{"total":18,"items":[{"citing_arxiv_id":"2606.25856","ref_index":62,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JWST resolves jet-driven H2 and ionized outflows in radio galaxy 3C305","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T14:03:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"JWST data on 3C305 shows the compact radio jet efficiently drives kiloparsec-scale multiphase outflows via shocks, with high coupling to the observed gas kinetic power and radiative losses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25164","ref_index":240,"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":"2606.12851","ref_index":136,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Supermassive Black Hole Assembly from Heavy Seeds with Dynamical Friction in the BRAHMA Simulations: Implications for JWST, LISA, and the Local Universe","primary_cat":"astro-ph.GA","submitted_at":"2026-06-11T03:32:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Lenient heavy-seed models in BRAHMA simulations produce black hole merger rates above 100 per year and near-unity occupation fractions down to low-mass galaxies, while strict models yield only about 1 merger per year and occupation fractions below 10 percent for galaxies under 10^8 solar masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16501","ref_index":124,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31","primary_cat":"astro-ph.GA","submitted_at":"2026-05-15T18:00:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"ARTEMIS and EAGLE simulations classify L* galaxies by central BH-to-stellar-mass ratio and trace how merger history drives divergence in BH growth, star formation, and morphology, offering an explanation for the observed scatter and for MW/M31 differences.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16192","ref_index":102,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Simulations of gas inflow in the Milky Way I. Stellar-Feedback-Regulated Transport from the Central Molecular Zone to the Circumnuclear disk","primary_cat":"astro-ph.GA","submitted_at":"2026-05-15T17:10:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Stellar feedback regulates radial gas inflow in the Milky Way center, yielding time-averaged rates that fall from 5e-3 to 1e-6 solar masses per year with both smooth secular and episodic components.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15893","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing the faint end of simulated galaxy counts at z>3","primary_cat":"astro-ph.CO","submitted_at":"2026-05-15T12:22:12+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"For FORECAST IUs, the stellar mass density of each re- alization was computed as the sum of the masses of the star particles belonging to all subhalos within the partition, divided by the comoving volume of the partition. For both simula- tion snapshot boxes, the stellar mass density was computed using the total stellar mass of all subhalos within the snap- shot (SubhaloMassType(4)for TNG100 (Nelson et al. 2019) andSubhalo.MassType_Starfor EAGLE (The EAGLE team 2017)), divided by their respective comoving volumes,V TNG = (110.7)3 cMpc3 andV EAGLE =(100) 3 cMpc3. In Figure A.1, we compare the stellar mass density of the full TNG100 snapshot (golden dots) and the EAGLE snapshot (green dots) with the average mass density of 200 realizations"},{"citing_arxiv_id":"2605.07684","ref_index":234,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The diverse morphologies and evolution of low-luminosity edge-brightened radio galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-05-08T12:54:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Low-luminosity FRII radio galaxies show higher core prevalence, comparable hotspots, and ~32% restarting/remnant behavior compared to bright FRIIs, revealing a highly diverse population where FRII dynamics occur at low powers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03154","ref_index":225,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-05-04T20:51:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"UNKNOWN","novelty_score":6.0,"formal_verification":"none","one_line_summary":"ArkenstoneBH is a new subgrid model for the hot phase of black hole feedback that, in isolated galaxy tests, suppresses star formation by counteracting gas inflows from the circumgalactic medium.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03008","ref_index":71,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-05-04T18:00:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Multiple galaxy formation simulations show that low-mass quenched galaxies at z>3 are predominantly environmentally quenched satellites, often only temporarily so, and match JWST observations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.02493","ref_index":103,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-05-04T11:43:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Massive quiescent galaxies at cosmic noon are compact and bulge-dominated with inside-out quenching, where inner regions formed stars ~0.5 Gyr earlier and quenched faster than outskirts.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.18808","ref_index":96,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Analysis of synthetic OVI absorption associated with galaxy groups in SIMBA and TNG50 simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-04-20T20:25:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Both SIMBA and TNG50 simulations underpredict OVI covering fractions around galaxy groups compared to observations, with most absorbers being gravitationally bound.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.16539","ref_index":59,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Classifying Supermassive Black Hole Growth Regimes to Observables Across Cosmological Simulations with Forecasts for LSST","primary_cat":"astro-ph.GA","submitted_at":"2026-04-16T23:53:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Machine learning on cosmological simulations achieves 91-94% accuracy classifying over-massive versus under-massive SMBH growth regimes from LSST photometry, with 83-89% cross-simulation transfer accuracy driven primarily by host galaxy colors.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.15182","ref_index":19,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Understanding the regulation of star formation within TNG100 galaxies on kpc-scales using machine learning I: Global versus local","primary_cat":"astro-ph.GA","submitted_at":"2026-04-16T16:10:55+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Machine-learning analysis of TNG100 galaxies finds global properties (black-hole mass, halo mass) control quenching while local stellar density controls ongoing star formation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.06977","ref_index":87,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Galaxy discs regulate the growth of supermassive black holes","primary_cat":"astro-ph.GA","submitted_at":"2026-04-08T11:53:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Disc galaxies inhibit supermassive black hole growth by preserving rotational support in central gas, while mergers in ellipticals disrupt this support and enable rapid accretion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.11062","ref_index":56,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties","primary_cat":"astro-ph.GA","submitted_at":"2025-12-11T19:23:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Varied cosmic ray feedback models from AGN in FIRE-3 simulations all quench massive galaxies consistently with observations but produce vastly different circumgalactic medium properties.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.03132","ref_index":99,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles","primary_cat":"astro-ph.GA","submitted_at":"2025-12-02T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Milky Way-mass dark matter density profiles in IllustrisTNG are largely insensitive to astrophysics and cosmology variations, dominated by halo-to-halo variance instead.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.26877","ref_index":160,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift","primary_cat":"astro-ph.GA","submitted_at":"2025-10-30T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Bursty stellar feedback produces systematically flatter metallicity gradients than smooth feedback in high-redshift galaxies across multiple simulation suites.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.20430","ref_index":256,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue","primary_cat":"astro-ph.GA","submitted_at":"2025-09-24T18:00:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A score-based diffusion generative model on deep infrared galaxy photometry yields a star formation rate density peaking at z=1.3 and shows distinct non-parametric star formation histories plus AGN activity peaking during the quenching transition of massive galaxies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}