{"total":19,"items":[{"citing_arxiv_id":"2605.23554","ref_index":188,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope","primary_cat":"astro-ph.HE","submitted_at":"2026-05-22T12:19:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A new redshift-correlation technique with third-generation GW detectors can constrain the BNS contribution to cosmic r-process nucleosynthesis to 5-6% precision via Fisher forecasts on mock bright- and dark-siren data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18975","ref_index":15,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues","primary_cat":"astro-ph.GA","submitted_at":"2026-05-18T18:01:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulation comparison finds bulgeless galaxies host more centrally concentrated, disc-aligned satellites with steeper faint-end luminosity functions than bulge-dominated controls, reflecting co-evolution and quieter merger histories.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06769","ref_index":238,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model","primary_cat":"astro-ph.GA","submitted_at":"2026-05-07T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Lumen modeling of IllustrisTNG50 shows that high ionization parameters from massive star clusters plus enhanced nitrogen abundances are needed to reproduce the extreme [OIII]/Hβ, [OIII]/[OII], and [NII]/Hα ratios seen in z>3 galaxies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.04144","ref_index":116,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The galaxy-halo connection and the dynamical evolution of a giant disc in a massive node of the Cosmic Web at z~3","primary_cat":"astro-ph.GA","submitted_at":"2026-05-05T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The Big Wheel at z~3 has a stellar-to-halo mass ratio of 0.06, higher than expected, implying efficient stellar assembly without major mergers or instabilities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.00988","ref_index":213,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. 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III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-04-20T08:45:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"New JWST pure-parallel imaging over 400 arcmin² yields UV luminosity functions at z~7.5-10 consistent with pre-JWST models and significant clustering of bright galaxies implying they occupy more massive halos than previously modeled.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.17660","ref_index":20,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History","primary_cat":"astro-ph.CO","submitted_at":"2026-04-19T23:20:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Cosmic star formation history provides complementary constraints on cosmological parameters, breaking degeneracies when combined with standard probes and yielding H0 = 68.28 ± 0.18 km s^{-1} Mpc^{-1} with DESI data.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Mobasher, A. L. Coil, M. Kriek, and B. Siana, Monthly Notices of the Royal Astronomical Society498, 3648 (2020). [18] S. Mordini, L. Spinoglio, and J. A. Fern' andez-Ontiveros, Astron. Astrophys.653, A36 (2021), arXiv:2105.04584 [astro-ph.GA]. [19] P. Madau and M. Dickinson, Ann. Rev. Astron. Astro- phys.52, 415 (2014), arXiv:1403.0007 [astro-ph.CO]. [20] B. P. Moster, T. Naab, and S. D. M. White,428, 3121 (2013), arXiv:1205.5807 [astro-ph.CO]. [21] P. G. P' erez-Gonz' alezet al., Astrophys. J.991, 179 (2025), arXiv:2503.15594 [astro-ph.GA]. [22] M. T. Botticella, S. J. Smartt, R. C. Kennicutt, E. Cap- pellaro, M. Sereno, and J. C. Lee, Astronomy & amp; Astrophysics537, A132 (2012). [23] S. Jiao, J."},{"citing_arxiv_id":"2604.17162","ref_index":95,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts","primary_cat":"astro-ph.CO","submitted_at":"2026-04-18T22:37:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"FRB dispersion measures directly constrain suppression of the matter power spectrum due to feedback at k ~ 0.1-3 h/Mpc, reduce posterior variance by a factor of ~8 at k~1 h/Mpc, and exclude extreme large-scale feedback scenarios at ~2 sigma.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Monthly Notices of the Royal Astronomical Society488, 3143-3194, DOI: https://dx.doi.org/10. 1093/mnras/stz1182 (2019). 1806.07893. [94] Moster, B. P., Naab, T. & White, S. D. M. Galactic star formation and accretion histories from matching galaxies to dark matter haloes. Monthly Notices of the Royal Astronomical Society428, 3121-3138, DOI: https://dx.doi.org/10.1093/mnras/sts261 (2013). 1205.5807. [95] Pranjal R., S., Pandey, S., Anbajagane, D., Krause, E. & Dolag, K. Testing halo models for con- straining astrophysical feedback with multi-probe modeling: I. 3D Power spectra and mass frac- tions. arXiv e-printsarXiv:2507.13317, DOI: https://dx.doi.org/10.48550/arXiv.2507.13317 (2025). 2507.13317. [96] Aricò, G. et al. The BACCO simulation project: a baryonification emulator with neural net-"},{"citing_arxiv_id":"2604.13866","ref_index":110,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies","primary_cat":"astro-ph.CO","submitted_at":"2026-04-15T13:29:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Bayesian joint constraints show that elevated star formation efficiency accounts for JWST high-z galaxy excess in flat Lambda CDM, without requiring deviations in dark energy equation of state or curvature.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.08682","ref_index":75,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Hubble sequence in JWST CEERS from unbiased galaxy morphologies","primary_cat":"astro-ph.GA","submitted_at":"2026-04-09T18:13:54+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A Hubble-like sequence of galaxy morphologies exists by redshift 4, with low-mass galaxies as persistent star-forming disks and massive galaxies following either stable disk or rapid compaction-quenching paths.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.03389","ref_index":64,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Role of Baryonic and Dark Matter in Bar Kinematics","primary_cat":"astro-ph.GA","submitted_at":"2026-04-03T18:48:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Bar pattern speeds anti-correlate with stellar and total dynamical mass in 30 galaxies, placing the slowest bars in the most massive systems and supporting angular momentum transfer to dark matter.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.05584","ref_index":7,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Stellar feedback drives the baryon deficiency in low-mass galaxies","primary_cat":"astro-ph.GA","submitted_at":"2025-12-05T10:10:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Stacking DESI spectra reveals star-formation-driven Mg II outflows from low-mass galaxies that escape dark matter halos, providing indirect evidence that stellar feedback causes baryon deficiency.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.00975","ref_index":99,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Atacama Cosmology Telescope: stellar mass growth in massive galaxy clusters from DR5 over the past 7 billion years","primary_cat":"astro-ph.GA","submitted_at":"2025-11-02T15:37:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Composite cluster stellar mass functions show marginal M* evolution at high z and a factor of 2.5 growth in stellar mass fraction from z=0.8 to 0.2 after accounting for halo mass growth.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.09576","ref_index":97,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way","primary_cat":"astro-ph.GA","submitted_at":"2025-09-11T16:11:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations show that observed rotation in 13.5-Gyr-old alpha-rich stars constrains the Gaia-Sausage-Enceladus merger to mass ratios below 1:4, with interaction and starburst times both near 11 Gyr.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.07097","ref_index":60,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger","primary_cat":"astro-ph.GA","submitted_at":"2025-09-08T18:00:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"FRB dispersion measures from CHIME/FRB Outrigger constrain gas mass fractions in galaxy groups and clusters, consistent with eROSITA at R500 but with mild tension at R200.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}