv

[203] [218]

Hviding, Raphael E. and de Graaff, Anna and Miller, Tim B. and Setton, David J. and Greene, Jenny E. and Labbé, Ivo and Brammer, Gabriel and Bezanson, Rachel and Boogaard, Leindert A. and Cleri, Nikko J. and Leja, Joel and Maseda, Michael V. and McConachie, Ian and Matthee, Jorryt and Naidu, Rohan P. and Oesch, Pascal A. and Wang, Bingjie and Whitaker, Ka...

View on Pith

[204] [219]

A. , author =. 2024 , note =. doi:10.3847/1538-4357/ad4265 , abstract =

View on Pith doi:10.3847/1538-4357/ad4265 2024

[205] [220]

, author =. 2024 , note =. doi:10.3847/1538-4357/ad1e5f , abstract =

View on Pith doi:10.3847/1538-4357/ad1e5f 2024

[206] [221]

A remarkable ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a little red dot at z = 3.5. , keywords =. doi:10.1051/0004-6361/202554681 , archivePrefix =. 2503.16600 , primaryClass =

View on Pith Pith review arXiv

[207] [222]

The Engine and its Flows: Little Red Dot spectra are shaped by the column densities of their gas envelopes. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.17667 , archivePrefix =. 2603.17667 , primaryClass =

View on Pith doi:10.48550/arxiv.2603.17667

[208] [223]

UNCOVER: 404 Error Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1. , keywords =. doi:10.3847/1538-4357/ada613 , archivePrefix =. 2410.06257 , primaryClass =

View on Pith Pith review arXiv

[209] [224]

RUBIES: Evolved Stellar Populations with Extended Formation Histories at z 7─8 in Candidate Massive Galaxies Identified with JWST/NIRSpec. , keywords =. doi:10.3847/2041-8213/ad55f7 , archivePrefix =. 2405.01473 , primaryClass =

View on Pith Pith review arXiv

[210] [225]

Ji, Xihan and Maiolino, Roberto and Übler, Hannah and Scholtz, Jan and D’Eugenio, Francesco and Sun, Fengwu and Perna, Michele and Turner, Hannah and Carniani, Stefano and Arribas, Santiago and Bennett, Jake S and Bunker, Andrew and Charlot, Stéphane and Cresci, Giovanni and Curti, Mirko and Egami, Eiichi and Fabian, Andy and Inayoshi, Kohei and Isobe, Yu...

View on Pith 2025

[211] [226]

A gas-enshrouded and gas-reddened black hole at cosmic dawn. , keywords =. doi:10.1038/s41586-026-10846-4 , archivePrefix =. 2503.16596 , primaryClass =

View on Pith Pith review arXiv

[212] [227]

Extremely. , author =. 2025 , note =. doi:10.3847/2041-8213/adaebd , abstract =

View on Pith doi:10.3847/2041-8213/adaebd 2025

[213] [228]

An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy. arXiv e-prints , keywords =. doi:10.48550/arXiv.2412.04557 , archivePrefix =. 2412.04557 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2412.04557

[214] [229]

Setton, David J. and Greene, Jenny E. and de Graaff, Anna and Ma, Yilun and Leja, Joel and Matthee, Jorryt and Bezanson, Rachel and Boogaard, Leindert A. and Cleri, Nikko J. and Katz, Harley and Labbe, Ivo and Maseda, Michael V. and McConachie, Ian and Miller, Tim B. and Price, Sedona H. and Suess, Katherine A. and van Dokkum, Pieter and Wang, Bingjie and...

View on Pith doi:10.3847/1538-4357/ae1500 2025

[215] [230]

Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies. , keywords =. doi:10.1146/annurev-astro-082708-101811 , archivePrefix =. 1304.7762 , primaryClass =

View on Pith Pith review arXiv

[216] [231]

GA-NIFS: A massive black hole in a low-metallicity AGN at z 5.55 revealed by JWST/NIRSpec IFS. , keywords =. doi:10.1051/0004-6361/202346137 , archivePrefix =. 2302.06647 , primaryClass =

View on Pith Pith review arXiv

[217] [232]

Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS. , keywords =. doi:10.3847/2041-8213/ace5a0 , archivePrefix =. 2302.00012 , primaryClass =

View on Pith Pith review arXiv

[218] [233]

Little Red and Blue Dots: simply stratified Broad Line Regions. arXiv e-prints , keywords =. doi:10.48550/arXiv.2603.22277 , archivePrefix =. 2603.22277 , primaryClass =

View on Pith doi:10.48550/arxiv.2603.22277

[219] [234]

Rinaldi, P. and Bonaventura, N. and Rieke, G. H. and Alberts, S. and Caputi, K. I. and Baker, W. M. and Baum, S. and Bhatawdekar, R. and Bunker, A. J. and Carniani, S. and Curtis-Lake, E. and D’Eugenio, F. and Egami, E. and Ji, Z. and Johnson, B. D. and Hainline, K. and Helton, J. M. and Lin, X. and Lyu, J. and Ma, Z. and Maiolino, R. and Pérez-González, ...

View on Pith 2025

[220] [235]

The Small Sizes and High Implied Densities of ``Little Red Dots'' with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus. , keywords =. doi:10.3847/2041-8213/ad90b8 , archivePrefix =. 2408.07745 , primaryClass =

View on Pith Pith review arXiv

[221] [236]

Hidden in Pixels. I. Discovery of dual ``little red dots'' indicates excess clustering on kilo-parsec scales. arXiv e-prints , keywords =. doi:10.48550/arXiv.2412.14246 , archivePrefix =. 2412.14246 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2412.14246

[222] [237]

Sizes and Mass Profiles of Candidate Massive Galaxies Discovered by JWST at 7 < z < 9: Evidence for Very Early Formation of the Central 100 pc of Present-day Ellipticals. , keywords =. doi:10.3847/2041-8213/acf5ef , archivePrefix =. 2305.17162 , primaryClass =

View on Pith Pith review arXiv

[223] [238]

(Re)solving the Complex Multiscale Morphology and V-shaped Spectral Energy Distribution of a Newly Discovered Strongly Lensed Little Red Dot in A383. , keywords =. doi:10.3847/2041-8213/ae82fe , archivePrefix =. 2512.03239 , primaryClass =

View on Pith Pith review arXiv

[224] [239]

Possible environmental quenching in an interacting little red dot pair at z 7. , keywords =. doi:10.1051/0004-6361/202553943 , archivePrefix =. 2501.17925 , primaryClass =

View on Pith Pith review arXiv

[225] [240]

A Deep Dive down the Broad-line Region: Permitted O I, Ca II, and Fe II Emission in an Active Galactic Nucleus Little Red Dot at z = 5.3. , keywords =. doi:10.3847/2041-8213/ae13a9 , archivePrefix =. 2507.20684 , primaryClass =

View on Pith arXiv

[226] [241]

A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling. arXiv e-prints , keywords =. doi:10.48550/arXiv.2605.30414 , archivePrefix =. 2605.30414 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2605.30414

[227] [242]

Extreme properties of a compact and massive accreting black hole host in the first 500 Myr. Nature Communications , keywords =. doi:10.1038/s41467-025-65070-x , archivePrefix =. 2412.04983 , primaryClass =

View on Pith Pith review arXiv

[228] [243]

JADES and BlackTHUNDER: rest-frame Balmer-line absorption and the local environment in a Little Red Dot at z = 5. , keywords =. doi:10.1093/mnras/staf2117 , archivePrefix =. 2506.14870 , primaryClass =

View on Pith arXiv

[229] [244]

A weak Ly halo for an extremely bright little red dot: Indications of enshrouded supermassive black hole growth. , keywords =. doi:10.1051/0004-6361/202555596 , archivePrefix =. 2505.09542 , primaryClass =

View on Pith arXiv

[230] [245]

VENUS: Two Faint Little Red Dots Separated by 70\,pc Hidden in a Single Lensed Galaxy at z 7. arXiv e-prints , keywords =. doi:10.48550/arXiv.2601.06015 , archivePrefix =. 2601.06015 , primaryClass =

View on Pith doi:10.48550/arxiv.2601.06015

[231] [246]

Connecting the Dots: UV-bright Companions of Little Red Dots as Lyman─Werner Sources Enabling Direct-collapse Black Hole Formation. , keywords =. doi:10.3847/2041-8213/ae58a5 , archivePrefix =. 2602.02702 , primaryClass =

View on Pith Pith review arXiv

[232] [247]

Beyond the Dot: An LRD-like Nucleus at the Heart of an IR-bright Galaxy and its Implications for High-redshift LRDs. , keywords =. doi:10.3847/1538-4357/ae80cd , archivePrefix =. 2507.17738 , primaryClass =

View on Pith Pith review arXiv

[233] [248]

A high black-hole-to-host mass ratio in a lensed AGN in the early Universe. , keywords =. doi:10.1038/s41586-024-07184-8 , archivePrefix =. 2308.05735 , primaryClass =

View on Pith Pith review arXiv

[234] [249]

Silencing the Giant: Evidence of Active Galactic Nucleus Feedback and Quenching in a Little Red Dot at z = 4.13. , keywords =. doi:10.3847/1538-4357/ad7d03 , archivePrefix =. 2407.20320 , primaryClass =

View on Pith Pith review arXiv

[235] [250]

Juodžbalis, Ignas and Marconcini, Cosimo and D’Eugenio, Francesco and Maiolino, Roberto and Marconi, Alessandro and Übler, Hannah and Scholtz, Jan and Ji, Xihan and Jones, Gareth C. and Perna, Michele and Arribas, Santiago and Bennett, Jake S. and Bromm, Volker and Bunker, Andrew J. and Carniani, Stefano and Charlot, Stéphane and Cresci, Giovanni and Daya...

View on Pith

[236] [251]

Pacucci, Fabio and Narayan, Ramesh , year=. Mildly Super-Eddington Accretion onto Slowly Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots , volume=. , publisher=. doi:10.3847/1538-4357/ad84f7 , number=

View on Pith doi:10.3847/1538-4357/ad84f7

[237] [252]

On the quenching of LRD X-ray emission by both Compton-thick gas and high accretion rates , author=. 2026 , eprint=

View on Pith 2026

[238] [253]

Stacking. , author =. 2024 , note =. doi:10.3847/2041-8213/ad7eba , abstract =

View on Pith doi:10.3847/2041-8213/ad7eba 2024

[239] [254]

Preparing Red-Green-Blue Images from CCD Data. , keywords =. doi:10.1086/382245 , archivePrefix =. astro-ph/0312483 , primaryClass =

View on Pith Pith review arXiv

[240] [255]

JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe. , keywords =. doi:10.1093/mnras/staf359 , archivePrefix =. 2405.00504 , primaryClass =

View on Pith Pith review arXiv

[241] [256]

X-Ray Weak Active Galactic Nuclei from Super-Eddington Accretion onto Infant Black Holes. , keywords =. doi:10.3847/2041-8213/ad90e1 , archivePrefix =. 2410.00417 , primaryClass =

View on Pith Pith review arXiv

[242] [257]

Do little red dots really form a distinct class of astronomical objects?. arXiv e-prints , keywords =. doi:10.48550/arXiv.2604.11677 , archivePrefix =. 2604.11677 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2604.11677

[243] [258]

Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST. , keywords =. doi:10.3847/1538-4357/acef21 , archivePrefix =. 2304.12347 , primaryClass =

View on Pith Pith review arXiv

[244] [259]

UNCOVER: A NIRSpec Identification of a Broad-line AGN at z = 8.50. , keywords =. doi:10.3847/2041-8213/ad037a , archivePrefix =. 2308.11610 , primaryClass =

View on Pith Pith review arXiv

[245] [260]

Extremely Red Galaxies at z = 5─9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?. , keywords =. doi:10.3847/1538-4357/ad167e , archivePrefix =. 2305.14418 , primaryClass =

View on Pith Pith review arXiv

[246] [261]

A. , author =. 2023 , note =. doi:10.3847/2041-8213/aca9d3 , abstract =

View on Pith doi:10.3847/2041-8213/aca9d3 2023

[247] [262]

JWST UNCOVER: Extremely Red and Compact Object at z _ phot ≃ 7.6 Triply Imaged by A2744. , keywords =. doi:10.3847/1538-4357/acdc9d , archivePrefix =. 2212.10531 , primaryClass =

View on Pith Pith review arXiv

[248] [263]

Counting Little Red Dots at z < 4 with Ground-based Surveys and Spectroscopic Follow-up. , keywords =. doi:10.3847/1538-4357/ae4596 , archivePrefix =. 2504.08032 , primaryClass =

View on Pith Pith review arXiv

[249] [264]

Super-Eddington Accretion of Black Holes in Early Nuclear Bursts Gives Birth to Little Red Dots. , keywords =. doi:10.3847/2041-8213/ae909e , archivePrefix =. 2605.31077 , primaryClass =

View on Pith Pith review arXiv

[250] [265]

Zhuang, Ming-Yang and Li, Junyao and Shen, Yue and Lin, Xiaojing and Shapley, Alice E. and Wang, Feige and Wu, Qiaoya and Yang, Qian , title =. , abstract =. 2026 , month =. doi:10.3847/1538-4357/ae3612 , url =

View on Pith doi:10.3847/1538-4357/ae3612 2026

[251] [266]

Discovery of a Little Red Dot candidate at z 10 in COSMOS-Web based on MIRI-NIRCam selection , author=. 2025 , eprint=

View on Pith 2025

[252] [267]

The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time. arXiv e-prints , keywords =. doi:10.48550/arXiv.2604.07138 , archivePrefix =. 2604.07138 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2604.07138

[253] [268]

(LRDs) ^2 : The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample. arXiv e-prints , keywords =. doi:10.48550/arXiv.2605.21574 , archivePrefix =. 2605.21574 , primaryClass =

View on Pith Pith review arXiv doi:10.48550/arxiv.2605.21574

[254] [269]

Little Red Dots as the Very First Activity of Black Hole Growth. , keywords =. doi:10.3847/2041-8213/adea66 , archivePrefix =. 2503.05537 , primaryClass =

View on Pith Pith review arXiv

[255] [270]

X-Ray View of Little Red Dots: Do They Host Supermassive Black Holes?. , keywords =. doi:10.3847/2041-8213/ad5669 , archivePrefix =. 2404.19010 , primaryClass =

View on Pith Pith review arXiv

[256] [271]

Furtak, Lukas J. and Secunda, Amy R. and Greene, Jenny E. and Zitrin, Adi and Labbé, Ivo and Golubchik, Miriam and Bezanson, Rachel and Kokorev, Vasily and Atek, Hakim and Brammer, Gabriel B. and Chemerynska, Iryna and Cutler, Sam E. and Dayal, Pratika and Feldmann, Robert and Fujimoto, Seiji and Glazebrook, Karl and Leja, Joel and Ma, Yilun and Matthee, ...

View on Pith

[257] [272]

Kokubo, Mitsuru and Harikane, Yuichi , title =. , abstract =. 2025 , month =. doi:10.3847/1538-4357/ae119e , url =

View on Pith doi:10.3847/1538-4357/ae119e 2025

[258] [273]

The GlimmIr: Spectroscopic Variability in a z 7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions , author=. 2026 , eprint=

View on Pith 2026

[259] [274]

Zhang, Zijian and Jiang, Linhua and Liu, Weiyang and Ho, Luis C. , title =. , abstract =. 2025 , month =. doi:10.3847/1538-4357/adcb3e , url =

View on Pith doi:10.3847/1538-4357/adcb3e 2025

[260] [275]

Jiang, Linhua and Fan, Xiaohui and Brandt, W. N. and Carilli, Chris L. and Egami, Eiichi and Hines, Dean C. and Kurk, Jaron D. and Richards, Gordon T. and Shen, Yue and Strauss, Michael A. and Vestergaard, Marianne and Walter, Fabian , year=. Dust-free quasars in the early Universe , volume=. Nature , publisher=. doi:10.1038/nature08877 , number=

View on Pith doi:10.1038/nature08877

[261] [276]

Lyu, Jianwei and Rieke, G. H. and Shi, Yong , title =. , abstract =. 2017 , month =. doi:10.3847/1538-4357/835/2/257 , url =

View on Pith doi:10.3847/1538-4357/835/2/257 2017

[262] [277]

The spectral energy distributions of active galactic nuclei. , keywords =. doi:10.1093/mnras/stz2324 , archivePrefix =. 1908.03720 , primaryClass =

View on Pith Pith review arXiv 1908

[263] [278]

Son, Suyeon and Kim, Minjin and Ho, Luis C. , title =. , abstract =. 2023 , month =. doi:10.3847/1538-4357/ace165 , url =

View on Pith doi:10.3847/1538-4357/ace165 2023

[264] [279]

Lyu, Jianwei and Rieke, George , year=. Infrared Spectral Energy Distribution and Variability of Active Galactic Nuclei: Clues to the Structure of Circumnuclear Material , volume=. Universe , publisher=. doi:10.3390/universe8060304 , number=

View on Pith doi:10.3390/universe8060304

[265] [280]

FORGE'd in FIRE: Resolving the End of Star Formation and Structure of AGN Accretion Disks from Cosmological Initial Conditions. The Open Journal of Astrophysics , keywords =. doi:10.21105/astro.2309.13115 , archivePrefix =. 2309.13115 , primaryClass =

View on Pith arXiv

[266] [281]

High-redshift clumpy discs and bulges in cosmological simulations. , keywords =. doi:10.1111/j.1365-2966.2010.16433.x , archivePrefix =. 0907.3271 , primaryClass =

View on Pith arXiv 2010

[267] [282]

Hot-dust-poor Type 1 Active Galactic Nuclei in the COSMOS Survey. , keywords =. doi:10.1088/2041-8205/724/1/L59 , archivePrefix =. 1009.3276 , primaryClass =

View on Pith Pith review arXiv

[268] [283]

Lyu, Jianwei and Alberts, Stacey and Rieke, George H. and Shivaei, Irene and Pérez-González, Pablo G. and Sun, Fengwu and Hainline, Kevin N. and Baum, Stefi and Bonaventura, Nina and Bunker, Andrew J. and Egami, Eiichi and Eisenstein, Daniel J. and Florian, Michael and Ji, Zhiyuan and Johnson, Benjamin D. and Morrison, Jane and Rieke, Marcia and Robertson...

View on Pith 2024

[269] [284]

Molecular Gas in z -0.5ex 6 Quasar Host Galaxies. , keywords =. doi:10.1088/0004-637X/714/1/699 , archivePrefix =. 1002.1561 , primaryClass =

View on Pith Pith review arXiv

[270] [285]

Enhanced star formation in z 6 quasar companions. , keywords =. doi:10.1093/mnras/stac978 , archivePrefix =. 2204.03658 , primaryClass =

View on Pith Pith review arXiv

[271] [286]

HYPerluminous quasars at the Epoch of ReionizatION (HYPERION): A new regime for the X-ray nuclear properties of the first quasars. , keywords =. doi:10.1051/0004-6361/202346795 , archivePrefix =. 2305.02347 , primaryClass =

View on Pith Pith review arXiv

[272] [287]

HYPERION. Shedding light on the first luminous quasars: A correlation between UV disc winds and X-ray continuum. , keywords =. doi:10.1051/0004-6361/202449662 , archivePrefix =. 2410.12786 , primaryClass =

View on Pith arXiv

[273] [288]

Systematic broad-band X-ray study of super-Eddington accretion on to supermassive black holes - I. X-ray continuum. , keywords =. doi:10.1093/mnras/stac3590 , archivePrefix =. 2212.06183 , primaryClass =

View on Pith Pith review arXiv

[274] [289]

The extreme properties of the nearby hyper-Eddington accreting active galactic nucleus in IRAS 04416+1215. , keywords =. doi:10.1093/mnras/stab3152 , archivePrefix =. 2109.02573 , primaryClass =

View on Pith Pith review arXiv

[275] [290]

An Investigation into the Selection and Colors of Little Red Dots and Active Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/ad9920 , archivePrefix =. 2410.00100 , primaryClass =

View on Pith Pith review arXiv

[276] [291]

Tee, Wei Leong and Fan, Xiaohui and Wang, Feige and Yang, Jinyi , title =. , abstract =. 2025 , month =. doi:10.3847/2041-8213/adc5e3 , url =

View on Pith doi:10.3847/2041-8213/adc5e3 2025

[277] [292]

The Sloan Digital Sky Survey: Technical Summary. , keywords =. doi:10.1086/301513 , archivePrefix =. astro-ph/0006396 , primaryClass =

View on Pith Pith review arXiv

[278] [293]

Composite Quasar Spectra from the Sloan Digital Sky Survey. , keywords =. doi:10.1086/321167 , archivePrefix =. astro-ph/0105231 , primaryClass =

View on Pith Pith review arXiv

[279] [294]

Glikman, Eilat and Helfand, David J. and White, Richard L. , title =. , abstract =. 2006 , month =. doi:10.1086/500098 , url =

View on Pith doi:10.1086/500098 2006

[280] [295]

CIGALE: a python Code Investigating GALaxy Emission⋆ , DOI= "10.1051/0004-6361/201834156", url= "https://doi.org/10.1051/0004-6361/201834156", journal =

View on Pith Pith review doi:10.1051/0004-6361/201834156

[281] [296]

Fitting AGN/Galaxy X-Ray-to-radio SEDs with CIGALE and Improvement of the Code. , keywords =. doi:10.3847/1538-4357/ac4971 , archivePrefix =. 2201.03718 , primaryClass =

View on Pith Pith review arXiv

[282] [297]

Yang(杨光), G and Boquien, M and Buat, V and Burgarella, D and Ciesla, L and Duras, F and Stalevski, M and Brandt, W N and Papovich, C , title =. , volume =. 2020 , month =. doi:10.1093/mnras/stz3001 , url =

View on Pith Pith review doi:10.1093/mnras/stz3001 2020

[283] [298]

Stalevski, Marko and Fritz, Jacopo and Baes, Maarten and Nakos, Theodoros and Popovi. 3D radiative transfer modelling of the dusty tori around active galactic nuclei as a clumpy two-phase medium , journal =. 2012 , month =. doi:10.1111/j.1365-2966.2011.19775.x , url =

View on Pith arXiv 2012

[284] [299]

Stalevski, Marko and Ricci, Claudio and Ueda, Yoshihiro and Lira, Paulina and Fritz, Jacopo and Baes, Maarten , title =. , volume =. 2016 , month =. doi:10.1093/mnras/stw444 , url =

View on Pith doi:10.1093/mnras/stw444 2016

[285] [300]

The first billion years according to JWST. Nature Astronomy , keywords =. doi:10.1038/s41550-025-02624-5 , archivePrefix =. 2405.21054 , primaryClass =

View on Pith Pith review arXiv