{"total":10,"items":[{"citing_arxiv_id":"2606.26223","ref_index":124,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T18:00:01+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":"2605.21436","ref_index":259,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum","primary_cat":"astro-ph.CO","submitted_at":"2026-05-20T17:26:36+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Validates redshift-space power spectrum and bispectrum analysis on Abacus-PNG mocks to recover unbiased f_NL constraints for Euclid spectroscopic sample.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13543","ref_index":124,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"UNIONS-3500 Weak Lensing: IV. 2D cosmological constraints in harmonic space","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T13:53:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"UNIONS r-band data constrains S8 to 0.891^{+0.057}_{-0.084} via 2D harmonic-space cosmic shear, consistent with Planck at 0.79 sigma after modeling baryonic feedback and intrinsic alignments.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.18111","ref_index":16,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Smokescreen: A Python package for data vector blinding and encryption in cosmological analyses","primary_cat":"astro-ph.IM","submitted_at":"2026-04-20T11:27:42+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Smokescreen is a Python package that blinds cosmological data vectors using Firecrown likelihoods on SACC files while encrypting the true data to avoid premature unblinding.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.11041","ref_index":121,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature","primary_cat":"astro-ph.CO","submitted_at":"2025-12-11T19:00:39+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"KiDS-Legacy cosmic shear plus external probes yields S8 = 0.816 ± 0.006 in Lambda-CDM and consistent bounds on w0, wa, sum m_nu and Omega_K with no strong preference for extensions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.18749","ref_index":50,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Symbolic Emulators for Cosmology: Accelerating Cosmological Analyses Without Sacrificing Precision","primary_cat":"astro-ph.CO","submitted_at":"2025-10-21T15:57:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Symbolic emulators approximate key Lambda CDM functions to 0.001-0.05% accuracy across relevant redshifts and Omega_m values, enabling faster 3x2pt inference with consistent results.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.00758","ref_index":10,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Dimensional reduction for sampled priors and application to photometric redshift distributions","primary_cat":"astro-ph.IM","submitted_at":"2025-06-01T00:09:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A modified PCA method compresses sampled nuisance priors in Bayesian inference by projecting out likelihood-insensitive modes, applied to photometric redshift distributions for DES weak lensing and galaxy clustering analyses.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2410.22272","ref_index":77,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Dark Energy Survey Year 3: Blue Shear","primary_cat":"astro-ph.CO","submitted_at":"2024-10-29T17:28:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Blue galaxy selection in DES Y3 cosmic shear mitigates IA effects, producing stable parameters with 1.5x smaller S8 uncertainty and improved CMB agreement versus the full sample.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2304.05203","ref_index":169,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters","primary_cat":"astro-ph.CO","submitted_at":"2023-04-11T13:13:14+00:00","verdict":"ACCEPT","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"ACT DR6 CMB lensing map gives σ8 = 0.819 ± 0.015 and H0 = 68.3 ± 1.1 km/s/Mpc, consistent with Planck ΛCDM but 1.7-2.1σ higher in S8 than KiDS, DES, and HSC galaxy surveys.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2202.04077","ref_index":224,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Pantheon+ Analysis: 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