{"total":10,"items":[{"citing_arxiv_id":"2606.31515","ref_index":280,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine","primary_cat":"astro-ph.GA","submitted_at":"2026-06-30T11:29:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"LRD host galaxies show average metallicity 0.08 Z_sun with narrow stable range, challenging pristine-gas formation models while ruling out typical local AGN.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21614","ref_index":182,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Little Red and Blue Dots: AGN-excited narrow lines, Lyman-$\\alpha$ emission, and resemblance to standard quasars","primary_cat":"astro-ph.GA","submitted_at":"2026-06-19T17:18:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"JWST data on LRDs and LBDs show AGN-like excitation, strong Lyα with broad components, and X-ray weakness, implying clumpy or equatorial geometries around growing black holes rather than complete gas envelopes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12355","ref_index":192,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Between Degeneracy and Evolution: UV-to-optical Insights into the BH$^*$ Model in Little Red Dots","primary_cat":"astro-ph.GA","submitted_at":"2026-06-10T17:27:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Bayesian continuum fitting of 66 LRDs shows the BH* model fits ~6% best, rising to ~40% under AGN-disfavoring priors, with most objects stellar/AGN-dominated and possible evolutionary trends.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05281","ref_index":54,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations","primary_cat":"astro-ph.GA","submitted_at":"2026-06-03T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Derives idealized P-L-T relation from hydrostatic envelope model for LRDs and uses sparse data to obtain preliminary H0 = 120.7 with large errors as proof-of-concept.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03522","ref_index":22,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The UV Side of Little Red Dots: Red, Compact, and Iron-Enhanced Rest-UV Emission with a Strong Downturn around Ly$\\alpha$","primary_cat":"astro-ph.GA","submitted_at":"2026-06-02T11:44:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Analysis of ~100 JWST LRDs finds redder, compact UV emission with Fe II/Mg II ~8-10 and correlations suggesting central red continuum (β_UV~0) beyond host galaxy contribution.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.29895","ref_index":24,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Transient Signatures of Star-Envelope Collisions in Little Red Dots","primary_cat":"astro-ph.HE","submitted_at":"2026-05-28T13:19:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Red supergiant collisions with massive gaseous envelopes around SMBHs in LRDs can produce detectable transients at rates up to ~0.3 yr^{-1} per LRD for compact clusters of size ≲10 pc.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.27903","ref_index":7,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Double Dots: Compact Pairs Mark Little Red Dots and High-Redshift Broad-line AGNs","primary_cat":"astro-ph.GA","submitted_at":"2026-05-27T03:26:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Close compact pairs mark ~67% of known Little Red Dots and both high-redshift BLAGNs in the A2744 field, suggesting merger-driven accretion at high redshift.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15263","ref_index":152,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"On the quenching of LRD X-ray emission by both Compton-thick gas and high accretion rates","primary_cat":"astro-ph.GA","submitted_at":"2026-05-14T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LRDs require Compton-thick gas at moderate metallicity plus high accretion rates producing weak X-rays to explain their non-detection, implying they are not chemically pristine.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15189","ref_index":171,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Strong Gravitational Lensing with the James Webb Space Telescope","primary_cat":"astro-ph.CO","submitted_at":"2026-05-14T17:59:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review summarizing recent advances in strong gravitational lensing applications and near-future prospects with the James Webb Space Telescope.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[169] Golubchik M, Furtak LJ, Allingham JFV, et al. VENUS: When Red meets Blue - A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383. arXiv e-prints. 2025 Dec;:arXiv:2512.02117. [170] Sharon K, Gladders MD, Rigby JR, et al. Source-plane Reconstruction of the Bright Lensed Galaxy RCSGA 032727-132609. Astrophys. J.. 2012 Feb;746(2):161. [171] Zitrin A, Broadhurst T, Coe D, et al. Strong-lensing analysis of MS 1358.4+6245: New multiple images and implications for the well-resolved z= 4.92 galaxy. Mon. Not. R. Astron. Soc.. 2011 May;413:1753-1763. [172] Law DR, Shapley AE, Steidel CC, et al. High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18. Nature. 2012 Jul;487(7407):338-340."},{"citing_arxiv_id":"2602.02702","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation","primary_cat":"astro-ph.GA","submitted_at":"2026-02-02T19:13:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"UV-bright companions to Little Red Dots provide Lyman-Werner fluxes of J21 ~ 10^2.5-10^5 that can suppress H2 cooling and enable direct collapse to massive black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}