{"total":10,"items":[{"citing_arxiv_id":"2606.30144","ref_index":3,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation","primary_cat":"astro-ph.HE","submitted_at":"2026-06-29T11:21:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Joint strong-lensing and population inference on resolved gravitational-wave events finds no lensed events and tightens constraints on the black-hole merger rate peak redshift and high-redshift tail.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06609","ref_index":178,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JWST absorption line spectroscopy with SPURS: ISM covering fractions and kinematics in individual galaxies at $z=5-9$","primary_cat":"astro-ph.GA","submitted_at":"2026-06-04T18:01:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"JWST spectra of six z=5-9 galaxies show low-ionization covering fractions of 0.2-0.9 and diverse kinematics including blueshifted outflows, indicating heterogeneous multiphase ISM.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.28658","ref_index":27,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks","primary_cat":"astro-ph.CO","submitted_at":"2026-05-27T15:57:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations indicate joint Taiji+LISA analysis of five SLGW events yields H0 95% credible interval uncertainties of 0.11 (source redshift unknown) or 0.042 (source redshift known).","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.27499","ref_index":78,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"GenSBI: Generative Methods for Simulation-Based Inference in JAX","primary_cat":"cs.LG","submitted_at":"2026-05-26T17:59:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"GenSBI delivers JAX-native implementations of generative SBI methods with transformer backbones and reports near-ideal calibration scores on standard benchmarks.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21212","ref_index":81,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Detection of a dark matter subhalo in the strongly lensed system PJ011646","primary_cat":"astro-ph.GA","submitted_at":"2026-05-20T14:07:43+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A subhalo of M200 = 2.78e10 solar masses and concentration 30 is detected at 5.8 sigma in PJ011646 via ALMA imaging and grid-based NFW search after fitting an elliptical power-law plus multipole macromodel.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18097","ref_index":43,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Effects of formation channels and gravitational lensing on stochastic gravitational wave background","primary_cat":"gr-qc","submitted_at":"2026-05-18T09:11:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Using HBI on GWTC-4 data the authors compute lensed SGWBs for ABHs and PBHs and conclude that LIGO and ET can distinguish the two formation channels in specific frequency ranges, with ET offering broader coverage.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15078","ref_index":133,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions","primary_cat":"astro-ph.CO","submitted_at":"2026-05-14T17:02:28+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Bayesian hierarchical modeling of photometric redshifts in KiDS+VIKING-450 raises S8 to 0.756 ± 0.039 and reduces Planck tension to 1.9σ.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.13223","ref_index":64,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Observational constraints on nonlocal black holes via gravitational lensing","primary_cat":"gr-qc","submitted_at":"2026-04-14T18:48:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Nonlocal black holes remain consistent with general relativity at the 1.13-sigma level after joint lensing and quasinormal-mode constraints.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Keeton and A. O. Petters, Phys. Rev. D72, 104006 (2005), arXiv:gr-qc/0511019. [61] L. Amendola, M. Kunz, and D. Sapone, JCAP04, 013 (2008), arXiv:0704.2421 [astro-ph]. [62] G. Crisnejo and E. Gallo, Phys. Rev. D97, 124016 (2018), arXiv:1804.05473 [gr-qc]. [63] G. Crisnejo, E. Gallo, and K. Jusufi, Phys. Rev. D100, 104045 (2019), arXiv:1910.02030 [gr-qc]. [64] T. Treu, Ann. Rev. Astron. Astrophys.48, 87 (2010), arXiv:1003.5567 [astro-ph.CO]. [65] P. V. P. Cunha and C. A. R. Herdeiro, Gen. Rel. Grav. 50, 42 (2018), arXiv:1801.00860 [gr-qc]. 10 [66] V. Bozza, Phys. Rev. D66, 103001 (2002), arXiv:gr- qc/0208075. [67] V. Cardoso, A. S. Miranda, E. Berti, H. Witek, and V. T. Zanchin, Phys. Rev. D79, 064016 (2009),"},{"citing_arxiv_id":"2510.07511","ref_index":54,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys","primary_cat":"astro-ph.GA","submitted_at":"2025-10-08T20:18:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A method using Balrog synthetic injections corrects spatially variable detection and classification rates in DES Y3 data, reducing relative detection rate standard deviation by a factor of five and lowering bias in stellar stream density power spectra.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2411.07970","ref_index":166,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"MUltiplexed Survey Telescope (MUST) Science White Paper I: Overview of Large-Scale Structure Cosmology in the Era of Stage-V Spectroscopic Surveys","primary_cat":"astro-ph.CO","submitted_at":"2024-11-12T17:51:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"MUST is a planned 6.5m Stage-V spectroscopic survey telescope targeting 100M+ galaxies and quasars to z~5.5 for large-scale structure cosmology studies.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"the spectroscopic data of galaxies in color space, thereby ex- panding the training set for calibrating photometric or slitless spectroscopic redshift measurements (e.g., [31, 165]). The high efficiency and large survey volume of MUST offers op- portunities to identify or confirm strong lensing systems, e.g., low-zbright galaxies with anomalously high-zemission lines [166]. Moreover, the cross-correlation between imaging data and Lyαforests from MUST may enable tracing LSS using Lyαintensity mapping [167]. 3.6.2 CMB S4 The next generation of CMB experiments, such as AliCPT [168], Simons Observatory [169], CMB-S4 [170], LiteBIRD [171], and PICO [172], holds significant promise for detect- ing primordial gravitational waves from the early-universe"}],"limit":50,"offset":0}