{"total":53,"items":[{"citing_arxiv_id":"2607.07750","ref_index":85,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Multi-Wavelength Signatures of a Giant Cometary Radio Halo in MACSJ0417-1154","primary_cat":"astro-ph.HE","submitted_at":"2026-07-08T11:28:23+00:00","verdict":"CONDITIONAL","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"MACSJ0417’s giant radio halo shows spectral steepening and radio–X-ray correlation consistent with turbulence from a 6:1 off-axis merger that preserved the cool core; pure hadronic models are energetically excluded.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.06143","ref_index":198,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Deep far-UV observations of the ELAIS N1 field using AstroSat: Source catalogue, spectral energy distribution modelling and star 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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":"2606.23393","ref_index":23,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A $\\lambda=1.3$ millimeter Survey for Disks around Herbig Be Stars","primary_cat":"astro-ph.SR","submitted_at":"2026-06-22T14:19:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"A millimeter survey detects disks around five Herbig 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IV. Observations of the G4Jy-3CRE Catalog with the Australian Square Kilometre Array Pathfinder","primary_cat":"astro-ph.GA","submitted_at":"2026-05-21T00:19:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New ASKAP continuum imaging classifies jet morphologies in 173 G4Jy-3CRE sources (66% of sample) including 37 newly detected jets and identifies six new optical counterparts.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19217","ref_index":91,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Taking Inventory of the Most Promising Lensed Radio Sources for Constraining Fundamental Properties of Dark Matter","primary_cat":"astro-ph.CO","submitted_at":"2026-05-19T00:43:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Reports results from two searches for new radio lenses in existing surveys and discusses the completeness of the population usable for constraining dark matter properties via astrometric perturbations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16917","ref_index":283,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky","primary_cat":"astro-ph.GA","submitted_at":"2026-05-16T10:13:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"SPICE-RACS DR2 delivers the largest single Faraday rotation measure catalog from a radio survey, with 250,000-340,000 RMs across most of the sky at median uncertainty of 2 rad m^{-2}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16495","ref_index":150,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A 14-year-old Mystery: The Peculiar Case of the Engine-driven SN 2012ap","primary_cat":"astro-ph.HE","submitted_at":"2026-05-15T18:00:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Late-time radio rebrightening in SN 2012ap is consistent with either progenitor mass-loss variation producing a density enhancement or an off-axis energetic jet viewed at large angle, potentially reclassifying it as GRB-like rather than weakly engine-driven.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15555","ref_index":40,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A VLBA-resolved Jet Associated with Super-Eddington Accretion in a Radio-loud Quasar at $z=3.4$","primary_cat":"astro-ph.GA","submitted_at":"2026-05-15T02:48:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"VLBA multi-frequency imaging reveals a relativistic, well-collimated jet of ~745 pc in a z=3.4 super-Eddington radio-loud quasar, distinct from low-redshift analogues.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15444","ref_index":42,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Clusters Hiding Under Millimeter Sources (CHUMS) I: Extreme CHUMS","primary_cat":"astro-ph.CO","submitted_at":"2026-05-14T21:58:46+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"AGN emission from central galaxies hides galaxy clusters in SZ surveys; CARMA-based subtraction recovers high-SNR detections in ACT maps for three specific clusters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.11101","ref_index":85,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Tracing Radio AGN-Driven Quenching in Post-Starburst Galaxies at Cosmic Noon","primary_cat":"astro-ph.GA","submitted_at":"2026-05-11T18:06:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Post-starburst galaxies at cosmic noon show very low radio detection rates and compact weak sources, consistent with short-lived low-luminosity AGN, while older quiescent galaxies exhibit stronger extended radio emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06766","ref_index":107,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline","primary_cat":"astro-ph.IM","submitted_at":"2026-05-07T18:00:00+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"The PINK updates enhance the CELEBI FRB pipeline with better astrometry, time-frequency gating, polarization calibration, DM optimization tools, and a software container for improved efficiency and localization of events like FRB 20251019A.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05303","ref_index":92,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Multi-wavelength outburst activity from EP J174942.2-384834: a very faint X-ray transient discovered by Einstein Probe","primary_cat":"astro-ph.HE","submitted_at":"2026-05-06T18:00:02+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"EP J174942.2-384834 is classified as a very faint X-ray transient black hole candidate based on its hard X-ray spectra, optical/UV brightening correlated with X-rays, and lack of radio emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.01981","ref_index":61,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Comprehensive Study of Morphology and Kinematics in Extended Nebulae Around UV Luminous Quasars at $z\\approx1$","primary_cat":"astro-ph.GA","submitted_at":"2026-05-03T17:30:40+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.27065","ref_index":51,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Dwarf Galaxies Hosting Extreme Star-Forming Regions and (Variable) AGNs at Radio Wavelengths","primary_cat":"astro-ph.GA","submitted_at":"2026-04-29T18:01:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Dwarf galaxies host compact thermal HII regions powered by up to 100,000 O-type stars and exhibit radio variability consistent with AGNs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.21405","ref_index":8,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Supermassive Black Hole Winds in X-rays: SUBWAYS IV. Tracing Radio Emission and Unveiling the Role of Winds","primary_cat":"astro-ph.GA","submitted_at":"2026-04-23T08:20:42+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.5,"formal_verification":"none","one_line_summary":"In the SUBWAYS sample, UFO-hosting AGN show larger radio extent and steep spectra consistent with wind-driven shocks, while ~80% of sources show outflow-like radio emission.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"winds and jets we refer to them more generally as outflows. Article number, page 2 of 25 E. Amenta et al.: Supermassive Black Hole Winds in X-rays: SUBW AYS Table 1.Table with general parameters of the sources in the SUBW AYS sample. ID Target Name R.A. Dec.z D L logL bol logL 2−10 keV logM BH logλ Edd vout J2000 J2000 (Gpc) (erg/s) (erg/s) (M ⊙) (c) (1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) 5 PG0804+761 08:10:58.60+76:02:43.00 0.100 0.46 45.27 44.46±0.01 8.31 +0.04 −0.04 -1.07 0.13±0.01 6 PG0947+396 09:50:48.42+39:26:50.64 0.205 1.01 45.89 44.37±0.01 8.68 +0.08 −0.10 -1.24 0.31 +0.02 −0.04 11 2MASXJ1051+35 10:51:44.24+35:39:30.76 0.159 0.76 44.88 43.70±0.01 8.40 +0.30 −0.30 -1.92 0.24±0.01 10 PG1114+445 11:17:06.40+44:13:33."},{"citing_arxiv_id":"2604.20609","ref_index":39,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Deep VLBI constraints on compact radio cores in four ultraluminous X-ray sources","primary_cat":"astro-ph.HE","submitted_at":"2026-04-22T14:23:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Deep VLBI observations of four ULXs yield no compact radio detections and tight upper limits, disfavoring persistently bright hard-state-like compact cores.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.20095","ref_index":13,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Detections of nearly bias-free core shifts with 5-30 $\\mu$as precisions at 8-43 GHz in BL Lacertae","primary_cat":"astro-ph.HE","submitted_at":"2026-04-22T01:27:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"High-precision VLBI detects 250 μas core shift between 8.4 and 43.2 GHz in BL Lacertae, with fitted index k_r = 1.18 consistent with equipartition.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.19896","ref_index":81,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"HI 21-cm absorption in low- and high-excitation radio-loud AGNs at $z<0.5$ from MALS","primary_cat":"astro-ph.GA","submitted_at":"2026-04-21T18:20:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Five new HI 21-cm absorption detections in LERGs and HERGs at z<0.5 reveal disturbed gas kinematics with velocity offsets over 350 km/s and a 3% detection rate consistent with lower-redshift samples.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.19435","ref_index":86,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy","primary_cat":"astro-ph.HE","submitted_at":"2026-04-21T13:09:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.13650","ref_index":73,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Prospects for GRB Afterglow Discovery with the Eric and Wendy Schmidt Observatory System","primary_cat":"astro-ph.HE","submitted_at":"2026-04-15T09:17:44+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations predict Argus and DSA will serendipitously catch GRB afterglows at rates of ~47/yr (Argus, reliable-fade metric) and ~82/yr (DSA) for Fermi/GBM LGRBs, with ~116 optical and ~217 radio orphan afterglows per year.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.13152","ref_index":30,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Persephone's Torch: A 15th Magnitude Quadruply-Lensed Quasar From the Couch Discovered with SPHEREx and the LBT","primary_cat":"astro-ph.GA","submitted_at":"2026-04-14T18:00:00+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Spectroscopic and imaging confirmation of the brightest known quadruply-lensed quasar J1330-0905 at z=2.22 with Einstein radius ~0.45 arcsec and predicted magnification ~56.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.11881","ref_index":50,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A sample of short-lived Galactic radio transients from ASKAP VAST","primary_cat":"astro-ph.HE","submitted_at":"2026-04-13T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Six new Galactic radio transients found and classified into two types, proposed to originate from wide-orbit white dwarf binaries.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.07431","ref_index":21,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Detection and Evolution of Linear Polarization of the Galactic Center Transient MAXI J1744-294","primary_cat":"astro-ph.HE","submitted_at":"2026-04-08T18:00:00+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"First polarization measurements of MAXI J1744-294 reveal a common Faraday screen with RM = -63606 rad m^{-2} matching the Galactic center magnetar, confirming the transient's location in the nuclear star cluster and suggesting an intrinsic RM for Sgr A*.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.13736","ref_index":36,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Blackbody Quasar and Radio Source (BBQSORS): A Candidate of Transitional Little Red Dots with a $T\\sim10^4\\ K$ Blackbody Spectrum","primary_cat":"astro-ph.GA","submitted_at":"2026-03-14T03:44:29+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A z=1.715 radio-loud quasar exhibits a ~10,000 K blackbody UV continuum and three-component blackbody photometry, marking it as a candidate transitional Little Red Dot.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}