{"total":18,"items":[{"citing_arxiv_id":"2606.30947","ref_index":2,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Square Kilometer Array Synergies for the Epoch of Reionization and Cosmic Dawn","primary_cat":"astro-ph.CO","submitted_at":"2026-06-29T22:01:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"Review of synergies with other telescopes to support SKA-low observations of the cosmic 21-cm signal during reionization and cosmic dawn.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30787","ref_index":39,"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":"2606.26640","ref_index":12,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cm-wavelength Studies of Molecular Gas and Star Formation at High Redshift with the SKA","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T06:05:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Advocates for SKA frequency coverage beyond 15 GHz to observe redshifted low-J CO, HCN and similar lines for cold molecular gas studies in high-redshift galaxies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26209","ref_index":85,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Fast Simultaneous Surveys with On-the-Fly Mapping","primary_cat":"astro-ph.IM","submitted_at":"2026-06-24T17:19:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"MeerKLASS applies on-the-fly imaging on MeerKAT for a 10,000 sq. deg. UHF-band continuum survey at 14 arcsec resolution and 25 μJy/beam rms, run commensally with HI intensity mapping.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25022","ref_index":23,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A massive barred spiral galaxy at z = 5.102 discovered by JWST","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":9.0,"formal_verification":"none","one_line_summary":"Discovery and characterization of the highest-redshift barred spiral galaxy candidate at z=5.102, with bar length ~4.5 kpc, stellar mass 10^10.45 solar masses, SFR 144 solar masses per year, and evidence for AGN and interaction.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.18229","ref_index":30,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"An extreme ram-pressure stripping event in a protocluster at redshift 4.3","primary_cat":"astro-ph.GA","submitted_at":"2026-06-16T17:55:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"ALMA and JWST data reveal an extreme ram-pressure stripping event removing most cold gas from a massive galaxy in a z=4.3 protocluster core.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17210","ref_index":50,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Testing masking effectiveness using multi-line image cubes based on COSMOS2020 for [CII] line intensity mapping at $z_{[CII]} > 3.5$","primary_cat":"astro-ph.GA","submitted_at":"2026-06-15T18:48:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Simulations from COSMOS2020 show masking recovers [CII] above 300 GHz in ideal conditions but noise prevents useful S/N until near the end of 2000-hour observations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13393","ref_index":65,"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":"2606.06108","ref_index":129,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Grain-size evolution and rapid dust growth in high-redshift galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-04T12:53:53+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A multiphase ISM grain-size model with low supernova dust yield reproduces observed dust-to-stellar mass ratios and UV luminosity functions at z=7-12 by letting small grains seed rapid metal accretion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.20698","ref_index":22,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"CO(7-6) and [C I](2-1) survey in z > 6 quasars","primary_cat":"astro-ph.GA","submitted_at":"2026-05-20T04:51:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"ALMA survey of CO(7-6) and [C I](2-1) in 18 z~6 quasars yields molecular gas mass estimates from multiple tracers and indicates that PDR models cannot fully account for the observed excitation, pointing to additional heating processes.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"Line-physics parameters αCO (K km s−1 pc2)−1 0.81 [0.37,1.53] 0.80 [0.40,1.62] r71 -0.18 [0.09,0.32] 0.17 [0.09,0.32] Tex,[CI] K48.67 [38.81,55.99] 46.84 [37.45,56.59] Tex,[CII] K93.50 [79.58,116.62] 100.73 [81.32,119.86] logX CI -−4.81 [−4.98,−4.55]−4.74 [−4.96,−4.51] logX C+ -−4.37 [−4.61,−4.20]−4.40 [−4.62,−4.17] α[CII] M⊙ L−1 ⊙ 13.46 [8.55,21.73] 13.71 [8.07,22.28] Dust-physics parameters κν cm2 g−1 10.05 [6.95,14.70] 10.08 [6.32,15.89] τ-0.23 [0.11,0.44] 0.20 [0.10,0.40] Td K45.59 [39.00,54.31] 45.42 [37.33,54.56] δGDR -102.09 [70.31,172.58] 119.67 [68.55,204.64] Intrinsic scatters σCO,int dex0.13 [0.08,0.18] 0.08 [0.04,0.12] σ[CI],int dex0.09 [0.03,0.18] 0.06 [0.02,0.11] σ[CII],int dex0.18 [0.13,0.25] 0.21 [0."},{"citing_arxiv_id":"2605.15361","ref_index":16,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Clumps in spiral galaxies at $z \\lesssim 3$: Disentangling two spatial modes of star formation","primary_cat":"astro-ph.GA","submitted_at":"2026-05-14T19:40:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Clumps in high-redshift spiral galaxies are smaller than commonly reported, spatially concentrated toward spiral arms, smaller but brighter inside arms than between them, with similar colors, suggesting arms stimulate clump formation but do not alter their star formation properties.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.11070","ref_index":139,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A correlation predicting galaxies without dark matter","primary_cat":"astro-ph.GA","submitted_at":"2026-05-11T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Baryonic fraction in certain galaxies correlates with baryonic acceleration as approximately a_bar inverse, placing known dark-matter-deficient galaxies at the high-acceleration extreme and predicting low dark matter content for ultra-diffuse galaxies brighter than 25 mag arcsec^{-2}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05298","ref_index":73,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Kinematic Stratification in Extremely Red Quasars Revealed by JWST","primary_cat":"astro-ph.GA","submitted_at":"2026-05-06T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"JWST observations of ERQs show stratified gas kinematics via deblended optical emission lines, with UV lines dominated by scattered light and optical lines mixing scattered and obscured emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.04144","ref_index":87,"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":"2604.22559","ref_index":17,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Quasar--Companion System Without AGN Outflow at $z \\sim 6$: The Case of PSO J083+11","primary_cat":"astro-ph.GA","submitted_at":"2026-04-24T13:54:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New ALMA [C II] and FIR data on PSO J083+11 at z=6.34 reveal ordered rotation, typical star-forming ratios, and no outflow signatures in either galaxy, interpreted as a pre-AGN-feedback accretion phase.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.19543","ref_index":35,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Dynamically cold discs in high-redshift galaxies: comparison between ALMA observations and TNG50","primary_cat":"astro-ph.GA","submitted_at":"2026-04-21T15:02:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"TNG50 shows most massive high-z star-forming galaxies are dynamically hotter than ALMA data indicate, with rare cold discs forming from aligned accretion and evolving into one-third discs and two-thirds early-type galaxies by z=0.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.07587","ref_index":12,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Multiphase Gas Structure in the Circumnuclear Region of NGC 5506 Observed with ALMA","primary_cat":"astro-ph.GA","submitted_at":"2026-04-08T20:39:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New ALMA observations of NGC 5506 show a thick rotating CND where supernova-driven turbulence supplies vertical support and AGN outflow dissociates CO.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1906.09656","ref_index":14,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The \"Red Radio Ring\": Ionised and Molecular Gas in a Starburst/Active Galactic Nucleus at $z \\sim 2.55$","primary_cat":"astro-ph.GA","submitted_at":"2019-06-23T21:41:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Detection of [NII]205μm and CO lines plus SED analysis in the Red Radio Ring at z=2.55 shows co-spatial ionized and molecular gas, high column density after dust correction, and starburst-powered ISM.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}