{"total":11,"items":[{"citing_arxiv_id":"2607.00105","ref_index":158,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN","primary_cat":"astro-ph.GA","submitted_at":"2026-06-30T19:45:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Higher Eddington ratio AGN exhibit increased [O III] outflow incidence and reduced obscuration, supporting radiative feedback as the regulator.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30390","ref_index":113,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"SN 2019vxm: A luminous and long-lived Type IIn supernova with early flash-ionisation features","primary_cat":"astro-ph.SR","submitted_at":"2026-06-29T14:44:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"SN 2019vxm is a luminous, long-lived Type IIn supernova showing early flash-ionization features, a power-law bolometric light curve, and mid-IR dust formation, with a progenitor mass-loss rate lower limit of at least 0.01 solar masses per year.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28918","ref_index":77,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Late-time evolution of the interacting stripped-envelope supernova 2017dio","primary_cat":"astro-ph.HE","submitted_at":"2026-06-27T13:49:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Late-time data on SN 2017dio yield mass-loss rates of ~0.2 M_sun/yr peak and ~0.06 typical, with H-rich CSM from a companion and dust masses 0.001-0.02 M_sun, indicating sudden mass-loss increase.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22619","ref_index":171,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation","primary_cat":"astro-ph.SR","submitted_at":"2026-06-21T18:01:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Binary evolution modeling constrains donor masses of 14-23 solar masses for two luminous red novae and shows dust masses are 1-5 orders of magnitude below total ejected envelope masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17734","ref_index":221,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Shape, Orientation and Colors Combined approach for Asteroids (SOCCA)","primary_cat":"astro-ph.EP","submitted_at":"2026-06-16T09:51:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"SOCCA extends HG1G2 by modeling the projected surface of a rotating triaxial ellipsoid to jointly retrieve absolute magnitude, phase parameters, spin state, and shape from sparse multi-band photometry, halving residuals and tripling precision on LSST simulations and Eugenia data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06578","ref_index":237,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A Disappearing Act: Constraints From \"Missing\" Flares of Repeating Partial TDE Candidates","primary_cat":"astro-ph.HE","submitted_at":"2026-06-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Non-detections of expected third flares in TDE 2022dbl and TDE 2020vdq support rpTDE interpretation over independent events, with modeling favoring bound main-sequence star orbits and deep initial encounters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.00208","ref_index":1,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JWST Reveals Large Reservoirs of Dust and Ongoing Circumstellar Interaction in SN Ibn/Icn 2023xgo over a Year Post-Explosion","primary_cat":"astro-ph.HE","submitted_at":"2026-05-29T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Late-time JWST spectra of SN 2023xgo detect cool silicate or carbonaceous dust masses of order 0.01-0.03 solar masses plus narrow He I emission indicating ongoing circumstellar interaction at +377 days.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"529, 155, doi: 10.1093/mnras/stae507 Dust in SN Ibn/Icn 2023xgo21 APPENDIX T able 2.Dust SED modeling priors. Priors are uniform within the reported ranges. Model logM 1 logM 2 T1 T2 logR in logR out [M⊙] [M ⊙] [K] [K] [cm] [cm] Si+Si sphere [−4,0] [−6,−2] [100,500] [400,1800] - [15,19] C+C sphere [−4,0] [−6,−2] [150,500] [500,1800] - [15,19] Si+Si shell [−4,−1] [−6,−2] [150,500] [500,1800] [10,17] [15,19] C+C shell [−4,−1] [−6,−2] [150,500] [500,1800] [10,17] [15,19] C+Si sphere [−4,0] [−6,0] [100,500] [400,1800] - [15,19] C+C optthick [−4,−1] [−6,−2] [150,500] [500,1800] - [15,17] TSi,warm(K) = 608 +61 −36 240 300 360 420 TSi,cold(K) TSi,cold(K) = 385 +42 −51 −3.0 −2.4 −1.8 −1.2 −0.6 log MSi,warm log MSi,warm = -1."},{"citing_arxiv_id":"2605.23814","ref_index":42,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction","primary_cat":"astro-ph.IM","submitted_at":"2026-05-22T16:16:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"ROSSINI achieves integral field spectroscopy without IFUs via rotational slitless imaging combined with tomographic reconstruction, recovering input datacubes to percent-level accuracy in numerical simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19059","ref_index":21,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"VarWISE: Infrared Variability via NEOWISE Single Exposure Photometry","primary_cat":"astro-ph.SR","submitted_at":"2026-05-18T19:29:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"VarWISE catalog identifies 457,080 high-confidence infrared variables (49.81% new) and an extended set of 1.9 million from NEOWISE photometry via spatial clustering, VARnet detection, and XGBoost classification.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13189","ref_index":229,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Accretion Process on Protostars","primary_cat":"astro-ph.SR","submitted_at":"2026-05-13T08:45:38+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"The paper reviews techniques for measuring protostellar accretion, analyzes methodological differences and caveats in comparing observations with simulations, and outlines next steps for a fuller picture.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2405.00809","ref_index":40,"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}],"limit":50,"offset":0}