{"total":12,"items":[{"citing_arxiv_id":"2606.31978","ref_index":242,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies?","primary_cat":"astro-ph.GA","submitted_at":"2026-06-30T17:18:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Quiescent galaxies cluster more strongly than star-forming ones by 0.5-1 dex after halo-mass matching, with one-halo conformity up to z~2 that disappears at higher redshifts.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30757","ref_index":283,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:00:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKAO continuum surveys will detect radio emission from JWST AGN and LRDs and distinguish between Compton-thick absorption, intrinsically weak accretion, and dense gas cocoon scenarios.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28489","ref_index":114,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web","primary_cat":"astro-ph.GA","submitted_at":"2026-06-26T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Galaxy size-mass relations exhibit double power-law breaks at different pivot masses for quiescent versus bulge-dominated samples, coinciding with AGN activity scales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28099","ref_index":112,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Thermal Sunyaev-Zel'dovich cross-correlations with unWISE galaxies: disentangling radio contamination, dust properties, and electron pressure","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T13:56:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Radio contamination must be jointly fit with tSZ and CIB in unWISE-Planck/ACT cross-spectra; its inclusion yields positive signals to ℓ ≃ 6000 that match a two-parameter generalized NFW pressure profile.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23790","ref_index":153,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters","primary_cat":"astro-ph.GA","submitted_at":"2026-06-22T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Anisotropic quenching is detected at the highest redshift yet and linked to preprocessing dominating over intrahalo effects by ~20% along the major axis in a delay-then-rapid quenching model informed by cluster accretion histories.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11308","ref_index":112,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"pop-cosmos: Disentangling galaxy properties from observables using data-driven approaches","primary_cat":"astro-ph.GA","submitted_at":"2026-06-09T18:00:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A beta-VAE analysis of pop-cosmos models finds that five latent dimensions capture the rest-frame optical SED, corresponding to stellar mass, recent star formation, dust, and two gas ionization states.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10538","ref_index":189,"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":"2606.04208","ref_index":53,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy","primary_cat":"astro-ph.GA","submitted_at":"2026-06-02T20:52:21+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"HETDEX PDR1 releases an expanded public catalog of 426,654 LAEs, 491,411 [O II] emitters and additional sources from 86.67 sq deg of integral-field spectroscopy with improved classifiers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23457","ref_index":279,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Cosmic web stripping and starvation of low-mass filament galaxies in TNG50","primary_cat":"astro-ph.GA","submitted_at":"2026-05-22T10:16:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Low-mass filament galaxies in TNG50 exhibit smaller asymmetric cold gas discs due to cosmic web tidal fields causing altered accretion or starvation and late-time stripping, while integrated stellar and halo properties remain similar to field counterparts after mass and environment controls.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.17022","ref_index":44,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The contribution from small scales on two-point shear analysis: comparison between power spectrum and correlation function","primary_cat":"astro-ph.CO","submitted_at":"2025-12-18T19:37:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Harmonic-space cosmic shear analysis yields 2-3 times smaller model-choice biases in S8 than real-space analysis when pushing to small scales, with BACCO emulator plus TATT model giving the most consistent constraints between spaces.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2405.00809","ref_index":65,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Kinetic Sunyaev Zel'dovich velocity reconstruction from Planck and unWISE","primary_cat":"astro-ph.CO","submitted_at":"2024-05-01T18:47:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Quadratic estimator reconstructs kSZ remote dipole from Planck and unWISE data with S/N of order unity, constrains multiplicative optical depth bias b_v < 1.04 at 68% confidence after foreground cleaning.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2105.13549","ref_index":148,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","primary_cat":"astro-ph.CO","submitted_at":"2021-05-28T01:58:58+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"DES Y3 3x2pt analysis constrains S8=0.776±0.017 and Ωm=0.339±0.032 in flat ΛCDM, consistent with Planck CMB results at p=0.13-0.48.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"The final Gold sample used in this work after all cuts contains 319 million objects. In addition to the wide-field Gold sample, we rely on data from the DES deep fields [116] covering a subset of the 27 deg2 DES transient search regions and the separate COSMOS field [147]. These images are taken in ugrizY bandpasses with DECam, and also have overlapping VIDEO [148] or Ul- traVISTA [149] imaging for near-IR photometry in YJHK over most of the area. Coadd images are constructed from the best images (i.e., with smallest point-spread function (PSF) full-width half-maximum (FWHM)) with a goal of attaining a depth approximately 10× the typical wide-field coadd image depth. From these coadd images, we produce a deep catalog"}],"limit":50,"offset":0}