{"paper":{"title":"Optical and near-infrared photometry of 94 type II supernovae from the Carnegie Supernova Project","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Goobar, A.L. Piro, A.V. Filippenko, B.J. Shappee, B. Madore, C. Ashall, C. Baltay, C. Contreras, C. Gall, C. Gonzalez, C.P. Gutierrez, C.R. Burns, D. DePoy, E. Baron, E. Hadjiyska, E.Y. Hsiao, F. Forster, F. Taddia, G. Folatelli, J. Anais, J. Marshall, J.P. Anderson, J-P. Rheault, J. Seron, J. Thomas-Osip, K. Krisciunas, L. Busta, L. Galbany, L. Martinez, M. Bersten, M.D. Stritzinger, M. Hamuy, M.M. Phillips, N.B. Suntzeff, N. Morrell, P. Hoeflich, P.J. Pessi, P. Nugent, S. Castellon, S. Gonzalez-Gaitan, S. Ryder, S. Torres, s. Uddin, T. de Jaeger, W. Krzeminski, W. Li","submitted_at":"2024-10-09T10:18:28Z","abstract_excerpt":"Type II supernovae (SNeII) mark the endpoint in the lives of hydrogen-rich massive stars. Their large explosion energies and luminosities allow us to measure distances, metallicities, and star formation rates into the distant Universe. To fully exploit their use in answering different astrophysical problems, high-quality low-redshift data sets are required. Such samples are vital to understand the physics of SNeII, but also to serve as calibrators for distinct - and often lower-quality - samples. We present uBgVri optical and YJH near-infrared (NIR) photometry for 94 low-redshift SNeII observe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.06738","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2410.06738/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}