{"total":15,"items":[{"citing_arxiv_id":"2606.10674","ref_index":33,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Comprehensive Study on the Line Profiles and Stark Widths of Ionic Transitions from Laser Produced Aluminum Plasma","primary_cat":"physics.plasm-ph","submitted_at":"2026-06-09T10:27:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The study creates a self-consistent Stark broadening database for Al II lines in laser-produced aluminum plasma by referencing Al III widths measured under identical conditions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06433","ref_index":28,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Depolarization and Polarization-Transfer Rates for Solar He I Lines due to Collisions with Neutral Hydrogen","primary_cat":"astro-ph.SR","submitted_at":"2026-06-04T17:36:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Computes multi-level and multi-term collisional rates for He I fine-structure levels and terms in the 10830 Å, D3 5876 Å, and related triplet lines using the frozen-core approximation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04793","ref_index":37,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines","primary_cat":"astro-ph.GA","submitted_at":"2026-06-03T12:19:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Multiphase CGM absorption in DESI data shows cooler ions (Ca II, Mg II) have steeper radial W profiles than C IV, with galaxy vs. quasar differences, consistent with simulations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.20360","ref_index":19,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Highly Variable Wind from WD J005311, the Stellar Remnant of the Peculiar Galactic Supernova of 1181","primary_cat":"astro-ph.SR","submitted_at":"2026-05-19T18:13:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Time-resolved spectroscopy reveals broad and narrow LPVs in O VI from WD J005311, linked to line-driven wind instabilities and an unstable RRM disk, plus a pseudo-periodic UV oscillation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15263","ref_index":258,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"On the quenching of LRD X-ray emission by both Compton-thick gas and high accretion rates","primary_cat":"astro-ph.GA","submitted_at":"2026-05-14T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LRDs require Compton-thick gas at moderate metallicity plus high accretion rates producing weak X-rays to explain their non-detection, implying they are not chemically pristine.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.11278","ref_index":37,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Detection of Gravitons by Measuring Excess of Photon Luminosities from Interstellar and Intergalactic Hydrogen","primary_cat":"hep-ph","submitted_at":"2026-05-11T22:02:11+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"graviton absorption wave lengths are in the UV region 91.1nm≤λg≤102.5nmand are very well overlapped with the spectrum of the graviton radiation of stars 1.88nm < λ⊙ g <1884nm (4.54). The spontaneous radiation of the Lyman UV photons is in the wave lengths spectrum 91.2nm≤λL ≤121.6nmand of the Balmer photons is in the wave lengths of the visible spectrum 364.6nm≤λB≤656.2nm[37]. The mean value of the hydrogen radius on the levelndis ¯r=3 2(n2−2)a.(3.42) This radius should be smaller than the mean distancedbetween hydrogen atoms in the interstellar gas and the maximal energy level available for the graviton absorption is defined by the condition ¯r∼d: nmax∼ √ 2d 3a.(3.43) In a typical spiral galaxyd≈1cm, and we will haven max≈108."},{"citing_arxiv_id":"2605.05100","ref_index":25,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Hyperfine-structure constants of the $^{45}\\!$Sc II ion and the nuclear quadrupole moment","primary_cat":"physics.atom-ph","submitted_at":"2026-05-06T16:36:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Relativistic CI+CCSD calculations of hyperfine constants in 45Sc+ yield nuclear quadrupole moment Q = 0.222(2) b consistent with molecular data.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"Table II lists the ionization energies of 58 states arising from the3d4s,3d 2,4s 2,4s4p,3d4p,3d5s,3d4d, and3d5p configurations of the Sc II ion. These energies are ob- tained by using CI+MBPT(2), CI+LCCSD, CI+CCSD, CI+LCCSDs and CI+CCSDs methods, respectively. We alsocompareourcalculatedresultswiththeexperimental valuesfromtheNationalInstituteofStandardsandTech- nology (NIST) [25]. For convenience, the CI+MBPT(2), CI+LCCSD, CI+CCSD, CI+LCCSDs and CI+CCSDs methods are denoted asM 1,M 2,M 3,M 4, andM 5 re- spectively. The symbol∆ n represents the absolute dif- ference between the theoretical results obtained by the Mn method and the experimental values, i.e.,∆ n = |EMn −E NIST|. As seen, CI+MBPT(2) method yields the largest mean deviation, 2380 cm−1; CI+LCCSD re-"},{"citing_arxiv_id":"2605.02929","ref_index":47,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Electron-impact ionization rates for neutral He, Li, and Be in the Tsallis framework","primary_cat":"physics.gen-ph","submitted_at":"2026-04-27T16:25:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"A sensitivity study shows Tsallis q-distributions alter ionization rates for He, Li, and Be, with q<1 suppressing and q>1 enhancing low-temperature rates, while separating cross-section and EEDF uncertainties and releasing the code.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.21374","ref_index":47,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Revisiting the luminescence properties of Pr3+: YAG within the framework of an extended approach of Judd-Ofelt theory","primary_cat":"physics.atom-ph","submitted_at":"2026-04-23T07:41:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"An extended Judd-Ofelt model yields better calculated absorption intensities for Pr3+:YAG, especially the hypersensitive transition, and identifies additional viable laser wavelengths at 566 nm and 931 nm.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.09399","ref_index":32,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Paschen Jumps in Little Red Dots: Evidence for Nebular Continua","primary_cat":"astro-ph.GA","submitted_at":"2026-04-10T15:13:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Paschen jumps in Little Red Dots indicate their continua originate from free-bound recombination emission in low-temperature nebular gas rather than thermalized or AGN components.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.05812","ref_index":47,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Strontium and helium in the kilonova AT2017gfo: Origin of the 1{\\mu}m feature constrained via NLTE calculations","primary_cat":"astro-ph.HE","submitted_at":"2026-04-07T12:49:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"NLTE calculations indicate strontium is required to explain the onset of the 1μm feature at early times in AT2017gfo, while helium can dominate at later epochs with plausible masses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.20460","ref_index":38,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLAS","primary_cat":"astro-ph.EP","submitted_at":"2026-03-20T19:40:35+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":"2603.15273","ref_index":12,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Design and operation of a flash lamp for vacuum ultraviolet light production","primary_cat":"physics.ins-det","submitted_at":"2026-03-16T13:38:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"A room-temperature flash lamp prototype is presented for generating VUV light at wavelengths matching noble liquid scintillators to test light sensors.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.08668","ref_index":10,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Atomic and molecular systems for radiation thermometry","primary_cat":"physics.atom-ph","submitted_at":"2025-12-09T14:52:28+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Atomic systems using 85Rb Rydberg atoms and vapor provide primary measurements of blackbody radiation temperature near 130 GHz and 24.5 THz with uncertainties of 1% and 0.13 K respectively.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"1906.08281","ref_index":51,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Non-LTE analysis of K I in late-type stars","primary_cat":"astro-ph.SR","submitted_at":"2019-06-19T18:04:02+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Non-LTE effects strengthen the K I 7698 Å line, requiring abundance corrections up to -0.7 dex that align literature values with GCE models incorporating yields from rotating massive stars.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}