{"total":13,"items":[{"citing_arxiv_id":"2606.29761","ref_index":38,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Estimating Cosmological Parameters from Localized Fast Radio Bursts: A Method for Removing Milky Way Dispersion-Measure Contributions","primary_cat":"astro-ph.CO","submitted_at":"2026-06-29T04:12:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A differential DM method using same-sky localized FRBs removes Milky Way contributions without Galactic models and produces a different constraint on Γ ≡ Ω_b H_0 f_d from current data compared to conventional approaches.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.29388","ref_index":29,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing the Baryon Distribution with Fast Radio Bursts","primary_cat":"astro-ph.CO","submitted_at":"2026-06-28T13:26:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Forecasts indicate SKA FRB observations can constrain baryonic feedback models, measure circumgalactic medium properties, and aid reionization studies through DM statistics and scattering timescales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27714","ref_index":196,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Fast Radio Bursts as Cosmological Probes","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T04:44:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"FRBs serve as cosmological probes via dispersion measure, scattering, and Faraday rotation to constrain baryon distribution, expansion history, magnetic fields, and fundamental physics effects.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25214","ref_index":40,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Fast Radio Bursts probe Galaxy Evolution: Evidence and implications of a redshift-dependent FRB host DM","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T22:20:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Forward modeling of 90 localized FRBs from DSA and ASKAP yields n_z = 1.62^{+1.48}_{-1.57} for DM_host(z) ∝ (1+z)^{n_z}, excluding n_z=0 at 1σ.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24061","ref_index":22,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"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":"2606.12980","ref_index":154,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Review on Resolving the Hubble Tension via Late-Universe Physics","primary_cat":"astro-ph.CO","submitted_at":"2026-06-11T07:13:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A review of late-universe models concludes that DESI BAO plus uncalibrated supernovae data indicate the Hubble tension originates in new low-redshift physics.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[153] presented the first estimation of the Hubble constant, H0 = 62.3 ± 9.1 km s−1 Mpc−1, based on a sample of 9 FRBs. By incorporating priors for DMIGM [151] and DMhost [152] derived from the IllustrisTNG simulation, Wu et al. [144] obtained a more constrained result of H0 = 68.81+4.99 −4.33 km s−1 Mpc−1 using 18 localized FRBs. Subsequently, James et al. [154] reported H0 = 73+12 −8 km s−1 Mpc−1. Their analysis employed an updated sample comprising 16 Australian Square Kilometre Array Pathfinder (ASKAP) FRBs detected by the Commensal Real-time ASKAP Fast Transients (CRAFT) Sur- vey and localized to their host galaxies, and 60 unlocalized FRBs from Parkes and ASKAP . Furthermore, Hagstotz et al. [153] conducted a forecast using a realistic mock sample,"},{"citing_arxiv_id":"2606.10538","ref_index":191,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"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":"2606.07087","ref_index":198,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst","primary_cat":"astro-ph.HE","submitted_at":"2026-06-05T09:34:11+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"A reported periodic fast radio burst is reclassified as Galactic pulsar emission due to CHIME calibration and beam-pointing error.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06766","ref_index":72,"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":"2604.22105","ref_index":53,"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":"2604.03163","ref_index":63,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cosmological Constraints from GW-FRB Associations without Redshift Measurements for LIGO-Virgo and Cosmic Explorer","primary_cat":"astro-ph.CO","submitted_at":"2026-04-03T16:36:16+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":"2509.07097","ref_index":41,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger","primary_cat":"astro-ph.GA","submitted_at":"2025-09-08T18:00:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"FRB dispersion measures from CHIME/FRB Outrigger constrain gas mass fractions in galaxy groups and clusters, consistent with eROSITA at R500 but with mild tension at R200.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2408.04878","ref_index":5,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Modelling DSA, FAST and CRAFT surveys in a z-DM analysis and constraining a minimum FRB energy","primary_cat":"astro-ph.CO","submitted_at":"2024-08-09T05:48:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"z-DM modeling of multiple FRB surveys constrains minimum burst energy to log E_min = 39.49^{+0.39}_{-1.48} erg and predicts 25-41% of FAST FRBs at z ≳ 2.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}