{"total":19,"items":[{"citing_arxiv_id":"2606.30787","ref_index":125,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JWST spectroscopy of galaxies at $z>10$: Damped Ly$\\alpha$ absorbers reveal efficient star formation and hidden redshift biases","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:16:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Analysis of JWST/NIRSpec Prism spectra for 25 z>=10 galaxies finds burstiness correlates with strong UV lines, short depletion times, and DLA-induced redshift biases of 0.39 and 0.14 with marginal impact on UV luminosity density.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30722","ref_index":35,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South","primary_cat":"astro-ph.EP","submitted_at":"2026-06-29T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Observational study of 290 exoplanet-host stars finds higher C, O, S, Fe, Ni abundances in giant-planet hosts than small-planet hosts, with C/O ratios, hot/warm differences, and mass correlations that vary by subpopulation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27426","ref_index":57,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Too shy to spin? Cosmic wallflowers as proto-globular clusters","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Simulation study proposes that weakly rotating, gas-rich cosmic wallflowers at high redshift are natural proto-globular cluster candidates based on kinematics and densities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25205","ref_index":98,"ref_count":3,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A new $H_0$ measurement with SNe Requiem and Encore using $\\texttt{Gravity.jl}$","primary_cat":"astro-ph.CO","submitted_at":"2026-06-23T21:54:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New H0 = 67.0 +9.3/-7.8 km/s/Mpc from joint lens-model fit to time delays of SN Requiem and SN Encore in MACS J0138.0-2155.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24114","ref_index":57,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Kepler Image-Subtracted Light Curves and Variable Star Catalog of NGC 6819","primary_cat":"astro-ph.SR","submitted_at":"2026-06-23T04:01:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Generates and publicly releases 81,498 detrended Kepler light curves plus a catalog of 87 periodic variables (26 new) in the 2.5 Gyr cluster NGC 6819 using Gaia DR3 for membership.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21855","ref_index":171,"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":"2606.10538","ref_index":178,"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":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10027","ref_index":170,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-06-08T18:08:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Four parameters suffice to describe dust attenuation curve diversity in TNG simulations, yielding a new symbolic-regression model that recovers curves and fluxes better than existing parameterizations while linking parameters to SFR surface density, metallicity, and geometry.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06868","ref_index":113,"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":"2606.04740","ref_index":74,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates","primary_cat":"astro-ph.HE","submitted_at":"2026-06-03T11:22:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"FIRE-2 simulations show per-galaxy tidal disruption rates peak near z=2.5 at 4e-4 per year, correlate with SFR and central density, and remain high in satellite galaxies at early times.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23554","ref_index":266,"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":"2605.22245","ref_index":45,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing freeze-in dark matter using Bose-Einstein condensate in neutron star","primary_cat":"hep-ph","submitted_at":"2026-05-21T09:51:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Bose-Einstein condensate formation in neutron stars enhances dark matter annihilation by 10^15-10^20, allowing freeze-in models to produce observable heating and probe neutrino-fog scattering cross-sections.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13966","ref_index":72,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Massive Galaxies Form Early and Gray: Stellar Assembly and Dust Attenuation at $\\mathbf{z>3.5}$ from CAPERS","primary_cat":"astro-ph.GA","submitted_at":"2026-05-13T18:00:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Massive galaxies at z>3.5 assembled stars earlier than theoretical models predict and exhibit gray dust attenuation, especially at the highest masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.10102","ref_index":8,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"From Large Telescopes to the MUltiplexed Survey Telescope (MUST)","primary_cat":"astro-ph.IM","submitted_at":"2026-05-11T07:18:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"MUST is a new 6.5 m telescope designed to deliver simultaneous optical spectra for over 20,000 targets across a 5 deg² field, enabling the largest 3D spectroscopic map of the Universe with redshifts for more than 100 million objects over an 8-year survey.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"In this exciting new era, optical and near-infrared observa- tions of the universe continue to be the cornerstone of astro- physics and cosmology. Over the past few decades, the astro- nomical community has pushed the design and development of large observing facilities to increasingly challenging lim- its on the ground or in space [e.g., James Webb Space Tele- scope (JWST) [8], Hubble Space Telescope (HST) 2), Very Large Telescope (VLT)3), Keck Observatory twin telescopes (Keck)4), etc.]. Right now, several 30-40 meter ground-based telescopes, such as the Extremely Large Telescope (ELT) [9], Thirty Meter Telescope (TMT) [10,11], Giant Magellan Tele- scope (GMT) [12], are either under construction or being planned. With the help of revolutionary active and adaptive"},{"citing_arxiv_id":"2604.21652","ref_index":114,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Constraining dark matter self-interaction from kinetic heating in neutron stars","primary_cat":"hep-ph","submitted_at":"2026-04-23T13:17:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Observation of neutron stars at 1000-1200 K could constrain asymmetric dark matter self-interaction cross-sections by two orders of magnitude beyond bullet cluster limits.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"However, infrared telescope like the James Webb Space Telescope (JWST) can potentially look into low heating signatures arising solely from DM scattering [91]. It was pointed out in [91] that old and isolated neutron stars ofO(1000) K are excellent targets for detecting DM heating signatures. Monte-Carlo orbital simulations of galactic neutron stars predict 1-2 (100-200) cold, old and isolated neutron stars within a distance of 10 (50) pc [114, 115]. However, it was recently shown in [116, 117] that there are no detectable neutron stars present within a distance of 10 pc from Earth and with tem- peratures of 2000 K.The currently operating JWST [118], along-with proposed European Extremely Large Telescope (ELT) [119] and Thirty Meter Telescope (TMT) [120] are capable of detecting BB temperatures of 1300-4300 K with their optical to near-infrared imaging instruments [121]."},{"citing_arxiv_id":"2604.13423","ref_index":90,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Into the Gompverse: A robust Gompertzian reionization model for CMB analyses","primary_cat":"astro-ph.CO","submitted_at":"2026-04-15T02:49:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A Gompertzian reionization model with three nuisance parameters demotes optical depth to a derived quantity, reducing its uncertainty by a factor of three and revealing potential neutrino mass tension in CMB analyses.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"We infer a larger value for the Hubble constant, very slightly more aligned with the SH0ES supernovae measurements calibrated using Cepheids (H 0 = 73.17±0.86 km s −1 Mpc−1 [88]). Likewise, our findings better align with the Chicago-Carnegie Hubble program using TRGB (Tip of the Red Giant Branch) stars for calibration [89]. In particular, their recent measurements using solely James Webb Space Telescope [90] data yieldH 0 = 68.81±2.22 [91] in good agreement with Eq. (5.1). The inclusion of BAO can also lead to smallerA s and largerτ reio. Ultimately, this is a consequence of the breaking of the Ω m −H 0 degeneracy. The BAO preference for smaller Ωm yields lower clustering, and hence lowerσ 8, while simultaneously decreasing thek eq, the scale of equality, and also delaying the equality (between matter and radiation)."},{"citing_arxiv_id":"2601.17117","ref_index":21,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass","primary_cat":"astro-ph.CO","submitted_at":"2026-01-23T19:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Non-equilibrium relativistic SIDM halo collapse produces seed black holes of mass ~3e-8 of the halo mass at apparent horizon formation.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[17] A. D. Gouldinget al., Astrophys. J. Lett.955, L24 (2023), arXiv:2308.02750 [astro-ph.GA]. [18] R. Maiolinoet al., Astron. Astrophys.691, A145 (2024), arXiv:2308.01230 [astro-ph.GA]. [19] C.-H. Chen, L. C. Ho, R. Li, and M.-Y . Zhuang, Astrophys. J. 983, 60 (2025). [20] A. Bogdanet al., Nature Astron.8, 126 (2024), arXiv:2305.15458 [astro-ph.GA]. [21] M. V olonteri, Astron. Astrophys. Rev.18, 279 (2010), arXiv:1003.4404 [astro-ph.CO]. [22] L. Baracket al., Class. Quant. Grav.36, 143001 (2019), arXiv:1806.05195 [gr-qc]. [23] T. Chantavat, S. Chongchitnan, and J. Silk, Mon. Not. Roy. Astron. Soc.522, 3256 (2023), arXiv:2302.09763 [astro- ph.SR]. [24] V . Bromm and A. Loeb, Astrophys. J.596, 34 (2003),"},{"citing_arxiv_id":"2303.15923","ref_index":59,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Science with the Einstein Telescope: a comparison of different designs","primary_cat":"gr-qc","submitted_at":"2023-03-28T12:29:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"The paper evaluates how triangular versus two-L-shaped geometries, arm lengths, and presence of low-frequency instruments affect the science reach of the Einstein Telescope for compact binaries, multi-messenger events, and stochastic backgrounds.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"4 Multi-messenger astrophysics In this section we study the impact of the different detector geometries and different ASDs on the multi-messenger capabilities of ET operating in synergy with electromagnetic (EM) observatories. ET will observe together with a new generation of innovative EM observatories, such as CTA [56], Athena [57], the Vera Rubin Observatory [58], JWST [59], ELT [60], SKA [61] and with the possible mission concepts UVEX [62], THESEUS [63], HERMES [64], GRINTA, ASTROGAM [65] and AMEGO [66]. These observatories will probe the formation, evolution, and physics of BNS systems in connection with kilonovae (KNe) and short gamma- ray bursts (GRBs) along the star formation and chemical evolution of the Universe."},{"citing_arxiv_id":"1912.02622","ref_index":89,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Science Case for the Einstein Telescope","primary_cat":"astro-ph.CO","submitted_at":"2019-12-05T14:57:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"The Einstein Telescope will enable gravitational-wave observations up to cosmological distances, opening avenues for discoveries in astrophysics, cosmology, and fundamental physics.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"Metzger, \"Collapsars as a major source of r-process elements,\" Nature 569 no. 7755, (May, 2019) 241-244, arXiv:1810.00098 [astro-ph.HE] . [88] W. Skidmore, TMT International Science Development Teams, and T. Science Advisory Committee, \"Thirty Meter Telescope Detailed Science Case: 2015,\" Research in Astronomy and Astrophysics 15 no. 12, (Dec, 2015) 1945, arXiv:1505.01195 [astro-ph.IM] . [89] J. P. Gardner et al., \"The James Webb Space Telescope,\" Space Science Reviews 123 no. 4, (Apr, 2006) 485-606, arXiv:astro-ph/0606175 [astro-ph] . [90] THESEUS Collaboration, G. Stratta et al., \"THESEUS: a key space mission concept for Multi-Messenger Astrophysics,\" Adv. Space Res. 62 (2018) 662-682, arXiv:1712.08153 [astro-ph.HE]. [91] G. P. Lamb et al."}],"limit":50,"offset":0}