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REVIEW 4 major objections 3 minor 1 cited by

COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12

T0 review · 4 major / 3 minor · reviewed 2026-05-21 · grok-4.3

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Pith's one-line read Mean star-formation rates in the most massive galaxies fall along the Hubble sequence from irregular to spheroid types between redshifts 2 and 4.5, showing quenching began shortly after the sequence emerged.

desk verdict Stacking on COSMOS-Web gives new quantitative SFR trends along the Hubble sequence at 2<z<4.5 and a working dust evolution model, but the no-AGN assumption in the 850um stacks is the main thing to check. read the letter →

arxiv 2605.19661 v2 pith:A2MODIRD submitted 2026-05-19 astro-ph.GA

Stephen Eales , Matthew Smith , Tom Bakx , Jordan D'Silva , Feng-Yuan Frey Liu , Aparna Venkateshwaran This is my paper · ORCID
classification astro-ph.GA
keywords galaxyevolutionstarformationquenchingHubblesequencedustmasssubmillimetregalaxiesredshiftmorphology
checked against Cost.FunctionalEquationreality_from_one_distinction
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper stacks one of the deepest SCUBA-2 850-micron images using the COSMOS-Web catalogue to measure average dust emission and thus star-formation rates for galaxies split by stellar mass and morphology from redshift 0 to 12. For galaxies around 10^11 solar masses at 2

What carries the argument

Stacking of SCUBA-2 850-micron images for galaxies classified by morphology along the Hubble sequence and stellar mass

What would settle it

A measurement showing that AGN contribute more than a few tens of percent of the stacked 850-micron flux for the high-redshift samples, or a reclassification of the same galaxies with higher-resolution imaging that removes the systematic drop in star-formation rate from irregulars to spheroids.

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Extended reading notes

Core claim

Stacking analysis of 850-micron emission reveals that, for the most massive galaxies, mean star-formation rate declines along the Hubble sequence from irregular galaxies at one end to spheroids at the other in the redshift window 2<z<4.5. This trend indicates that quenching was already operating soon after the Hubble sequence appeared. The decline can be matched by a starvation model with a depletion time of 10^8.2 years, while the observed growth in number density of massive bulge-dominated and spheroidal galaxies between 1.5<z<4 is reproduced by the transformation of submillimetre galaxies. A chemical-evolution model built on the cosmic star-formation history and equal gas outflow rate is,

Load-bearing premise

The 850-micron stacked emission is produced almost entirely by dust heated by star formation with negligible AGN or other contamination, and that morphological types remain reliably assigned at redshifts above 2.

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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

4 major / 3 minor

Summary. This paper uses stacking of deep SCUBA-2 850μm imaging in the COSMOS-Web field to measure average submillimeter fluxes for galaxies binned by stellar mass (~10^11 M⊙) and morphological type (irregular, bulge-dominated, spheroid) from z=0 to z=12. It finds that mean SFRs rise with redshift and, at 2<z<4.5, decline along the Hubble sequence from ~280 M⊙/yr (irregulars) to ~80 M⊙/yr (spheroids), suggesting early quenching. A starvation model with ~10^8.2 yr depletion time reproduces the spheroid trend, while SMG evolution matches the rise in massive spheroid number densities at 1.5<z<4. Dust-to-stellar mass ratios increase to z~8, and a chemical evolution model with outflow rate = SFR reproduces the mean dust density evolution.

Significance. Should the results prove robust against systematics, they would strengthen evidence for quenching processes operating soon after the Hubble sequence forms at high redshift and provide empirical constraints on dust production and evolution models. The stacking technique enables statistical measurements for faint high-z sources, and the model comparisons offer testable predictions, though the parameter choices limit the independence of the fits.

major comments (4)
  1. [Abstract and stacking analysis] No error bars or uncertainty estimates are provided for the mean SFR values (e.g., the ~280 to ~80 M⊙ yr⁻¹ decline at 2<z<4.5), which is essential to evaluate if the trend along the Hubble sequence is statistically significant or affected by sample variance.
  2. [Stacking analysis description] The central assumption that 850μm stacked flux is dominated by star-formation-heated dust with negligible AGN contribution is not tested, despite spheroids and bulge-dominated galaxies being more likely to host AGN; this could bias the SFR estimates upward for later Hubble types and undermine the quenching interpretation.
  3. [Morphological classification] No robustness checks or redshift-dependent reliability assessments are described for the morphological classifications used to split samples at z>2, where visual or parametric typing becomes challenging and could invalidate the Hubble sequence trends.
  4. [Chemical evolution model] The model reproduces the dust-to-stellar mass ratio and mean dust density 'remarkably accurately' only after setting the outflow rate equal to the star-formation rate; this parameterization choice reduces the result to a consistency check rather than an independent validation of the model.
minor comments (3)
  1. [Abstract] Typo: 'soar masses' should read 'solar masses'.
  2. [Methods] Details on galaxy sample selection, completeness corrections, and handling of source blending in the stacks are not provided, which are needed for reproducibility.
  3. [Figure captions] Figures showing the stacked images or SFR trends should include error bars and indicate the number of galaxies per bin.

Simulated Author's Rebuttal

4 responses · 0 unresolved

We thank the referee for their thoughtful and constructive report. We address each major comment below and have made revisions to strengthen the manuscript where possible.

read point-by-point responses

  1. Referee: [Abstract and stacking analysis] No error bars or uncertainty estimates are provided for the mean SFR values (e.g., the ~280 to ~80 M⊙ yr⁻¹ decline at 2<z<4.5), which is essential to evaluate if the trend along the Hubble sequence is statistically significant or affected by sample variance.

    Authors: We agree that uncertainty estimates are necessary to assess the robustness of the reported trends. In the revised manuscript we have added bootstrap-derived uncertainties to the mean SFR values quoted in the abstract and main text, along with a brief discussion of sample variance and its impact on the Hubble-sequence trend at 2<z<4.5. revision: yes

  2. Referee: [Stacking analysis description] The central assumption that 850μm stacked flux is dominated by star-formation-heated dust with negligible AGN contribution is not tested, despite spheroids and bulge-dominated galaxies being more likely to host AGN; this could bias the SFR estimates upward for later Hubble types and undermine the quenching interpretation.

    Authors: We acknowledge the possibility of AGN contamination. However, multiple studies of submillimetre emission in high-redshift AGN hosts show that the 850 μm flux remains dominated by star-formation-heated dust. We have added a dedicated paragraph in the revised methods section citing this literature and noting that any residual AGN contribution would not reverse the observed decline along the Hubble sequence. A full empirical test would require new multi-wavelength data beyond the scope of the present work. revision: partial

  3. Referee: [Morphological classification] No robustness checks or redshift-dependent reliability assessments are described for the morphological classifications used to split samples at z>2, where visual or parametric typing becomes challenging and could invalidate the Hubble sequence trends.

    Authors: The COSMOS-Web imaging is sufficiently deep to permit reliable visual and parametric classifications up to z≈4.5. In the revised manuscript we have inserted a new subsection that quantifies classification reliability as a function of redshift, including agreement between visual and parametric methods and the fraction of ambiguous objects in each bin. These checks confirm that the Hubble-sequence trends remain robust within the redshift range used for the SFR comparison. revision: yes

  4. Referee: [Chemical evolution model] The model reproduces the dust-to-stellar mass ratio and mean dust density 'remarkably accurately' only after setting the outflow rate equal to the star-formation rate; this parameterization choice reduces the result to a consistency check rather than an independent validation of the model.

    Authors: We accept that fixing the outflow rate to equal the star-formation rate makes the exercise a consistency check rather than a fully independent test. In the revised text we have rephrased the relevant section to clarify the observational motivation for this choice and to present the model as demonstrating that a simple chemical-evolution framework with this physically motivated outflow prescription can reproduce the observed dust evolution, rather than claiming an independent validation. revision: yes

Circularity Check

1 steps flagged · score 6.0 of 10

Chemical evolution model 'reproduction' of dust ratios is forced by setting outflow rate equal to SFR

  1. fitted input called prediction [abstract (side-project paragraph)]
    "We show that a chemical evolution model based on the `star-formation history' of the universe, with a gas outflow rate equal to the star-formation rate, can explain the monotonic rise in the dust-to-stellar mass ratio and reproduce the relationship between mean dust density and redshift remarkably accurately."

    The model is stated to reproduce the observed dust-to-stellar mass ratio and mean dust density once the outflow rate is set equal to the star-formation rate. This parameter choice is tuned to the quantities derived from the paper's own stacking results, so the match is achieved by construction rather than emerging as an independent prediction from the model.

full rationale

The paper derives mean dust-to-stellar mass ratios and dust densities from 850μm stacking, then presents a chemical evolution model that matches these quantities 'remarkably accurately' after explicitly setting the outflow rate equal to the star-formation rate. This choice is a direct modeling input rather than an independent prediction or first-principles derivation, reducing the claimed explanatory success to a fit by construction. No other circular steps are identified in the observational stacking or morphological analysis.

Assumptions & free parameters 2 free parameters · 2 assumptions · 0 invented entities

The central claims rest on standard submillimeter astronomy assumptions plus two explicit modeling choices (depletion timescale and outflow scaling) introduced to match the data.

free parameters (2)
  • starvation depletion time = ~10^{8.2} years
    Specific value of ~10^{8.2} years chosen to reproduce the observed SFR decline for spheroidal galaxies.
  • gas outflow rate scaling = equal to SFR
    Set equal to the star-formation rate in the chemical evolution model to match dust observations.
assumptions (2)
  • domain assumption 850-micron flux density traces dust emission heated by star formation
    Invoked to convert stacked submillimeter flux to star-formation rate.
  • domain assumption Morphological classifications remain reliable at z>2
    Required to bin galaxies by Hubble sequence type in the stacking analysis.

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Cite this review

Pith. "Pith review of COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12." pith.science (2026). https://pith.science/paper/A2MODIRD

@misc{pith2026260519661,
  author       = {Pith},
  title        = {Pith review of: COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/A2MODIRD}},
  note         = {Machine review of arXiv:2605.19661}
}
read the original abstract

We have carried out a stacking analysis with the COSMOS-Web catalogue on one of the deepest ever SCUBA-2 images at 850 microns, allowing us to estimate the mean submillimetre flux density for samples of galaxies split by stellar mass and morphological class over the redshift range 0<z<12. For all morphological classes, the mean star-formation rate estimated from the dust emission increases with redshift, reaching a value for the most massive galaxies (~10^11 soar masses) of >~80 solar masses per year at 2 < z < 4.5. In this redshift range, the mean star-formation rate for these galaxies falls along the Hubble sequence from ~280 solar masses per year for irregular galaxies at one end to ~80 solar masses per year for spheroids at the other end, which shows that quenching was already happening shortly after the emergence of the Hubble sequence. The decrease in the star-formation rate for the spheroidal galaxies can be reproduced with a `starvation' quenching model with a depletion time of ~10^{8.2} years. We also show that the transformation of `submillimetre galaxies' can reproduce the growth in number-density of massive bulge-dominated and spheroidal galaxies over the redshift range 1.5 <z < 4. As a side-project, we have used our stacking results to show that the ratio of dust mass to stellar mass in galaxies increases with redshift out to z~8 and to determine the relationship between the mean density of dust and redshift in the range 0 < z <12. We show that a chemical evolution model based on the `star-formation history' of the universe, with a gas outflow rate equal to the star-formation rate, can explain the monotonic rise in the dust-to-stellar mass ratio and reproduce the relationship between mean dust density and redshift remarkably accurately.

Figures

Figures reproduced from arXiv: 2605.19661 by the authors.

Figure 1
Figure 1. Images showing the signal-to-noise of our measurements of the mean 850-𝜇m flux density of 70 samples of galaxies, with the results from the basic stacking method shown above and from SIMSTACK shown below. The annotation shows the redshift and mass range for each sample. Each pixel in each image represents a different offset from the COSMOS-Web positions, with the zero-offset position being in the centre. The images … view at source ↗
Figure 2
Figure 2. Mean flux density at 850 𝜇m versus mass for each redshift interval. The mauve points are the values measured with the basic stacking method. The cyan points are the values measured with SIMSTACK. The two sets have been offset by 0.1 in log10 (M∗ ), to prevent an overlap. The horizontal dashed line at a flux density of 0.1 mJy has been drawn to aid comparison between the panels. The limits are 3𝜎 upper limits. z > 2 … view at source ↗
Figure 3
Figure 3. Mean flux density at 850 𝜇m estimated with SIMSTACK (§2.4) for star-forming galaxies (mauve) and quiescent galaxies (cyan) plotted against stellar mass for the 14 redshift intervals. The two sets of points have been offset by 0.1 in log10 (M∗ ) so that they don’t overlap. The horizontal dashed line at a flux density of 0.1 mJy has been drawn to aid comparison between the panels. The upper limits are 3𝜎 upper limits.… view at source ↗
Figures from the paper (12 more)
Figure 4
Figure 4. Figure 4: Mean flux density at 850 𝜇m estimated with SIMSTACK for the four different morphological classes from Huertas-Company et al. (2025): irregular galaxies–green; disk-dominated galaxies–blue; bulge-dominated galaxies–cyan; spheroids–red. The horizontal dashed line at 0.1 …
Figure 5
Figure 5. Figure 5: The mean ratio of dust mass to stellar mass versus stellar mass for the 14 redshift intervals. The coloured symbols show the results for the three temperature models: blue–COLD; red–STAR-FORMER; cyan–EVOLVE. The three sets of points have been offset by ±0.1 along the x…
Figure 6
Figure 6. Figure 6: The mean ratio of dust mass to stellar mass versus redshift for the five intervals of stellar mass. The coloured symbols are for the different temperature models: blue–COLD; red–STAR-FORMER; cyan–EVOLVE. The sets of points have been offset by ±0.1 in redshift for great…
Figure 7
Figure 7. Figure 7: shows the weighted mean value of the five values for the dust-to-stellar mass ratio in each redshift interval plotted against redshift. We have calculated these weighted means separately for each temperature model and used the errors on dust-to-stellar mass ratios show…
Figure 8
Figure 8. Figure 8: The mean dust density versus redshift for COLD (blue), STAR￾FORMER (red) and EVOLVE (cyan). The purple circles show our estimates based on the ground-based surveys of COSMOS (Eales & Ward 2024). The grey crosses show the estimates of Magnelli et al. (2020). A compariso…
Figure 9
Figure 9. Figure 9: Estimated star-formation rate versus redshift for a galaxy with an 850-𝜇m flux density of 1 mJy (see text for details) and for the temperature models: EVOLVE (cyan) and STAR-FORMER (red). We have not included COLD because any galaxy containing OB stars must contain som…
Figure 10
Figure 10. Figure 10: Mean value of the star-formation rate estimated from the bolometric dust luminosity plotted against redshift, with the colour of the symbol showing the morphological class: red–spheroids; blue–disk-dominated galaxies; green–irregular galaxies; cyan–bulge-dominated gal…
Figure 11
Figure 11. Figure 11: Ratio of the mean star-formation rate estimate from the dust emission to the mean of the COSMOS-Web estimates from the UV-to-near-IR SED for the same sample of galaxies. The continuous horizontal line shows where the two estimates are equal and the two dashed lines sh…
Figure 12
Figure 12. Figure 12: Mean star-formation rate estimated from the dust emission for galaxies in the four morphological classs in the redshift range 2 < 𝑧 < 4.5 and 10.0 < log10M∗ < 10.5 (blue), 10.5 < log10M∗ < 11.0 (red) and 11.0 < log10M∗ < 11.5 (mauve). The horizontal dashed lines show …
Figure 13
Figure 13. Figure 13: Histograms of the specific star-formation rate for the four morpho￾logical classes in the redshift range 2 < z < 4.5 and with 11.5 > log10M∗ > 10.5. In this case, the star-formation rates are the values estimated from UV￾to-near-IR photometry in the COSMOS-Web catalog…
Figure 15
Figure 15. Figure 15: shows the results for Λ = 0, Λ = 1 and Λ = 2. The 0 2 4 6 8 10 12 Redshift 10 4 10 3 10 2 10 1 10 0 10 1 D u s t D e n s i ty/ 1 0 5 M M p c 3 COLD STAR-FORMER EVOLVE [PITH_FULL_IMAGE:figures/full_fig_p020_15.png]
Figure 16
Figure 16. Figure 16: The mean density of dust-traced gas versus redshift for COLD (blue), STAR-FORMER (red) and EVOLVE (cyan) and from our previous study (purple). The solid line shows the ‘star-formation history of the uni￾verse’, an analytic relationship derived from empirical estimates…

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  • IndisputableMonolith/Cost/FunctionalEquation.lean washburn_uniqueness_aczel unclear
    ?
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    Relation between the paper passage and the cited Recognition theorem.

    mean star-formation rate ... falls along the Hubble sequence from ~280 ... to ~80 ... starvation quenching model with a depletion time of ~10^8.2 years ... chemical evolution model ... gas outflow rate equal to the star-formation rate

  • IndisputableMonolith/Foundation/RealityFromDistinction.lean reality_from_one_distinction unclear
    ?
    unclear

    Relation between the paper passage and the cited Recognition theorem.

    stacking analysis ... morphological classes ... dust mass to stellar mass ... mean density of dust and redshift

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Works this paper leans on

175 extracted references · 175 canonical work pages · cited by 1 Pith paper

  1. [1]

    ISM masses and the star formation law at Z = 1 to 6 // ALMA observations of dust continuum in 145 galaxies in the COSMOS survey field

    ISM Masses and the Star formation Law at Z = 1 to 6: ALMA Observations of Dust Continuum in 145 Galaxies in the COSMOS Survey Field. , keywords =. doi:10.3847/0004-637X/820/2/83 , archivePrefix =. 1511.05149 , primaryClass =

    work page Pith review arXiv doi:10.3847/0004-637x/820/2/83

  2. [2]

    The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time

    The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time. , keywords =. doi:10.1146/annurev-astro-082812-141034 , archivePrefix =. 2003.06245 , primaryClass =

    work page doi:10.1146/annurev-astro-082812-141034 2003

  3. [3]

    , keywords =

    Metal factories in the early Universe. , keywords =. doi:10.1093/mnras/stae1564 , archivePrefix =. 2303.07376 , primaryClass =

    work page doi:10.1093/mnras/stae1564

  4. [4]

    The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions

    The Evolving Interstellar Medium of Star-forming Galaxies since z = 2 as Probed by Their Infrared Spectral Energy Distributions. , keywords =. doi:10.1088/0004-637X/760/1/6 , archivePrefix =. 1210.1035 , primaryClass =

    work page Pith review arXiv doi:10.1088/0004-637x/760/1/6

  5. [5]

    The evolution of the dust temperatures of galaxies in the SFR$-M_{\ast}$ plane up to $z$$\,\thicksim\,$$2$

    The evolution of the dust temperatures of galaxies in the SFR-M _ * plane up to z 2. , keywords =. doi:10.1051/0004-6361/201322217 , archivePrefix =. 1311.2956 , primaryClass =

    work page Pith review arXiv doi:10.1051/0004-6361/201322217

  6. [6]

    An ALMA Survey of Submillimetre Galaxies in the Extended Chandra Deep Field South: The Far-Infrared Properties of SMGs

    An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs. , keywords =. doi:10.1093/mnras/stt2273 , archivePrefix =. 1310.6362 , primaryClass =

    work page Pith review arXiv doi:10.1093/mnras/stt2273

  7. [7]

    Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

    Evolution of the dust emission of massive galaxies up to z = 4 and constraints on their dominant mode of star formation. , keywords =. doi:10.1051/0004-6361/201425031 , archivePrefix =. 1409.5796 , primaryClass =

    work page Pith review arXiv doi:10.1051/0004-6361/201425031

  8. [8]

    J., Lewis, A

    The Space Density of Luminous Dusty Star-forming Galaxies at z > 4: SCUBA-2 and LABOCA Imaging of Ultrared Galaxies from Herschel-ATLAS. , keywords =. doi:10.3847/0004-637X/832/1/78 , archivePrefix =. 1611.00762 , primaryClass =

    work page Pith review arXiv doi:10.3847/0004-637x/832/1/78

Show all 175 references
  1. [9]

    , keywords =

    Are High-redshift Galaxies Hot? Temperature of z > 5 Galaxies and Implications for Their Dust Properties. , keywords =. doi:10.3847/1538-4357/aa886c , archivePrefix =. 1708.07842 , primaryClass =

    doi arXiv

  2. [10]

    , keywords =

    Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0 < z < 4. , keywords =. doi:10.1051/0004-6361/201731506 , archivePrefix =. 1710.10276 , primaryClass =

    doi arXiv

  3. [11]

    , keywords =

    The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5-10 UV-selected Galaxies and the Implied High-redshift Star Formation History. , keywords =. doi:10.3847/1538-4357/abb830 , archivePrefix =. 2009.10727 , primaryClass =

    2009 doi

  4. [12]

    , keywords =

    The early Universe was dust-rich and extremely hot. , keywords =. doi:10.1093/mnrasl/slac075 , archivePrefix =. 2203.14312 , primaryClass =

    doi

  5. [13]

    , keywords =

    An empirical study of dust properties at the earliest epochs. , keywords =. doi:10.1093/mnras/stad1470 , archivePrefix =. 2305.09714 , primaryClass =

    doi

  6. [14]

    , keywords =

    Cold Dust in Galaxies. , keywords =. doi:10.1086/167341 , adsurl =

    doi

  7. [15]

    , keywords =

    An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies. , keywords =. doi:10.3847/1538-4357/aacd11 , archivePrefix =. 1806.05603 , primaryClass =

    doi arXiv

  8. [16]

    , keywords =

    Discovery of Four Apparently Cold Dusty Galaxies at z = 3.62-5.85 in the COSMOS Field: Direct Evidence of Cosmic Microwave Background Impact on High-redshift Galaxy Observables. , keywords =. doi:10.3847/1538-4357/ab55d6 , archivePrefix =. 1906.00040 , primaryClass =

    1906 doi

  9. [17]

    , keywords =

    An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies. , keywords =. doi:10.1093/mnras/staa769 , archivePrefix =. 1910.07524 , primaryClass =

    1910 doi

  10. [18]

    , keywords =

    No Redshift Evolution of Galaxies' Dust Temperatures Seen from 0 < z < 2. , keywords =. doi:10.3847/1538-4357/ac6270 , archivePrefix =. 2203.16655 , primaryClass =

    doi

  11. [19]

    , keywords =

    On the Effect of the Cosmic Microwave Background in High-redshift (Sub-)millimeter Observations. , keywords =. doi:10.1088/0004-637X/766/1/13 , archivePrefix =. 1302.0844 , primaryClass =

    doi arXiv

  12. [20]

    450- m data: evidence for cold dust in bright IRAS galaxies

    The SCUBA Local Universe Galaxy Survey - II. 450- m data: evidence for cold dust in bright IRAS galaxies. , keywords =. doi:10.1046/j.1365-8711.2001.04789.x , archivePrefix =. astro-ph/0106362 , primaryClass =

    2001 doi

  13. [21]

    , keywords =

    On the dust temperatures of high-redshift galaxies. , keywords =. doi:10.1093/mnras/stz2134 , archivePrefix =. 1902.10727 , primaryClass =

    1902 doi

  14. [22]

    , keywords =

    Little evolution of dust emissivity in bright infrared galaxies from 2 < z < 6. , keywords =. doi:10.1093/mnras/stae405 , archivePrefix =. 2402.05182 , primaryClass =

    doi

  15. [23]

    Millimetre photometry of gravitational lens candidates

    The bright extragalactic ALMA redshift survey (BEARS) - II. Millimetre photometry of gravitational lens candidates. , keywords =. doi:10.1093/mnras/stac3771 , archivePrefix =. 2301.02584 , primaryClass =

    doi

  16. [24]

    , keywords =

    Realistic multitemperature dust: how well can we constrain the dust properties of high-redshift galaxies?. , keywords =. doi:10.1093/mnras/staf897 , archivePrefix =. 2505.20105 , primaryClass =

    doi

  17. [25]

    , keywords =

    The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations. , keywords =. doi:10.1093/mnras/stx2267 , archivePrefix =. 1709.01514 , primaryClass =

    doi arXiv

  18. [26]

    , keywords =

    H-ATLAS: estimating redshifts of Herschel sources from sub-mm fluxes. , keywords =. doi:10.1093/mnras/stt1369 , archivePrefix =. 1308.5681 , primaryClass =

    doi arXiv

  19. [27]

    , keywords =

    HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift. , keywords =. doi:10.1088/0004-637X/779/1/32 , archivePrefix =. 1304.0446 , primaryClass =

    doi arXiv

  20. [28]

    , keywords =

    Can Dust Emission be Used to Estimate the Mass of the Interstellar Medium in Galaxies A Pilot Project with the Herschel Reference Survey. , keywords =. doi:10.1088/0004-637X/761/2/168 , archivePrefix =. 1202.0547 , primaryClass =

    doi arXiv

  21. [29]

    , keywords =

    The rise and fall of dust in the Universe. , keywords =. doi:10.1093/mnras/stae403 , archivePrefix =. 2402.05181 , primaryClass =

    doi

  22. [30]

    , keywords =

    The interstellar medium of quiescent galaxies and its evolution with time. , keywords =. doi:10.1051/0004-6361/202039280 , archivePrefix =. 2101.04700 , primaryClass =

    doi

  23. [31]

    , keywords =

    ALMA uncovers the [C II] emission and warm dust continuum in a z = 8.31 Lyman break galaxy. , keywords =. doi:10.1093/mnras/staa509 , archivePrefix =. 2001.02812 , primaryClass =

    2001 doi

  24. [32]

    , keywords =

    A Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution. , keywords =. doi:10.1086/311017 , archivePrefix =. astro-ph/9708135 , primaryClass =

    doi arXiv

  25. [33]

    , keywords =

    High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey. , keywords =. doi:10.1038/28328 , archivePrefix =. astro-ph/9806297 , primaryClass =

    doi arXiv

  26. [34]

    , keywords =

    The Canada-UK Deep Submillimeter Survey: First Submillimeter Images, the Source Counts, and Resolution of the Background. , keywords =. doi:10.1086/307069 , archivePrefix =. astro-ph/9808040 , primaryClass =

    doi arXiv

  27. [35]

    The Canada-United Kingdom Deep Submillimeter Survey. II. First Identifications, Redshifts, and Implications for Galaxy Evolution. , keywords =. doi:10.1086/307310 , archivePrefix =. astro-ph/9901047 , primaryClass =

    doi arXiv

  28. [36]

    , keywords =

    Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations. , keywords =. doi:10.3847/1538-4357/ab14e8 , archivePrefix =. 1904.11556 , primaryClass =

    1904 doi arXiv

  29. [37]

    A unified picture from low-metallicity systems to the Galaxy

    Dust-depletion sequences in damped Lyman- absorbers. A unified picture from low-metallicity systems to the Galaxy. , keywords =. doi:10.1051/0004-6361/201527895 , archivePrefix =. 1608.08621 , primaryClass =

    doi arXiv

  30. [38]

    METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. IV. Calibration of Dust Depletions versus Abundance Ratios in the Milky Way and Magellanic Clouds and Application to Damped Ly Systems. , keywords =. doi:10.3847/1538-4357/ac7713...

    doi

  31. [39]

    , keywords =

    Dust, CO, and [C I]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time. , keywords =. doi:10.1093/mnras/stac2098 , archivePrefix =. 2208.01622 , primaryClass =

    doi

  32. [40]

    , keywords =

    The CO-to-H _ 2 Conversion Factor. , keywords =. doi:10.1146/annurev-astro-082812-140944 , archivePrefix =. 1301.3498 , primaryClass =

    doi arXiv

  33. [41]

    , keywords =

    The Evolution of Interstellar Medium Mass Probed by Dust Emission: ALMA Observations at z = 0.3-2. , keywords =. doi:10.1088/0004-637X/783/2/84 , archivePrefix =. 1401.2987 , primaryClass =

    doi arXiv

  34. [42]

    Astroparticle Physics , keywords =

    The extragalactic background light and the gamma-ray opacity of the universe. Astroparticle Physics , keywords =. doi:10.1016/j.astropartphys.2012.09.003 , archivePrefix =. 1209.4661 , primaryClass =

    2012 doi arXiv

  35. [43]

    , keywords =

    The Cosmic Evolution Survey (COSMOS): Overview. , keywords =. doi:10.1086/516585 , archivePrefix =. astro-ph/0612305 , primaryClass =

    doi arXiv

  36. [44]

    , keywords =

    The East Asian Observatory SCUBA-2 Survey of the COSMOS Field: Unveiling 1147 Bright Sub-millimeter Sources across 2.6 Square Degrees. , keywords =. doi:10.3847/1538-4357/ab23ff , archivePrefix =. 1912.02229 , primaryClass =

    1912 doi

  37. [45]

    , keywords =

    S2COSMOS: Evolution of gas mass with redshift using dust emission. , keywords =. doi:10.1093/mnras/staa609 , archivePrefix =. 2003.01727 , primaryClass =

    2003 doi

  38. [46]

    Thirteen billion years of stellar mass assembly in ten snapshots

    The COSMOS2015 galaxy stellar mass function . Thirteen billion years of stellar mass assembly in ten snapshots. , keywords =. doi:10.1051/0004-6361/201730419 , archivePrefix =. 1701.02734 , primaryClass =

    doi arXiv

  39. [47]

    , keywords =

    COSMOS-Web: An Overview of the JWST Cosmic Origins Survey. , keywords =. doi:10.3847/1538-4357/acc2bc , archivePrefix =. 2211.07865 , primaryClass =

    doi

  40. [48]

    arXiv e-prints , keywords =

    COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging. arXiv e-prints , keywords =. doi:10.48550/arXiv.2506.03243 , archivePrefix =. 2506.03243 , primaryClass =

    doi

  41. [49]

    arXiv e-prints , keywords =

    COSMOS-Web: The emergence of the Hubble Sequence. arXiv e-prints , keywords =. doi:10.48550/arXiv.2502.03532 , archivePrefix =. 2502.03532 , primaryClass =

    doi

  42. [50]

    , keywords =

    A high-resolution investigation of the multiphase ISM in a galaxy during the first two billion years. , keywords =. doi:10.1093/mnras/stab3569 , archivePrefix =. 2112.03936 , primaryClass =

    doi

  43. [51]

    , keywords =

    Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA. , keywords =. doi:10.1093/mnras/stv1442 , archivePrefix =. 1503.08720 , primaryClass =

    doi arXiv

  44. [52]

    , keywords =

    COSMOS-Web: Intrinsically Luminous z 10 Galaxy Candidates Test Early Stellar Mass Assembly. , keywords =. doi:10.3847/1538-4357/ad2075 , archivePrefix =. 2308.10932 , primaryClass =

    doi

  45. [53]

    , keywords =

    Hydrodynamical Simulations of the Galaxy Population: Enduring Successes and Outstanding Challenges. , keywords =. doi:10.1146/annurev-astro-041923-043618 , archivePrefix =. 2309.17075 , primaryClass =

    doi

  46. [54]

    , year = 1972, month = dec, volume =

    Galactic Bridges and Tails. , year = 1972, month = dec, volume =. doi:10.1086/151823 , adsurl =

    1972 doi

  47. [55]

    , keywords =

    The Herschel Reference Survey: Dust in Early-type Galaxies and across the Hubble Sequence. , keywords =. doi:10.1088/0004-637X/748/2/123 , archivePrefix =. 1112.1408 , primaryClass =

    doi arXiv

  48. [56]

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

    2015 doi arXiv

  49. [57]

    , keywords =

    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 =

    doi

  50. [58]

    arXiv e-prints , keywords =

    Low dust mass and high star-formation efficiency at z>12 from deep ALMA observations. arXiv e-prints , keywords =. doi:10.48550/arXiv.2501.19384 , archivePrefix =. 2501.19384 , primaryClass =

    doi

  51. [59]

    arXiv e-prints , keywords =

    The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5 Source Catalog and Redshift Distribution. arXiv e-prints , keywords =. doi:10.48550/arXiv.2408.14546 , archivePrefix =. 2408.14546 , primaryClass =

    doi

  52. [60]

    , keywords =

    Deep ALMA redshift search of a z 12 GLASS-JWST galaxy candidate. , keywords =. doi:10.1093/mnras/stac3723 , archivePrefix =. 2208.13642 , primaryClass =

    doi

  53. [61]

    , keywords =

    BLAST: Resolving the Cosmic Submillimeter Background. , keywords =. doi:10.1088/0004-637X/707/2/1729 , archivePrefix =. 0904.1205 , primaryClass =

    doi arXiv

  54. [62]

    , keywords =

    Measuring star formation in high-z massive galaxies: a mid-infrared to submillimetre study of the GOODS NICMOS Survey sample. , keywords =. doi:10.1111/j.1365-2966.2012.20456.x , archivePrefix =. 1008.4359 , primaryClass =

    2012 doi

  55. [63]

    , keywords =

    COSMOS-Web: Stellar mass assembly in relation to dark matter halos across 0.2 < z < 12 of cosmic history. , keywords =. doi:10.1051/0004-6361/202452570 , archivePrefix =. 2410.08290 , primaryClass =

    doi

  56. [64]

    , keywords =

    Star Formation in the Milky Way and Nearby Galaxies. , keywords =. doi:10.1146/annurev-astro-081811-125610 , archivePrefix =. 1204.3552 , primaryClass =

    doi arXiv

  57. [65]

    , keywords =

    Star Formation in Galaxies Along the Hubble Sequence. , keywords =. doi:10.1146/annurev.astro.36.1.189 , archivePrefix =. astro-ph/9807187 , primaryClass =

    doi arXiv

  58. [66]

    , keywords =

    The dust emissivity index in infrared-bright galaxies at 1.5 < z < 4.2. , keywords =. doi:10.1093/mnras/staf816 , archivePrefix =. 2505.12141 , primaryClass =

    doi

  59. [67]

    z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies. II. Dust properties. , keywords =. doi:10.1051/0004-6361/202346804 , archivePrefix =. 2307.15747 , primaryClass =

    doi

  60. [68]

    , keywords =

    Herschel-ATLAS: rapid evolution of dust in galaxies over the last 5 billion years. , keywords =. doi:10.1111/j.1365-2966.2011.19363.x , archivePrefix =. 1012.5186 , primaryClass =

    2011 doi

  61. [69]

    , keywords =

    SCUBA observations of galaxies with metallicity measurements: a new method for determining the relation between submillimetre luminosity and dust mass. , keywords =. doi:10.1046/j.1365-8711.2002.05660.x , archivePrefix =. astro-ph/0204519 , primaryClass =

    2002 doi

  62. [70]

    , keywords =

    Measurements of the Dust Properties in z ≃ 1-3 Submillimeter Galaxies with ALMA. , keywords =. doi:10.3847/1538-4357/ac0ae0 , archivePrefix =. 2106.08566 , primaryClass =

    doi

  63. [71]

    , keywords =

    A simple model to interpret the ultraviolet, optical and infrared emission from galaxies. , keywords =. doi:10.1111/j.1365-2966.2008.13535.x , archivePrefix =. 0806.1020 , primaryClass =

    2008 doi

  64. [72]

    A Herschel [C ii] Galactic plane survey. I. The global distribution of ISM gas components. , keywords =. doi:10.1051/0004-6361/201321188 , archivePrefix =. 1304.7770 , primaryClass =

    doi arXiv

  65. [73]

    , keywords =

    Fermi Observations of Cassiopeia and Cepheus: Diffuse Gamma-ray Emission in the Outer Galaxy. , keywords =. doi:10.1088/0004-637X/710/1/133 , archivePrefix =. 0912.3618 , primaryClass =

    doi arXiv

  66. [74]

    Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the ``dark gas'' in our Galaxy. , keywords =. doi:10.1051/0004-6361/201116479 , archivePrefix =. 1101.2029 , primaryClass =

    doi arXiv

  67. [75]

    , keywords =

    Dust continuum, CO, and [C I] 1 - 0 lines: self-consistent H _ 2 mass estimates and the possibility of globally CO-'dark' galaxies at z = 0.35. , keywords =. doi:10.1093/mnras/staa3526 , archivePrefix =. 2111.09067 , primaryClass =

    doi

  68. [76]

    , keywords =

    Cosmic Star-Formation History. , keywords =. doi:10.1146/annurev-astro-081811-125615 , archivePrefix =. 1403.0007 , primaryClass =

    doi arXiv

  69. [77]

    arXiv e-prints , keywords =

    Galaxies and Black Holes in the First Billion Years. arXiv e-prints , keywords =. doi:10.48550/arXiv.2508.16948 , archivePrefix =. 2508.16948 , primaryClass =

    doi

  70. [78]

    , keywords =

    A Highly Consistent Framework for the Evolution of the Star-Forming ``Main Sequence'' from z -0.5ex 0-6. , keywords =. doi:10.1088/0067-0049/214/2/15 , archivePrefix =. 1405.2041 , primaryClass =

    doi arXiv

  71. [79]

    , keywords =

    Gas Regulation of Galaxies: The Evolution of the Cosmic Specific Star Formation Rate, the Metallicity-Mass-Star-formation Rate Relation, and the Stellar Content of Halos. , keywords =. doi:10.1088/0004-637X/772/2/119 , archivePrefix =. 1303.5059 , primaryClass =

    doi arXiv

  72. [80]

    The dynamics of the gas regulator model and the implied cosmic sSFR history

    From haloes to Galaxies - I. The dynamics of the gas regulator model and the implied cosmic sSFR history. , keywords =. doi:10.1093/mnras/stu1288 , archivePrefix =. 1402.5964 , primaryClass =

    doi arXiv

  73. [81]

    METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios versus Metallicity. , keywords =. doi:10.3847/1538-4357/ac5248 , archivePrefix =. 2202.04765 , primaryClass =

    doi

  74. [82]

    , year = 1990, month = oct, volume =

    General Constraints on the Effect of Gas Flows in the Chemical Evolution of Galaxies. , year = 1990, month = oct, volume =

    1990

  75. [83]

    , keywords =

    Maximum dust masses in galaxies. , keywords =. doi:10.1046/j.1365-8711.1998.01971.x , adsurl =

    1998 doi

  76. [84]

    , keywords =

    The implications of large dust masses at high redshifts: a first look at galactic evolution in the submillimetre waveband. , keywords =. doi:10.1093/mnras/280.4.1167 , adsurl =

    doi

  77. [85]

    The submillimetre background and source counts

    A robust method for investigating galactic evolution in the submillimetre waveband - II. The submillimetre background and source counts. , keywords =. doi:10.1093/mnras/286.3.732 , archivePrefix =. astro-ph/9609120 , primaryClass =

    doi arXiv

  78. [86]

    , keywords =

    De re metallica: the cosmic chemical evolution of galaxies. , keywords =. doi:10.1007/s00159-018-0112-2 , archivePrefix =. 1811.09642 , primaryClass =

    doi arXiv

  79. [87]

    Revisiting the Integrated Star Formation Law. II. Starbursts and the Combined Global Schmidt Law. , keywords =. doi:10.3847/1538-4357/abd3a2 , archivePrefix =. 2012.05363 , primaryClass =

    2012 doi

  80. [88]

    , keywords =

    GAMA/H-ATLAS: a meta-analysis of SFR indicators - comprehensive measures of the SFR-M _ * relation and cosmic star formation history at z < 0.4. , keywords =. doi:10.1093/mnras/stw1342 , archivePrefix =. 1606.06299 , primaryClass =

    doi arXiv

  81. [89]

    Herschel Exploitation of Local Galaxy Andromeda (HELGA). III. The Star Formation Law in M31. , keywords =. doi:10.1088/0004-637X/769/1/55 , archivePrefix =. 1303.6284 , primaryClass =

    doi arXiv

  82. [90]

    SCUBADive. I. JWST+ALMA Analysis of 289 Submillimeter Galaxies in COSMOS-web. , keywords =. doi:10.3847/1538-4357/ada357 , archivePrefix =. 2408.08346 , primaryClass =

    doi

  83. [91]

    , keywords =

    Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North. , keywords =. doi:10.1046/j.1365-8711.1999.02978.x , archivePrefix =. astro-ph/9902290 , primaryClass =

    1999 doi

  84. [92]

    , keywords =

    Stellar population synthesis at the resolution of 2003. , keywords =. doi:10.1046/j.1365-8711.2003.06897.x , archivePrefix =. astro-ph/0309134 , primaryClass =

    2003 doi

  85. [93]

    , keywords =

    Turbulent Gas in Lensed Planck-selected Starbursts at z 1-3.5. , keywords =. doi:10.3847/1538-4357/abcc01 , archivePrefix =. 2010.16231 , primaryClass =

    2010 doi

  86. [94]

    , keywords =

    Environment and self-regulation in galaxy formation. , keywords =. doi:10.1111/j.1365-2966.2010.16427.x , archivePrefix =. 0912.0259 , primaryClass =

    2010 doi

  87. [95]

    Submillimetre maps, sources and number counts

    The SCUBA 8-mJy survey - I. Submillimetre maps, sources and number counts. , keywords =. doi:10.1046/j.1365-8711.2002.05193.x , archivePrefix =. astro-ph/0107446 , primaryClass =

    2002 doi

  88. [96]

    , keywords =

    The star-formation history of the Universe from the stellar populations of nearby galaxies. , keywords =. doi:10.1038/nature02474 , archivePrefix =. astro-ph/0403293 , primaryClass =

    doi arXiv

  89. [97]

    , keywords =

    The Cosmic Evolution Early Release Science Survey (CEERS). , keywords =. doi:10.3847/2041-8213/adbbd3 , archivePrefix =. 2501.04085 , primaryClass =

    doi

  90. [98]

    , keywords =

    The Epochs of Early-Type Galaxy Formation as a Function of Environment. , keywords =. doi:10.1086/426932 , archivePrefix =. astro-ph/0410209 , primaryClass =

    doi arXiv

  91. [99]

    , keywords =

    Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift. , keywords =. doi:10.1038/28338 , archivePrefix =. astro-ph/9806317 , primaryClass =

    doi arXiv

  92. [100]

    Encyclopedia of Astrophysics , year = 2026, volume =

    Observations of the first galaxies in the Era of JWST. Encyclopedia of Astrophysics , year = 2026, volume =. doi:10.1016/B978-0-443-21439-4.00128-0 , adsurl =

    2026 doi

  93. [101]

    , keywords =

    Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z -0.5ex 2.5 to z -0.5ex 0.1. , keywords =. doi:10.1088/0004-637X/742/2/96 , archivePrefix =. 1107.0317 , primaryClass =

    doi arXiv

  94. [102]

    Nature Astronomy , keywords =

    The unexpectedly large dust and gas content of quiescent galaxies at z > 1.4. Nature Astronomy , keywords =. doi:10.1038/s41550-017-0352-5 , archivePrefix =. 1703.02207 , primaryClass =

    doi arXiv

  95. [103]

    , keywords =

    Quenching of star formation from a lack of inflowing gas to galaxies. , keywords =. doi:10.1038/s41586-021-03806-7 , archivePrefix =. 2109.10384 , primaryClass =

    doi

  96. [104]

    Quenching precedes bulge formation in dense environments but follows it in the field

    Euclid Quick Data Release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field. arXiv e-prints , keywords =

  97. [105]

    Exploring galaxy morphology across cosmic time through Sersic fits

    Euclid Quick Data Release (Q1). Exploring galaxy morphology across cosmic time through Sersic fits. arXiv e-prints , keywords =. doi:10.48550/arXiv.2503.15309 , archivePrefix =. 2503.15309 , primaryClass =

    doi

  98. [106]

    , keywords =

    Dusty galaxies in the Epoch of Reionization: simulations. , keywords =. doi:10.1093/mnras/sty552 , archivePrefix =. 1802.07772 , primaryClass =

    doi arXiv

  99. [107]

    Cosmic Sands. II. Challenges in Predicting and Measuring High-z Dust Temperatures. , keywords =. doi:10.3847/1538-4357/ad306c , archivePrefix =. 2306.07338 , primaryClass =

    doi

  100. [108]

    Earth, Planets and Space , keywords =

    Dust formation history of galaxies: A critical role of metallicity* for the dust mass growth by accreting materials in the interstellar medium. Earth, Planets and Space , keywords =. doi:10.5047/eps.2012.04.014 , archivePrefix =. 1206.0817 , primaryClass =

    2012 doi arXiv

  101. [109]

    Genesis and evolution of dust in galaxies in the early Universe. I. Modelling dust evolution in starburst galaxies. , keywords =. doi:10.1051/0004-6361/201015286 , archivePrefix =. 1011.3157 , primaryClass =

    doi arXiv

  102. [110]

    , keywords =

    Modeling Dust Evolution in Galaxies with a Multiphase, Inhomogeneous ISM. , keywords =. doi:10.3847/0004-637X/831/2/147 , archivePrefix =. 1608.04781 , primaryClass =

    doi arXiv

  103. [111]

    , keywords =

    Simulating the dust content of galaxies: successes and failures. , keywords =. doi:10.1093/mnras/stx467 , archivePrefix =. 1606.02714 , primaryClass =

    doi arXiv

  104. [112]

    , keywords =

    Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations. , keywords =. doi:10.1051/0004-6361/202449784 , archivePrefix =. 2402.18515 , primaryClass =

    doi

  105. [113]

    , keywords =

    Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models. , keywords =. doi:10.1093/mnras/stac695 , archivePrefix =. 2203.03686 , primaryClass =

    doi

  106. [114]

    , keywords =

    The dust content of galaxies from z = 0 to z = 9. , keywords =. doi:10.1093/mnras/stx1545 , archivePrefix =. 1609.08622 , primaryClass =

    doi arXiv

  107. [115]

    , keywords =

    Dust formation in early galaxies. , keywords =. doi:10.1046/j.1365-8711.2003.06681.x , archivePrefix =. astro-ph/0302566 , primaryClass =

    2003 doi

  108. [116]

    , keywords =

    Cosmic Evolution of Gas and Star Formation. , keywords =. doi:10.3847/1538-4357/aca1bc , archivePrefix =. 2211.07836 , primaryClass =

    doi

  109. [117]

    , keywords =

    Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift. , keywords =. doi:10.3847/1538-4357/aa61a0 , archivePrefix =. 1702.04729 , primaryClass =

    doi arXiv

  110. [118]

    , keywords =

    The Cold Interstellar Medium of Galaxies in the Local Universe. , keywords =. doi:10.1146/annurev-astro-021022-043545 , archivePrefix =. 2202.00690 , primaryClass =

    doi

  111. [119]

    , year = 1994, month = jan, volume =

    Physical Parameters along the Hubble Sequence. , year = 1994, month = jan, volume =. doi:10.1146/annurev.aa.32.090194.000555 , adsurl =

    1994 doi

  112. [120]

    , keywords =

    JWST's PEARLS: A JWST/NIRCam View of ALMA Sources. , keywords =. doi:10.3847/2041-8213/aca9d0 , archivePrefix =. 2210.08163 , primaryClass =

    doi

  113. [121]

    , keywords =

    JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon. , keywords =. doi:10.3847/2041-8213/ac98c6 , archivePrefix =. 2208.05296 , primaryClass =

    doi

  114. [122]

    , keywords =

    Galaxy And Mass Assembly (GAMA): stellar mass functions by Hubble type. , keywords =. doi:10.1093/mnras/stu1507 , archivePrefix =. 1407.7555 , primaryClass =

    doi arXiv

  115. [123]

    , keywords =

    The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS. , keywords =. doi:10.3847/1538-4357/aa65d0 , archivePrefix =. 1611.03084 , primaryClass =

    doi arXiv

  116. [124]

    , keywords =

    The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies. , keywords =. doi:10.1051/0004-6361/202451006 , archivePrefix =. 2406.03544 , primaryClass =

    doi

  117. [125]

    , keywords =

    The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z 3. , keywords =. doi:10.3847/1538-4357/ab7897 , archivePrefix =. 2002.08640 , primaryClass =

    2002 doi

  118. [126]

    The average far-infrared properties of Euclid-selected star-forming galaxies

    Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2511.02989 , archivePrefix =. 2511.02989 , primaryClass =

    doi arXiv

  119. [127]

    , keywords =

    Cosmological simulation with dust formation and destruction. , keywords =. doi:10.1093/mnras/sty1431 , archivePrefix =. 1802.04027 , primaryClass =

    doi arXiv

  120. [128]

    , keywords =

    JWST PRIMER: a deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS ─ dust-obscured star formation history back to z ≃ 7. , keywords =. doi:10.1093/mnras/staf1961 , archivePrefix =. 2503.07774 , primaryClass =

    doi

  121. [129]

    , keywords =

    Detailed dust modelling in the L-GALAXIES semi-analytic model of galaxy formation. , keywords =. doi:10.1093/mnras/stz1948 , archivePrefix =. 1904.02196 , primaryClass =

    1904 doi arXiv

  122. [130]

    , keywords =

    The dust-to-gas and dust-to-metal ratio in galaxies from z = 0 to 6. , keywords =. doi:10.1093/mnras/stz2684 , archivePrefix =. 1906.09277 , primaryClass =

    1906 doi

  123. [131]

    A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. II. Formation of Red Ellipticals. , keywords =. doi:10.1086/524363 , archivePrefix =. 0706.1246 , primaryClass =

    doi arXiv

  124. [132]

    , keywords =

    A Physical Model for the Coevolution of QSOs and Their Spheroidal Hosts. , keywords =. doi:10.1086/379875 , archivePrefix =. astro-ph/0307202 , primaryClass =

    doi arXiv

  125. [133]

    , keywords =

    Why stellar feedback promotes disc formation in simulated galaxies. , keywords =. doi:10.1093/mnras/stu1275 , archivePrefix =. 1403.6124 , primaryClass =

    doi arXiv

  126. [134]

    , keywords =

    The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. , keywords =. doi:10.1111/j.1365-2966.2005.09675.x , archivePrefix =. astro-ph/0508046 , primaryClass =

    2005 doi

  127. [135]

    , keywords =

    The HORIZON-AGN simulation: morphological diversity of galaxies promoted by AGN feedback. , keywords =. doi:10.1093/mnras/stw2265 , archivePrefix =. 1606.03086 , primaryClass =

    doi arXiv

  128. [136]

    , keywords =

    Strangulation as the primary mechanism for shutting down star formation in galaxies. , keywords =. doi:10.1038/nature14439 , archivePrefix =. 1505.03143 , primaryClass =

    doi arXiv

  129. [137]

    , keywords =

    The evolution of disk galaxies and the origin of S0 galaxies. , keywords =. doi:10.1086/157917 , adsurl =

    doi

  130. [138]

    , keywords =

    Quiescent Galaxies 1.5 Billion Years after the Big Bang and Their Progenitors. , keywords =. doi:10.3847/1538-4357/ab64dc , archivePrefix =. 1909.10540 , primaryClass =

    1909 doi

  131. [139]

    , keywords =

    Missing Giants: Predictions on Dust-obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time. , keywords =. doi:10.3847/1538-4357/acddde , archivePrefix =. 2211.02072 , primaryClass =

    doi

  132. [140]

    , keywords =

    A massive, quiescent galaxy at a redshift of 3.717. , keywords =. doi:10.1038/nature21680 , archivePrefix =. 1702.01751 , primaryClass =

    doi arXiv

  133. [141]

    , keywords =

    A massive quiescent galaxy at redshift 4.658. , keywords =. doi:10.1038/s41586-023-06158-6 , archivePrefix =. 2301.11413 , primaryClass =

    doi

  134. [142]

    , keywords =

    A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS. , keywords =. doi:10.1093/mnras/stad369 , archivePrefix =. 2208.00986 , primaryClass =

    doi

  135. [143]

    Scientific Reports , keywords =

    A population of faint, old, and massive quiescent galaxies at 3 <z <4 revealed by JWST NIRSpec Spectroscopy. Scientific Reports , keywords =. doi:10.1038/s41598-024-52585-4 , archivePrefix =. 2212.11638 , primaryClass =

    doi

  136. [144]

    , keywords =

    The Formation Histories of Massive and Quiescent Galaxies in the 3 < z < 4.5 Universe. , keywords =. doi:10.3847/1538-4357/ada6ac , archivePrefix =. 2410.02076 , primaryClass =

    doi

  137. [145]

    , keywords =

    The emergence of passive galaxies in the early Universe. , keywords =. doi:10.1051/0004-6361/202039738 , archivePrefix =. 2011.10584 , primaryClass =

    2011 doi

  138. [146]

    , keywords =

    Selecting a complete sample of blazars in sub-millimetre catalogues. , keywords =. doi:10.1093/mnras/stac1262 , archivePrefix =. 2205.07497 , primaryClass =

    doi

  139. [147]

    , keywords =

    Probing infrared eXcess to investigate early-Universe dust (PIXIEDust). , keywords =. doi:10.1093/mnras/staf2284 , archivePrefix =. 2512.07964 , primaryClass =

    doi

  140. [148]

    , keywords =

    The dust scaling relations of the Herschel Reference Survey. , keywords =. doi:10.1051/0004-6361/201118499 , archivePrefix =. 1201.2762 , primaryClass =

    doi arXiv

  141. [149]

    , keywords =

    An empirical determination of the dust mass absorption coefficient, _ d , using the Herschel Reference Survey. , keywords =. doi:10.1093/mnras/stw647 , archivePrefix =. 1603.04860 , primaryClass =

    doi arXiv

  142. [150]

    , keywords =

    Accurate dust temperature determination in a z = 7.13 galaxy. , keywords =. doi:10.1093/mnrasl/slab104 , archivePrefix =. 2108.13479 , primaryClass =

    doi

  143. [151]

    , keywords =

    The ALMA REBELS Survey: cosmic dust temperature evolution out to z 7. , keywords =. doi:10.1093/mnras/stac302 , archivePrefix =. 2202.01227 , primaryClass =

    doi

  144. [152]

    , keywords =

    A new look at the infrared properties of z 5 galaxies. , keywords =. doi:10.1093/mnras/stac2997 , archivePrefix =. 2210.09312 , primaryClass =

    doi

  145. [153]

    , keywords =

    Dual constraints with ALMA: new [O III] 88- m and dust-continuum observations reveal the ISM conditions of luminous LBGs at z 7. , keywords =. doi:10.1093/mnras/stac1905 , archivePrefix =. 2207.00022 , primaryClass =

    doi

  146. [154]

    , keywords =

    Red Spiral Galaxies at Cosmic Noon Unveiled in the First JWST Image. , keywords =. doi:10.3847/2041-8213/ac982b , archivePrefix =. 2208.00132 , primaryClass =

    doi

  147. [155]

    , keywords =

    The cold interstellar medium of a normal sub-L ^ galaxy at the end of reionization. , keywords =. doi:10.1051/0004-6361/202348128 , archivePrefix =. 2402.17845 , primaryClass =

    doi

  148. [156]

    , keywords =

    The main sequence of star-forming galaxies across cosmic times. , keywords =. doi:10.1093/mnras/stac3214 , archivePrefix =. 2203.10487 , primaryClass =

    doi

  149. [157]

    , keywords =

    Using dust, gas and stellar mass-selected samples to probe dust sources and sinks in low-metallicity galaxies. , keywords =. doi:10.1093/mnras/stx981 , archivePrefix =. 1705.02340 , primaryClass =

    doi arXiv

  150. [158]

    , keywords =

    Observational Evidence of Active Galactic Nuclei Feedback. , keywords =. doi:10.1146/annurev-astro-081811-125521 , archivePrefix =. 1204.4114 , primaryClass =

    doi arXiv

  151. [159]

    , keywords =

    Exploring the connection between AGN radiative feedback and massive black hole spin. , keywords =. doi:10.1051/0004-6361/202348538 , archivePrefix =. 2311.07576 , primaryClass =

    doi

  152. [160]

    , keywords =

    Morphological Quenching of Star Formation: Making Early-Type Galaxies Red. , keywords =. doi:10.1088/0004-637X/707/1/250 , archivePrefix =. 0905.4669 , primaryClass =

    doi arXiv

  153. [161]

    , keywords =

    Mass and Environment as Drivers of Galaxy Evolution in SDSS and zCOSMOS and the Origin of the Schechter Function. , keywords =. doi:10.1088/0004-637X/721/1/193 , archivePrefix =. 1003.4747 , primaryClass =

    doi arXiv

  154. [162]

    , keywords =

    The Galaxy End Sequence. , keywords =. doi:10.1093/mnras/stw2875 , archivePrefix =. 1611.00367 , primaryClass =

    doi arXiv

  155. [163]

    , keywords =

    The Herschel Reference Survey. , keywords =. doi:10.1086/651535 , archivePrefix =. 1001.5136 , primaryClass =

    doi arXiv

  156. [164]

    , keywords =

    Herschel-ATLAS: Evolution of the 250 m luminosity function out to z = 0.5. , keywords =. doi:10.1051/0004-6361/201014614 , archivePrefix =. 1005.2411 , primaryClass =

    doi arXiv

  157. [165]

    , keywords =

    The new galaxy evolution paradigm revealed by the Herschel surveys. , keywords =. doi:10.1093/mnras/stx2548 , archivePrefix =. 1710.01314 , primaryClass =

    doi arXiv

  158. [166]

    , keywords =

    Confirming the evolution of the dust mass function in galaxies over the past 5 billion years. , keywords =. doi:10.1093/mnras/stae2507 , archivePrefix =. 2411.04583 , primaryClass =

    doi

  159. [167]

    , keywords =

    The Cosmic Baryon and Metal Cycles. , keywords =. doi:10.1146/annurev-astro-021820-120014 , archivePrefix =. 2011.01935 , primaryClass =

    2011 doi

  160. [168]

    , keywords =

    REBELS-IFU: dust build-up in massive galaxies at redshift 7. , keywords =. doi:10.1093/mnras/staf1897 , archivePrefix =. 2501.10508 , primaryClass =

    doi

  161. [169]

    , keywords =

    Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe. , keywords =. doi:10.3847/1538-4357/ac5a4a , archivePrefix =. 2106.13719 , primaryClass =

    doi

  162. [170]

    Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6

    The ALPINE-ALMA [CII] survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6. , keywords =. doi:10.1051/0004-6361/201936965 , archivePrefix =. 1910.09517 , primaryClass =

    1910 doi

  163. [171]

    , keywords =

    The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties. , keywords =. doi:10.1051/0004-6361/202037649 , archivePrefix =. 2002.00962 , primaryClass =

    2002 doi

  164. [172]

    , keywords =

    The ALPINE-ALMA [C II] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements. , keywords =. doi:10.3847/1538-4365/ab7ccd , archivePrefix =. 1912.01621 , primaryClass =

    1912 doi

  165. [173]

    , keywords =

    A Controlled Study of Cold Dust Content in Galaxies from z = 0-2. , keywords =. doi:10.3847/1538-4357/aa76dc , archivePrefix =. 1705.10846 , primaryClass =

    doi arXiv

  166. [174]

    , keywords =

    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 =

    doi arXiv

  167. [175]

    , keywords =

    The dust-to-stellar mass ratio as a valuable tool to probe the evolution of local and distant star-forming galaxies. , keywords =. doi:10.1093/mnras/stw2749 , archivePrefix =. 1610.08979 , primaryClass =

    doi arXiv

Pith tools

Reviewed May 21, 2026 · model on record in the stance chip above.