{"total":10,"items":[{"citing_arxiv_id":"2606.29300","ref_index":3,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"SPICE: Scintillation Pipeline for Interferometric Candidate Extraction","primary_cat":"astro-ph.IM","submitted_at":"2026-06-28T09:40:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"SPICE is an automated pipeline that recovers known pulsars in GMRT data by detecting scintillation signatures in interferometric visibilities.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26072","ref_index":2,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Observations of the Cosmic Dawn and Epoch of Reionization with the SKAO: Observational Lessons Learned from Precursors and Pathfinder Instruments","primary_cat":"astro-ph.IM","submitted_at":"2026-06-24T17:47:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Summarizes observational lessons on simulation pipelines and systematic mitigation from SKAO precursors for Cosmic Dawn and EoR studies.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"(2024) and Munshi et al. (2025a). ThefirstyearsofCosmicDawnobservationswithNenuFARhaveprovidedvaluableinsightintothe challenges faced by compact low-frequency arrays operating in the30−85MHz range. Three key lessons emerged: (1) impedance mismatches in the analogue chain generate cable reflections that needtobeaccuratelymodelledandmitigatedindelayspace;(2)thelocalRFIenvironment,though relativelystable,remainsdynamicanddominatedbyintermittentground-basedemittersthatcanbe identifiedthroughnear-fieldimaging;and(3)thesuccessofdeepintegrationsdependscriticallyon the selection of a clean, high-latitude field with minimal bright Galactic and extragalactic sources and high elevation. These lessons have direct relevance for the design and calibration strategy of"},{"citing_arxiv_id":"2606.25158","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T20:45:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"SKAO will enable detection of synchrotron emission from prestellar cores to probe their magnetic field properties in nearby star-forming regions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20836","ref_index":43,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Old and Bright: The Remarkable Radio Brightening of the Engine-driven SN 2012au Several Years After Explosion Signals the Birth of a PWN","primary_cat":"astro-ph.HE","submitted_at":"2026-06-18T18:21:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Late-time radio observations of SN 2012au show re-brightening best explained by emission from a newborn pulsar wind nebula rather than continued shock interaction with circumstellar material.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"3 β,(42) whereβ≡v/candτ n es(t) is determined by the balance between pair creation and annihilation (Metzger & Piro 2014, their Eq. 14). We considerτ n es(t) in the limit t≫t sd ast fo > tsd for our relevant range of parameters. Setting Equation 42 equal to Equation 14 in Metzger & Piro (2014)17 we find: tfo = 760 d \u0012 β 1.67×10 −3 \u0013−1\u0012 B∗ 5×10 14G \u0013−2/3 ,(43) 17 With normalization revised for self-consistency with our spin- down time-scale definition of Equation 26 SN 2012au Radio re-brightening27 where we normalize to our average value ofB ∗ and a nebula expansion velocity ofv= 500 km/s as inferred from observations. The total number of pairs at freeze out is then: Nfo ± =n fo ±V fo = τ n es(tfo) σT Rfo"},{"citing_arxiv_id":"2606.18333","ref_index":121,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Polarisation and Faraday rotation measure imaging at metre wavelengths with sub-arcsecond resolution: a foundational calibration strategy","primary_cat":"astro-ph.IM","submitted_at":"2026-06-16T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A calibration strategy using full-Jones corrections with an in-field unpolarised calibrator and visibility-based multi-epoch alignment enables sub-arcsecond polarimetric imaging with LOFAR at metre wavelengths.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21840","ref_index":129,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Powerful Radio Sources in the Southern Sky. 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":190,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"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":"2605.17253","ref_index":235,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"HI Observations of Baryon-Dominated Dwarf Galaxy Candidates","primary_cat":"astro-ph.GA","submitted_at":"2026-05-17T04:22:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Resolved HI observations of six baryon-dominated dwarf galaxy candidates show four are dark-matter deficient with high baryon efficiency, two in isolated environments without tidal signs.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.11966","ref_index":29,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Limit on high energy neutrino emission from Abell 119 using IceCube 10-year muon track data","primary_cat":"astro-ph.HE","submitted_at":"2026-05-12T11:19:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Upper limit on muon neutrinos from Abell 119 is 1.2 times below the flux predicted for hadronic gamma-ray production, marginally excluding that origin.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"from this cluster was carried out using the COMPTEL and INTEGRAL satellites, but null results were obtained [27]. This cluster has also been extensively imaged in X-Rays using the Chandra satellite (See [26] and references therein.) Abell 119 has also been imaged in radio 2 waves at 1.4 GHz as part of the FIRST survey [28] and 150 MHz as part of TIFR GMRT Sky Survey [29]. Abell 119 has also been detected ar microwave lengths using the Sunyaev- Zeldovich effect using the Planck Satellite [30]. Finally we note that accretion shocks in nearby galaxy clusters such as VIRGO have also been proposed as potential sources of ultra-high cosmic rays detected by Pierre Auger Observatory [31]. However, since Abell 119 is ten times further away than VIRGO, it is unlikely to produce any of the events observed"},{"citing_arxiv_id":"2504.01669","ref_index":29,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics","primary_cat":"astro-ph.CO","submitted_at":"2025-04-02T12:17:19+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":2.0,"formal_verification":"none","one_line_summary":"The CosmoVerse White Paper compiles observational tensions in cosmology and maps strategies using improved systematics checks and tests of fundamental physics to resolve them.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}