{"total":15,"items":[{"citing_arxiv_id":"2606.30413","ref_index":36,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Sloshing Motions in Abell 3571 Revealed by XRISM/Resolve Velocity Mapping","primary_cat":"astro-ph.HE","submitted_at":"2026-06-29T15:00:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"XRISM velocity maps of Abell 3571 show subsonic gas motions and thermodynamic asymmetry consistent with early-phase sloshing from an off-axis minor merger with Abell 3572 as candidate perturber.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28915","ref_index":35,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Tracing the Orbital Motion of the Accreting White Dwarf in EX~Hydrae with XRISM/Resolve","primary_cat":"astro-ph.HE","submitted_at":"2026-06-27T13:45:02+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"XRISM/Resolve high-resolution spectroscopy detects coherent orbital modulation in Fe XXV Kα line centroids from EX Hydrae, yielding K1 = 58.1 km/s and a white dwarf mass of 0.79 solar masses consistent with optical tracers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17371","ref_index":108,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Reduced Effective Viscosity from Anisotropic Transport and Plasma Instabilities in the Sloshing Cores of Galaxy Clusters","primary_cat":"astro-ph.GA","submitted_at":"2026-06-16T00:02:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Braginskii-MHD simulations of sloshing cluster cores show that pressure-anisotropy limiters plus turbulent magnetic structure reduce effective viscosity far below the Spitzer value, steepening velocity spectra and dissipating a small fraction of turbulent kinetic energy.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10028","ref_index":149,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures","primary_cat":"astro-ph.CO","submitted_at":"2026-06-08T18:08:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"50 constrained simulations of Coma cluster analogues reproduce the observed radial X-ray surface brightness and Compton-y profiles within the scatter expected from environment and assembly history.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.08773","ref_index":102,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context","primary_cat":"astro-ph.SR","submitted_at":"2026-06-07T18:37:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New X-ray flare detections from M dwarfs combined with literature data yield flare frequency constraints and an upper limit of 0.5-30 Myr on atmospheric loss times for habitable planets orbiting them.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.08349","ref_index":46,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos","primary_cat":"astro-ph.HE","submitted_at":"2026-05-08T18:01:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Ancient cosmic ray halos from the central galaxy boost Perseus's cool core via inverse-Compton scattering, simultaneously explaining radio minihalo, giant halo, X-ray properties, and gamma-ray data without re-acceleration.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06917","ref_index":56,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf","primary_cat":"astro-ph.HE","submitted_at":"2026-05-07T20:27:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"X-ray spectral modeling and timing analysis of V1674 Her constrain its white dwarf mass to 1.09-1.12 solar masses, well below the near-Chandrasekhar value expected from its t2~1 day decline time.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05068","ref_index":59,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The NUV transit of XO-3 b","primary_cat":"astro-ph.EP","submitted_at":"2026-05-06T16:02:32+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"NUV transit depth of XO-3b measured at 0.1371 with 22-minute late center; X-ray data yield mass-loss rate ~10^4 g/s; bow-shock model predicts early rather than late transit.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.04577","ref_index":182,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"HD3191, the high-mass X-ray binary that wasn't there","primary_cat":"astro-ph.HE","submitted_at":"2026-05-06T07:27:49+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"HD3191 is a single rapidly rotating B1 IV:nn star showing multi-mode non-radial pulsations, not a high-mass X-ray binary.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.02998","ref_index":69,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The SRG/eROSITA diffuse soft X-ray background II. spectra and morphology of the eROSITA bubbles in the western Galactic hemisphere","primary_cat":"astro-ph.HE","submitted_at":"2026-05-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Spectra of the western eROSITA bubbles reveal two uniform components at 0.60 keV and 0.21 keV with sub-solar abundances, plus a geometrical model constraining horizontal size to ~6 kpc but leaving vertical extent uncertain.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.24494","ref_index":42,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation","primary_cat":"astro-ph.GA","submitted_at":"2026-04-27T13:59:12+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"TNG50 MW analogues reproduce global soft X-ray luminosity, inner surface brightness, emission measure and O VII absorption but show too-steep radial decline in X-ray brightness and 65% lower O VIII absorption than observed, indicating overly central feedback.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.22255","ref_index":37,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Quiescent and flaring states of three active stars: V834 Tau, LQ Hya, and BY Dra","primary_cat":"astro-ph.SR","submitted_at":"2026-04-24T05:57:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"X-ray data from V834 Tau, LQ Hya, and BY Dra show two-temperature quiescent coronae with iron depletion and six superflares, with recurrent events on LQ Hya suggesting stable magnetic structures.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.22105","ref_index":103,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers","primary_cat":"astro-ph.CO","submitted_at":"2026-04-23T22:27:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"FRB DMs correlate at 2.6-5 sigma with galaxies, weak lensing, CIB, CMB lensing, tSZ, X-ray clusters, SXRB and radio continuum, consistent with moderate feedback models while ruling out weak feedback at 3.5 sigma via SXRB-DM.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.07976","ref_index":73,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The puzzling story of flare inactive ultra fast rotating M dwarfs -- III. Investigating X-ray Activity","primary_cat":"astro-ph.SR","submitted_at":"2026-04-09T08:43:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"X-ray data show ultra-fast rotating M dwarfs have saturated or enhanced coronal emission, ruling out supersaturation as the cause of their unexpectedly low flaring activity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.06591","ref_index":44,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Plasma Dynamics of Radiative Cooling Accretion Flow in AM Herculis with XRISM","primary_cat":"astro-ph.HE","submitted_at":"2026-04-08T02:21:24+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"XRISM spectroscopy of AM Herculis reveals bulk velocity and temperature gradients in the radiative cooling accretion column, with derived shock temperature of 24 keV, velocity of 1116 km/s, and density of 5-6 x 10^15 cm^-3.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}