{"total":12,"items":[{"citing_arxiv_id":"2606.26996","ref_index":6,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"How to access astronomical observation facilities ?","primary_cat":"astro-ph.IM","submitted_at":"2026-06-25T13:13:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"A review and practical guide to the telescope time proposal framework and preparation process in astronomy.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26072","ref_index":8,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"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":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25017","ref_index":66,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Low-frequency VLBI with the SKA-Low","primary_cat":"astro-ph.IM","submitted_at":"2026-06-23T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"LAMBDA proposes megameter-scale baselines using additional Australian stations to extend SKA-Low for high-resolution low-frequency VLBI.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21160","ref_index":34,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Star Formation at the Periphery of a Molecular Superbubble: The Case of G12.79+0.43","primary_cat":"astro-ph.GA","submitted_at":"2026-06-19T06:54:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Observational study of G12.79+0.43 identifies YSOs and HII regions powered by B-type stars and associates the complex with the rim of a molecular superbubble of diameter ~50 pc and expansion age ~0.3 Myr without establishing causality.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05343","ref_index":63,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211","primary_cat":"astro-ph.HE","submitted_at":"2026-06-03T18:35:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Bayesian fitting of an eccentric Keplerian orbit to the radio light curve of PKS 2131-021 gives e = 0.053 ± 0.015 without red noise but favors a circular orbit plus DRW noise with e < 0.15.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04084","ref_index":136,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster","primary_cat":"astro-ph.GA","submitted_at":"2026-06-02T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both young and old electrons to radiate.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01644","ref_index":56,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised","primary_cat":"astro-ph.IM","submitted_at":"2026-06-01T03:50:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"MWA Phase III upgrade adds receivers and uses MWAX correlator to support full 256-tile correlation, doubling sensitivity and quadrupling baselines.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02653","ref_index":4,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Systematic Polarization Errors from Parallactic-Angle Dependent Leakage in Pseudo-Circular Feeds","primary_cat":"astro-ph.IM","submitted_at":"2026-05-31T23:26:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Hybrid imperfections cause parallactic-angle-dependent leakage in pseudo-circular feeds via non-commutative Jones matrix interaction, and a SOP pre-correction is introduced to remove it before sky-frame projection.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.23768","ref_index":189,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies","primary_cat":"astro-ph.SR","submitted_at":"2026-05-22T15:38:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"GMRT sub-GHz survey of 44 magnetic hot stars detects emission in 11 cases and finds scaling of radio luminosity with magnetic field and rotation period consistent with higher-frequency work.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.25278","ref_index":35,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The GMRT High-Resolution Southern Sky Survey for pulsars and transients -- VIII: Orbital Variability and the Evolution of a 1-Day He-WD Millisecond Pulsar J2101-4208","primary_cat":"astro-ph.HE","submitted_at":"2026-04-28T06:36:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"PSR J2101-4802 is a transitional millisecond pulsar with a ~1-day orbit, 0.15 solar mass He-WD companion, and large orbital period derivative that links redback-like systems to detached binaries.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"inclination and impact angle) of this system. The combination of a∼1-day orbit,∼0.15M ⊙ com- panion, modest spin-down power, unusually large ˙Pb, and phase-locked magnetized intrabinary plasma signatures suggests that PSR J2101−4802 represent a transitional system linking redback-like spiders to detached He-WD MSP binaries. Keywords:Pulsar (33) - MSP (35) - Pulsar timing (59) - Polarization (30) 1.INTRODUCTION Millisecond pulsars (MSPs) are rotating neutron stars (NSs) with spin periodsP <30 ms. About 80% of MSPs are in binaries, typically with white dwarf (WD) companions, but also with main-sequence (MS) stars or other NSs (D. R. Lorimer 2008; B. Bhattacharyya & J. Roy 2022). According to the theory of pulsar evolu-"},{"citing_arxiv_id":"2604.15440","ref_index":45,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys","primary_cat":"astro-ph.CO","submitted_at":"2026-04-16T18:01:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Forecasts indicate 10-sigma detection for squeezed triangles and 100-sigma for combined shapes in the 21cm-galaxy cross-bispectrum with 100 hours of SKA-Mid interferometric observations on scales 0.2 to 0.9 per Mpc.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2507.08823","ref_index":10,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Studying Ionospheric Phase Structure Functions Using Wide-Band uGMRT (Band-4) Interferometric Data","primary_cat":"physics.space-ph","submitted_at":"2025-06-30T06:53:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"uGMRT Band-4 data on 3C48 show ionospheric phase structure functions with power-law turbulence, diffractive scales of 6.7-8.3 km, and anisotropy consistent with MSTIDs at ~19°N latitude.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}