{"total":137,"items":[{"citing_arxiv_id":"2606.27853","ref_index":36,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec","primary_cat":"astro-ph.GA","submitted_at":"2026-06-26T08:52:55+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New JWST data on 23 galaxies at 0.5<z<1.7 show median dark matter fraction of 0.63 at effective radius with 0.2 dex scatter, and a mix of rising, flat, and falling rotation curves.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27714","ref_index":225,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Fast Radio Bursts as Cosmological Probes","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T04:44:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"FRBs serve as cosmological probes via dispersion measure, scattering, and Faraday rotation to constrain baryon distribution, expansion history, magnetic fields, and fundamental physics effects.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27423","ref_index":43,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Analytical and fitting formulae for solutions to Lyman-alpha radiative transfer equations: the effects of geometry, recoil, and velocity gradients","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Derives analytical solutions and fitting formulae for Lyα spectra under cylindrical geometry including recoil and velocity gradients, validated against Monte Carlo simulations.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"𝜕(H𝐽) 𝜕𝑦 =− 3H𝑗 𝜈 𝑛0𝜎0 ,(42) where𝑥 T ≡ (𝑘 B𝑇)/(ℎΔ𝜈 D)(Zheng & Miralda-Escudé 2002)5. The recoileffectisdescribedbythetermcontaining𝑥 T.Wefirstseparate variables following𝐽(𝑦, 𝜏)= Í∞ 𝑛=0 𝐸𝑛 (𝜏)𝑓 𝑛 (𝑦). The recoil term doesnotaffecttheprocedureforobtaining𝐸 𝑛 (𝜏),whiletheequation for𝑓 𝑛 (𝑦)becomes d2 𝑓𝑛 d𝑦2 + √ 6 2𝑥T d(H𝑓 𝑛) d𝑦 −𝜆 2 𝑛 𝑓𝑛 =− 3H𝑄 𝑛 𝑛0𝜎0 .(43) Torevealthehiddenstructureinequation(43),weadoptthefollowing trial solution𝑓 𝑛 (𝑦)=ℎ 𝑛 (𝑦)E (𝑦), where we requireℎ𝑛 (𝑦)to be the recoil-freesolutionandsatisfyequation(23).Withthistrialfunction, equation (43) becomes E d2ℎ𝑛 d𝑦2 + 2 dE d𝑦 + √ 6 2𝑥T H E ! dℎ𝑛 d𝑦 + \" d2E d𝑦2 + √ 6 2𝑥T d(H E) d𝑦 −𝜆 2 𝑛E # ℎ𝑛 =− 3H𝑄 𝑛 𝑛0𝜎0 . (44) Withoutexplicitlysolvingequation(44),wederiveanapproximate"},{"citing_arxiv_id":"2606.26576","ref_index":107,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor","primary_cat":"astro-ph.IM","submitted_at":"2026-06-25T03:52:30+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"A new 296-detector 90 GHz TES bolometer array for CLASS achieves uniform properties, 16 μK√s NET, 0.37 optical efficiency, and a 41% mapping speed boost after addressing blue-leak radiation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26355","ref_index":35,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing the Nature of Lyman Continuum Emitting and Low-metallicity Galaxies Using the SKA","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T20:09:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"SKA-Mid is predicted to yield samples of 10-100 low-metallicity Lyman continuum emitting galaxies per square degree, enabling multi-wavelength studies of feedback processes linked to ionizing photon escape.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26218","ref_index":52,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dark Matter in Draco and Bo\\\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"GraphNPE recovers a significantly lower central density for Boötes I consistent with a core while Draco remains marginally cuspy, and demonstrates that higher-order velocity moments reduce bias in dynamical modeling.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25583","ref_index":14,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Weak Lensing with SKAO: Cosmic Shear Cosmology","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T08:56:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Forecasts indicate SKAO cosmic shear can constrain S8 to 5% alone and 3% combined with LSST or Euclid, with added benefits from polarization and kinematics for separating lensing signals.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25517","ref_index":19,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Unveiling the nature of barium stars. I. Asteroseismic masses and the evolutionary link between Ba dwarfs and giants","primary_cat":"astro-ph.SR","submitted_at":"2026-06-24T07:50:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Asteroseismic masses average 1.29 Msun for Ba dwarfs versus 1.96 Msun for Ba giants, supporting main-sequence accretion evolution from dwarfs to giants, though models fail to match the observed [hs/ls] ratio.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"2016, (5) Komiya et al. 2007, (6) Barbuy et al. 1992, (7) Tomkin & Lambert 1979, (8) Sneden et al. 1981, (9) Smiljanic et al. 2007, (10) Masseron et al. 2010, (11) Andrievsky et al. 2002, (12) Zacs 1994, (13) Katime Santrich et al. 2013, (14) Yang et al. 2024, (15) Karinkuzhi et al. 2018, (16) Smith 1984, (17) Jorissen 1988, (18) Karinkuzhi & Goswami 2014, (19) Karinkuzhi & Goswami 2015, (20) Dimoffet al. 2024, (21) Tomkin et al. 1976, (22) Deming 1978, (23) Kong et al. 2018b, (24) Merle et al. 2016, (25) Liang et al. 2003, (26) Luck 2017, (27) Soubiran & Girard 2005, (28) Gustafsson et al. 1999, (29) Shi et al. 2004, (30) Edvardsson et al. 1993, (31) Luck & Heiter 2006, (32) Boesgaard et al. 1999, (33) Ramírez et al."},{"citing_arxiv_id":"2606.25164","ref_index":216,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T20:53:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Line ratio diagnostics in NGC 1068 indicate AGN outflows are shock-accelerated, with outflowing gas dust-free and 19-110 times denser than disk gas.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23651","ref_index":12,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Revisiting the 'Lensing is Low' Problem with UNIONS","primary_cat":"astro-ph.CO","submitted_at":"2026-06-22T17:36:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New UNIONS galaxy-galaxy lensing data around CMASS galaxies indicates no significant lensing is low problem, with joint HOD fits to GGL and GC favoring a slightly lower matter power spectrum amplitude than Planck.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23551","ref_index":122,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system","primary_cat":"astro-ph.EP","submitted_at":"2026-06-22T16:25:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New 2025 transit timing of HIP 41378 f shows a 7-hour early arrival consistent with TTVs; N-body modeling with TRADES refines ephemerides for planets d, e, and f.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22619","ref_index":50,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation","primary_cat":"astro-ph.SR","submitted_at":"2026-06-21T18:01:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Binary evolution modeling constrains donor masses of 14-23 solar masses for two luminous red novae and shows dust masses are 1-5 orders of magnitude below total ejected envelope masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22302","ref_index":50,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Revisiting cosmic anisotropy with the Pantheon+ compilation","primary_cat":"astro-ph.CO","submitted_at":"2026-06-21T02:05:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Re-analysis of Pantheon+ supernovae finds no statistically compelling evidence for intrinsic cosmic anisotropy; reported signals are subsample-dependent and attributed to data distribution artifacts.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21855","ref_index":154,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The panchromatic JWST dayside spectrum of WASP-121 b reveals a refractory-rich formation","primary_cat":"astro-ph.EP","submitted_at":"2026-06-20T03:23:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Panchromatic JWST spectrum of WASP-121 b detects SiO and measures refractory-to-volatile ratios 3x stellar, consistent with mixed solid-gas accretion or migration with continued solid accretion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20953","ref_index":87,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Variables in S-PLUS: I. Multiband period-luminosity relations and reddening maps of the Magellanic Clouds using classical Cepheids","primary_cat":"astro-ph.GA","submitted_at":"2026-06-18T21:34:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"First multiband P-L relations for Cepheids in S-PLUS system with reddening maps of the Magellanic Clouds from single-epoch photometry.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20845","ref_index":208,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon","primary_cat":"astro-ph.GA","submitted_at":"2026-06-18T18:27:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"LEGGOS presents a uniform framework that jointly models lensing, photometry, and integral-field spectroscopy to disentangle stellar populations in clumps of high-redshift lensed galaxies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20836","ref_index":148,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Old and Bright: The Remarkable Radio Brightening of the Engine-driven SN 2012au Several Years After Explosion Signals the Birth of a PWN","primary_cat":"astro-ph.HE","submitted_at":"2026-06-18T18:21:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Late-time radio observations of SN 2012au show re-brightening best explained by emission from a newborn pulsar wind nebula rather than continued shock interaction with circumstellar material.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20794","ref_index":18,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Constraints on Horndeski Gravity with Phantom Crossing","primary_cat":"astro-ph.CO","submitted_at":"2026-06-18T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"ACG models embed the observationally preferred phantom-crossing dark energy behavior inside a consistent Horndeski Lagrangian and achieve data fits of similar quality to w0waCDM while being narrowed by perturbative probes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.18355","ref_index":35,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-Consistent Tidal Distortion Model","primary_cat":"astro-ph.EP","submitted_at":"2026-06-16T18:03:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Revised mass of 0.503 M_Earth and radius of 0.736 R_Earth for GJ 367 b give a density of 6.9 g cm^{-3} and an iron fraction of 50-70% via new tidal and composition modeling.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.18334","ref_index":105,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-16T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"76 N/O-enhanced galaxies at 4<z<8.5 are observed shortly after starbursts, either in the WR enrichment phase within 10 Myr or the AGB phase after 30-40 Myr following outflows.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17896","ref_index":20,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Detectability of deuterium in spectra of early-type stars","primary_cat":"astro-ph.SR","submitted_at":"2026-06-16T13:16:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Synthetic spectra and MCMC analysis establish deuterium detection limits in early-type stars as a function of SNR, Teff, and v sin i, with upper limits D/H < -5.5 dex for HD 32115 and < -4.9 dex for 21 Peg.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17230","ref_index":15,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The properties of tidal disruption event infrared counterparts produced by dust rings and inference of the observing angle","primary_cat":"astro-ph.HE","submitted_at":"2026-06-15T19:22:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A toy model of dust rings in TDEs predicts brighter IR emission on-axis, explaining X-ray/IR correlations and enabling viewing-angle constraints from observed light curves.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17146","ref_index":125,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon","primary_cat":"astro-ph.GA","submitted_at":"2026-06-15T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"JWST MIRI observations of 634 galaxies at 0.2<z<2 yield IR luminosity functions with faint-end slope α≈0.147, implying lower dust-obscured SFRD than previous ALMA/Herschel/Spitzer studies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.16796","ref_index":171,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity","primary_cat":"astro-ph.GA","submitted_at":"2026-06-15T14:38:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"HINSA observations show CRIR decreasing with H2 column density in both clouds, with IC 348 values an order of magnitude above NGC 1333, modeled as an order-of-magnitude difference in low-energy CR populations from local acceleration sources.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13393","ref_index":147,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$","primary_cat":"astro-ph.GA","submitted_at":"2026-06-11T14:24:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Direct detection of CO(3-2) at z=7.31 in REBELS-25 gives M_mol ~ 10^11 M_sun with f_gas ~0.95, confirming a massive molecular reservoir and showing low-J CO remains detectable in the Epoch of Reionization.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12517","ref_index":49,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Hubble Missing Globular Clusters Survey IV. Ultra-faint compact satellites of the Milky Way. The case of Koposov 2","primary_cat":"astro-ph.GA","submitted_at":"2026-06-10T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Koposov 2 is shown to be an old (13.7 Gyr) star cluster with half-light radius 2.7 pc, absolute magnitude -0.95, and stellar mass 372 solar masses, supporting a star cluster classification over a dwarf galaxy.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12010","ref_index":64,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The 35-Myr old infant planet TOI-837 b has a mildly misaligned orbit","primary_cat":"astro-ph.EP","submitted_at":"2026-06-10T12:33:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"TOI-837 b has a true obliquity of 25.9+7.5-6.3 deg, the first planet younger than 100 Myr with accessible ψ incompatible with an aligned orbit, favoring primordial disc torque followed by disc-driven migration.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11939","ref_index":66,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Detection of a parsec-scale, compact, and fading ejecta from an accreting massive black hole","primary_cat":"astro-ph.HE","submitted_at":"2026-06-10T11:11:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"VLBI at 4.9 GHz plus multi-epoch survey data reveal a fading parsec-scale radio component near the optical center of a dwarf galaxy, interpreted as transient ejecta from IMBH accretion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11345","ref_index":260,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity","primary_cat":"astro-ph.GA","submitted_at":"2026-06-09T18:23:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"New stack-based strong-line calibrations from ~1500 spectra yield mass-metallicity relations at z=1-10 with decreasing metallicity toward higher redshift and no slope change, plus 50 EMPG candidates at 1-4% solar metallicity showing large scatter and opposite sSFR trends.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11328","ref_index":70,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Morphology, sizes, and scatter in a large sample of distant quiescent galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-09T18:09:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New high-redshift quiescent galaxy sample shows size decreasing with redshift and wavelength, with stellar mass plus redshift sufficient to predict size but large residual scatter.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11026","ref_index":257,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"MINDS survey of silicates in T Tauri disks: Correlation between dust and gas","primary_cat":"astro-ph.SR","submitted_at":"2026-06-09T15:59:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Spectral decomposition of 26 T Tauri disks finds Mg-rich silicate dust with 5-24% crystallinity and correlations linking annealed silica to stronger CO2 emission and forsterite to stronger H2O emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10712","ref_index":76,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"DIffuse X-ray Explorer (DIXE): Sky Survey Strategy and Collimator Response Demodulation","primary_cat":"astro-ph.IM","submitted_at":"2026-06-09T11:16:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"DIXE proposes CSS-based survey strategies covering 72.5% of the sky with 26-68 ks exposures and shows via simulation that MCMC collimator demodulation yields 1° point-source localization and 3° extended-source resolution.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10623","ref_index":86,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-09T09:22:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A 6D kinematic census identifies 18 anomalous Cepheids with extreme orbits, including one possibly scattered by globular cluster E3, and finds consistency between dynamical and stellar ages.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10558","ref_index":50,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Hector Galaxy Survey: Linking the low- and high-mass ends of the initial mass function in star-forming galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-09T08:25:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Simultaneous measurement of low- and high-mass IMF slopes in 214 star-forming galaxies reveals diversity, weak correlation between ends, and links to stellar mass, star formation rate, and metallicity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10538","ref_index":16,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Updating the PATH framework with FRB host galaxy models","primary_cat":"astro-ph.HE","submitted_at":"2026-06-09T08:07:25+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"PATH is extended with three fitted P(m_r|z) prior models combined with P(z|DM), raising host-association confidence for ASKAP FRBs while showing fainter-than-expected host magnitude distribution.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"We also construct a functionP(O|m) in § 4.1, such that P(O) = Z P(O|m)P(m)dm(14) P(U) = Z (1−P(O|m))P(m)dm, (15) which ensures correct normalisations on the priors that the true host is or is not seen in an image. The priorP(O i) that a particular galaxy of magnitudem i is the host is therefore the integrand of Equation 14, i.e. P(Oi) =P(O|m i)P(mi). (16) This effect must also be accounted-for in the galaxy density function,ρ(m i). Thus we use ρ(mi) =P(O|m i)ρD16(mi) (17) where ρD16(mi) is the galaxy density function from Driver et al. (2016). In effect, this means that factorsP(O|m i) in both the numerator and denominator of Equation 10 cancel, and this term affects the likelihood only throughP(U)-which"},{"citing_arxiv_id":"2606.08782","ref_index":7,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe","primary_cat":"astro-ph.GA","submitted_at":"2026-06-07T18:58:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"JWST spectra reveal that two z~7 galaxies already show near-solar iron-to-silicon ratios with no strong odd-even effect, favoring early Type Ia supernovae over pair-instability supernovae as the source of iron enrichment.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"1210, 1264, 1286, 1287, 4540; GO-1895, PI: P. Oesch Oesch et al. 2023 2514, PI: C. Williams, Williams et al. 2025 2674, PI: P. Arrabal Haro, 3577, PI: E. Egami, 4762, PI: S. Fujimoto, 5398, PI: J. Kartaltepe, and 6434, PI: E. Egami, Sun et al. 2025). 4Nakane et al. T able 1.Sample in This Study. Name R.A. Decl.z sys MUV re µReference [mag] [pc] (1) (2) (3) (4) (5) (6) (7) (8) GN-11 189.106030 62.242046 10.6034−21.71 +0.02 −0.04 67.7+2.9 −5.8 - Bu23, This work Gz9p3† 3.617169 -30.425549 9.3111−21.24 +0.06 −0.09 409.2+31.7 −31.6 1.62 Ch26, This work CEERS-1025 214.967547 52.932953 8.7163−20.96 +0.02 −0.02 53.4+7.3 −4.6 - This work CEERS-1019† 215.035391 52.890662 8.6778−21.87 +0.08 −0.13 102.6+5.9a −8.9 - This work GLASS-100003† 3."},{"citing_arxiv_id":"2606.07087","ref_index":84,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst","primary_cat":"astro-ph.HE","submitted_at":"2026-06-05T09:34:11+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A reported periodic fast radio burst is reclassified as Galactic pulsar emission due to CHIME calibration and beam-pointing error.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06868","ref_index":42,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The mass of TOI-1883 b: A low density super-Neptune in the ridge regime transiting an early-M dwarf","primary_cat":"astro-ph.EP","submitted_at":"2026-06-05T03:35:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Mass of 13.7 Earth masses and density 0.4 g cm^{-3} measured for TOI-1883 b, a super-Neptune in the ridge regime around an early-M dwarf, with implications for disk migration and photoevaporation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06731","ref_index":87,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Direct simulations of very high energy cosmic ray acceleration in 3D MHD model of a compact star cluster","primary_cat":"astro-ph.HE","submitted_at":"2026-06-04T21:35:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"3D MHD simulations of young massive star clusters find proton acceleration to hundreds of TeV near O-star termination shocks, with even faster acceleration to over 100 TeV in under 100 years when a supernova remnant expands inside the core.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06578","ref_index":60,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A Disappearing Act: Constraints From \"Missing\" Flares of Repeating Partial TDE Candidates","primary_cat":"astro-ph.HE","submitted_at":"2026-06-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Non-detections of expected third flares in TDE 2022dbl and TDE 2020vdq support rpTDE interpretation over independent events, with modeling favoring bound main-sequence star orbits and deep initial encounters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06213","ref_index":130,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing a new subclass of llGRB-SN transients: Insights from EP250304a and its associated supernova","primary_cat":"astro-ph.HE","submitted_at":"2026-06-04T14:23:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"EP250304a/SN 2025fhm is presented as a member of an emerging subclass of shocked cocoon-dominated low-luminosity GRB-SNe based on spectral, photometric, and light-curve modeling comparisons to prior events.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05343","ref_index":205,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211","primary_cat":"astro-ph.HE","submitted_at":"2026-06-03T18:35:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Bayesian fitting of an eccentric Keplerian orbit to the radio light curve of PKS 2131-021 gives e = 0.053 ± 0.015 without red noise but favors a circular orbit plus DRW noise with e < 0.15.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05146","ref_index":282,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Early Multiwavelength Observations of AT 2026fgk: The Luminous Afterglow to Sub-luminous GRB 260310A, Identified Independently of a Gamma-ray Trigger","primary_cat":"astro-ph.HE","submitted_at":"2026-06-03T17:51:05+00:00","verdict":"ACCEPT","verdict_confidence":"HIGH","novelty_score":5.0,"formal_verification":"none","one_line_summary":"First blind optical identification of a z=0.153 sub-luminous GRB afterglow with Ic-BL SN, yielding a volumetric rate consistent with on-axis high-luminosity long GRBs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04875","ref_index":97,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A Model Selection Criterion for Multidimensional Gaussian Processes: Application to Radial Velocities","primary_cat":"astro-ph.IM","submitted_at":"2026-06-03T13:38:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Introduces MGIC_rv, an information criterion that combines conditional RV likelihood with an effective parameter count for selecting multi-GP models focused on radial velocities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04827","ref_index":160,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Steep Redshift Evolution of the Ionizing Escape Fraction at $z = 5$--$12$: Empirical Constraints and Comparison with Simulations","primary_cat":"astro-ph.CO","submitted_at":"2026-06-03T12:50:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Empirical three-parameter fit to f_esc(M_h,z) yields steep redshift evolution with population-averaged escape fraction rising from ~2% at z=5 to ~9% at z=12.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04585","ref_index":191,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Earliest simultaneous multi-color optical observations of GRB 230328B: from 41 seconds to the host-galaxy identification","primary_cat":"astro-ph.HE","submitted_at":"2026-06-03T08:24:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New early multi-wavelength data on GRB 230328B shows afterglow with early bump and late achromatic rebrightening at ~4000 s, modeled via MCMC as forward shock plus late energy injection in a dusty S0 host with AV~0.8 and no supernova signature.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03901","ref_index":61,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The VMC survey -- LV. The coherent expansion of the SMC","primary_cat":"astro-ph.GA","submitted_at":"2026-06-02T16:56:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Improved VMC proper motions show SMC expansion along SE-NW axes consistent with LMC tides, radial inward motions with no rotation, and northward motion in older RGB stars from a prior interaction.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03824","ref_index":238,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The CRIMSON survey I: super-stellar SiO in the directly imaged companion TWA 5 B from high-resolution M-band spectroscopy","primary_cat":"astro-ph.EP","submitted_at":"2026-06-02T16:07:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"High-resolution M-band spectroscopy detects super-stellar SiO in TWA 5 B, implying no significant magnesium-silicate clouds and formation consistent with core accretion beyond the CO snowline or gravitational instability with solid enrichment.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03737","ref_index":37,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"J0404+1112: A 3-Hour Eclipsing White Dwarf-Brown Dwarf Probing Multiple Atmospheric Regimes","primary_cat":"astro-ph.SR","submitted_at":"2026-06-02T14:53:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"J0404+1112 is a 2.93 hr period totally eclipsing WD+BD system with a hot DA white dwarf (T_eff ~28,000 K) and ~40 M_Jup brown dwarf, enabling isolation of nightside emission and serving as a JWST atmospheric benchmark.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02688","ref_index":248,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"NOEMA$^\\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\\sim1$","primary_cat":"astro-ph.GA","submitted_at":"2026-06-01T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Deep interferometric observations of a z≈1.12 barred spiral reveal bar-driven molecular inflows at a rate matching the galaxy's star formation rate of ~36 M⊙/yr.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}