{"total":13,"items":[{"citing_arxiv_id":"2606.28314","ref_index":32,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Role of Scintillation in Detecting HI Absorption in FRB Spectra","primary_cat":"astro-ph.HE","submitted_at":"2026-06-26T17:56:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations indicate HI absorption in FRB spectra is detectable when scintillation decorrelation bandwidth differs markedly from absorption width, with ≳1000 stacked bursts needed at current sensitivities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27225","ref_index":81,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A search for Fast Radio Bursts from globular clusters in M49 with FAST","primary_cat":"astro-ph.HE","submitted_at":"2026-06-25T16:13:28+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A 9-hour FAST observation covering ~4230 GCs in M49 found no FRBs and sets an upper limit of 4.7e-4 FRB GC^-1 hr^-1 above ~16.5 mJy ms fluence.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26334","ref_index":82,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Debiasing the Observed Fast Radio Burst Population with the CHIME/FRB Selection Function","primary_cat":"astro-ph.HE","submitted_at":"2026-06-24T19:21:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Analysis of CHIME/FRB Catalog 2 with synthetic injections and a multidimensional selection function yields evidence for a slight downturn in the intrinsic scattering timescale distribution, though flat or rising distributions remain possible.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25580","ref_index":51,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The magnetic field in the Milky Way Galaxy: from large to small scales","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T08:54:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"The paper describes the expected capabilities of the SKA-Mid survey to produce a complete map of the Milky Way's magnetic field in the southern hemisphere using rotation measures and polarized emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24061","ref_index":41,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing Baryonic Feedback Effect with CSST Weak Lensing and Future FRB Measurements","primary_cat":"astro-ph.CO","submitted_at":"2026-06-23T02:10:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Forecasts using mock CSST lensing and SKA/DSA-2000 FRB DM data show joint analysis improves log10 T_AGN precision from 3.1% to 0.4% and tightens sum m_nu upper limit to <0.47 eV.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23926","ref_index":71,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Detection of relativistic orbital deformation from improved timing of PSR J1757$-$1854","primary_cat":"astro-ph.HE","submitted_at":"2026-06-22T20:44:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"First detection of relativistic angular deformation δ_θ in PSR J1757−1854 via MeerKAT-enhanced timing, ruling out two of four prior geometric solutions while confirming GR consistency for orbital decay.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.19276","ref_index":51,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Improved proper motion and gravity tests with PSR J1913+1102","primary_cat":"astro-ph.HE","submitted_at":"2026-06-17T16:52:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Updated timing of PSR J1913+1102 yields threefold better total mass precision and fivefold better intrinsic orbital decay, consistent with general relativity and constraining dipolar gravitational wave emission plus scalarisation near 1.6 solar masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.18823","ref_index":50,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Discovery of a 24-millisecond pulsar in a very long orbit with the Murchison Widefield Array","primary_cat":"astro-ph.HE","submitted_at":"2026-06-17T08:45:23+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Discovery of PSR J0125-5854, a 24 ms pulsar in a binary with orbital period ~834 days, low eccentricity, and likely helium white dwarf companion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10538","ref_index":64,"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":"2605.04988","ref_index":37,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The one and the only: the pulsar - white dwarf system in NGC 6749","primary_cat":"astro-ph.HE","submitted_at":"2026-05-06T14:46:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A phase-coherent 20-year timing solution for PSR J1905+0154A yields precise spin, orbital and astrometric parameters, identifies a helium white dwarf companion of 0.17-0.19 solar masses, and indicates the system may be unbound from NGC 6749.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.05093","ref_index":32,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Great Walls of Cosmic Baryons in the Northern Sky","primary_cat":"astro-ph.CO","submitted_at":"2026-04-06T18:46:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"FRB dispersion measures reveal a large-scale excess of ionized gas in the northern sky spatially aligned with the Ursa Major supercluster.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.01203","ref_index":60,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The RRATalog: a Galactic census of rotating radio transients","primary_cat":"astro-ph.HE","submitted_at":"2026-04-01T17:47:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"RRATs number up to 400000 in the Galaxy with a birth rate of at most 1.4 per century, comparable in size to pulsars at high luminosities and consistent with supernova rates.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.20663","ref_index":33,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"FAST Polarization Catalog of FRB 20240114A","primary_cat":"astro-ph.HE","submitted_at":"2026-03-21T05:39:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A polarization catalog of 6,131 bursts from FRB 20240114A reveals linearly decreasing rotation measure, stable dispersion measure, high linear polarization fractions, low circular polarization, and a broad distribution of intrinsic polarization angles, indicating a dynamically evolving magneto-ionic","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}