{"total":18,"items":[{"citing_arxiv_id":"2605.11703","ref_index":115,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors","primary_cat":"gr-qc","submitted_at":"2026-05-12T07:58:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"The first informative astrophysical calibration of gravitational-wave detectors is reported using GW240925 and GW250207.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"laboration, KAGRA Collaboration), Tests of General Rel- ativity with GWTC-3, Phys. Rev. D112, 084080 (2025), arXiv:2112.06861 [gr-qc]. [114] N. K. Johnson-McDaniel, A. Ghosh, S. Ghonge, M. Saleem, N. V . Krishnendu, and J. A. Clark, Investigating the relation between gravitational wave tests of general relativity, Phys. Rev. D105, 044020 (2022), arXiv:2109.06988 [gr-qc]. [115] A. G. Abacet al.(LIGO Scientific Collaboration, Virgo Col- laboration, KAGRA Collaboration), GWTC-4.0: Tests of General Relativity. I. Overview and General Tests, arXiv e- prints (2026), arXiv:2603.19019 [gr-qc]. [116] A. K. Mehta, A. Buonanno, R. Cotesta, A. Ghosh, N. Sennett, and J. Steinhoff, Tests of general relativity with gravitational-wave observations using a flexible theory-"},{"citing_arxiv_id":"2605.04224","ref_index":7,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Black-Hole Scattering in Einstein-scalar-Gauss-Bonnet: Numerical Relativity Meets Analytics","primary_cat":"gr-qc","submitted_at":"2026-05-05T19:08:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Numerical relativity simulations of black hole scattering in Einstein-scalar-Gauss-Bonnet gravity agree closely with effective-one-body analytic predictions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03576","ref_index":10,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Ringdown Analysis of GW250114 with Orthonormal 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Quant. Grav.32, 024001 (2015), arXiv:1408.3978 [gr-qc]. [4] T. Akutsuet al.(KAGRA), Nature Astron.3, 35 (2019), arXiv:1811.08079 [gr-qc]. [5] A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), (2025), arXiv:2508.18083 [astro-ph.HE]. [6] A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), (2025), arXiv:2509.04348 [astro-ph.CO]. [7] A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), (2026), arXiv:2603.19019 [gr-qc]. [8] A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), (2026), arXiv:2603.19020 [gr-qc]. [9] A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), (2026), arXiv:2603.19021 [gr-qc]. [10] C. V. Vishveshwara, Phys. Rev. D1, 2870 (1970). [11] W. H. Press, Astrophys. J. Lett.170, L105 (1971)."},{"citing_arxiv_id":"2604.13687","ref_index":15,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"VIGILant: an automatic classification pipeline for glitches in the Virgo detector","primary_cat":"gr-qc","submitted_at":"2026-04-15T10:09:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"VIGILant applies tree-based models and a ResNet CNN to classify Virgo O3b glitches with 98% accuracy and has been deployed for daily use with an interactive dashboard.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.11895","ref_index":14,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Novel ringdown tests of general relativity with black hole greybody factors","primary_cat":"gr-qc","submitted_at":"2026-04-13T18:00:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"GreyRing model based on greybody factors reproduces numerical relativity ringdown signals with mismatches of order 10^{-6} and enables a new post-merger consistency test of general relativity applied to GW250114.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.11755","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Ringing of rapidly rotating black holes in effective field theory","primary_cat":"gr-qc","submitted_at":"2026-04-13T17:28:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Leading-order cubic-curvature corrections to scalar quasinormal modes of black holes with spins up to 0.99M are computed numerically for modes up to l=5 with relative errors below 10^{-4}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.09828","ref_index":37,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Testing the Kerr hypothesis beyond the quadrupole with GW241011","primary_cat":"gr-qc","submitted_at":"2026-04-10T18:58:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"GW241011 data shows consistency with Kerr black holes for both quadrupole and octupole moments and delivers the first observational bounds on spin-induced octupole deviations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.08680","ref_index":19,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Prompt Response from Plunging Sources in Schwarzschild Spacetime","primary_cat":"gr-qc","submitted_at":"2026-04-09T18:12:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The prompt response is ~1.2 times stronger than quasinormal mode excitation during inspiral and enables 99% accurate reconstruction of the full inspiral-merger-ringdown waveform when combined with other components.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.02214","ref_index":11,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Quadratic gravity corrections to scalar QNMs of rapidly rotating black holes","primary_cat":"gr-qc","submitted_at":"2026-04-02T16:06:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Leading-order deviations from general relativity in scalar quasinormal modes of rotating black holes are computed numerically up to dimensionless spins of 0.99 in quadratic-curvature scalar-tensor theories.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}