{"total":13,"items":[{"citing_arxiv_id":"2607.05208","ref_index":13,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","primary_cat":"astro-ph.GA","submitted_at":"2026-07-06T15:26:08+00:00","verdict":"CONDITIONAL","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"FABLE simulation predictions for the nanohertz gravitational wave background are statistically consistent with NANOGrav 15-year data at 1–2.5σ tension, with physically motivated population modifications further improving agreement.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26445","ref_index":199,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T23:14:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New hydrodynamical simulations show that dwarf galaxy stellar mass-halo mass relations and star formation histories are more influenced by host halo concentration than by the 5 cMpc scale environment.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23798","ref_index":78,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating","primary_cat":"astro-ph.GA","submitted_at":"2026-06-22T18:00:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Presents 24 AREPO+IllustrisTNG zoom-in simulations of clusters above 10^15 solar masses showing converged magnetic fields with volume-averaged plasma beta approximately 100 inside R200 after z~1.2, declining Faraday rotation profiles, and intermittent Braginskii heating approaching cooling rates in ","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23651","ref_index":200,"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":"2605.11083","ref_index":79,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics","primary_cat":"astro-ph.CO","submitted_at":"2026-05-11T18:00:10+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"tSZ cross-correlations with large-scale structure tracers prefer low S8 and strong baryonic feedback, yielding S8 = 0.72 and low group baryon fraction in FLAMINGO simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06782","ref_index":101,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The galaxy ultraviolet luminosity function from $z=7$ to $15$ in the COLIBRE simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-05-07T18:00:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"COLIBRE simulations underpredict bright-end UV galaxy luminosities by 1 to 2.5 magnitudes at z=7-15 compared with observations, with the discrepancy persisting after dust attenuation and uncertainty accounting.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03154","ref_index":162,"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":38,"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":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.02022","ref_index":55,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-05-03T19:02:49+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"COLIBRE simulations with SKIRT post-processing match observed galaxy luminosity functions from FUV to submm at z=0, except underpredicting bright mid-IR galaxies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.06977","ref_index":39,"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":"2602.10192","ref_index":61,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-02-10T19:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The OBSIDIAN simulation with its three-regime AGN feedback best reproduces the observed stellar masses, star formation rates, and ages of brightest group galaxies, unlike the other simulations which show mismatches in quenching behavior.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.04067","ref_index":77,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase","primary_cat":"astro-ph.GA","submitted_at":"2025-09-04T09:58:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"COLIBRE calibrates supernova and AGN feedback parameters in multi-phase ISM cosmological simulations using emulator-based fitting to reproduce the z=0 galaxy stellar mass function and size-stellar mass relation at three resolutions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1902.05554","ref_index":234,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback","primary_cat":"astro-ph.GA","submitted_at":"2019-02-14T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"TNG50 shows galactic outflow mass loading is non-monotonic with stellar mass, rising rapidly above 10^10.5 Msun due to black hole feedback, and produces fast multi-phase outflows with emergent collimation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}