{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:GRH44OOXD5T6FJ3C3AT6JF44WK","short_pith_number":"pith:GRH44OOX","schema_version":"1.0","canonical_sha256":"344fce39d71f67e2a762d827e4979cb2bf4d79382db0bce229ad8955024007c3","source":{"kind":"arxiv","id":"1205.3828","version":1},"attestation_state":"computed","paper":{"title":"The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Eigenbrot, A. Saha, A. Schechtman-Rook, A. Weyant, B. Simmons, D. Harbeck, D. R. Silva, D. Summers, D. Williams, E. Manne-Nicholas, E. M. Wilcots, E. P. Horch, G. Will, H. Herbst, H. Schweiker, J. D. Simon, J. F. Kaczmarek, J. J. Adams, J. Power, J. Rajagopal, J. R. Hargis, J. S. Gallagher, K. Butler, K. L. Rhode, K. Milliman, K. Reetz, L. E. Allen, M. A. Bershady, M. A. Camarata, M. C. Bentz, M. D. Young, M. E. Schwamb, M. Everett, M. Meixner, P. Knezek, P. M. Garnavich E. Glikman, R. D. Mathieu, R. E. Anderson, R. R. Joyce, S. B. Howell, S. Jha, T. L. Beck, T. Matheson, W. M. Wood-Vasey, W. S. Binkert","submitted_at":"2012-05-16T23:07:06Z","abstract_excerpt":"We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera (WHIRC). When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 \\pm 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1205.3828","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-05-16T23:07:06Z","cross_cats_sorted":[],"title_canon_sha256":"7978dfb54791649fd2726d40026fb595e6f2b41790b820ecb8026c2c2b7ac223","abstract_canon_sha256":"60d294f3962ad72cb917f98bde27df071d241e83e78358ffc1410fbab2238421"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:31.038360Z","signature_b64":"yetbAwzlkXpI81hS3lljU5lFLI/aqEd5a9UFCmlFsxETzQT4LypHzqqF/rutHpx0rD8R2c3y3EQe20BG+WQdAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"344fce39d71f67e2a762d827e4979cb2bf4d79382db0bce229ad8955024007c3","last_reissued_at":"2026-05-18T01:57:31.037782Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:31.037782Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Eigenbrot, A. Saha, A. Schechtman-Rook, A. Weyant, B. Simmons, D. Harbeck, D. R. Silva, D. Summers, D. Williams, E. Manne-Nicholas, E. M. Wilcots, E. P. Horch, G. Will, H. Herbst, H. Schweiker, J. D. Simon, J. F. Kaczmarek, J. J. Adams, J. Power, J. Rajagopal, J. R. Hargis, J. S. Gallagher, K. Butler, K. L. Rhode, K. Milliman, K. Reetz, L. E. Allen, M. A. Bershady, M. A. Camarata, M. C. Bentz, M. D. Young, M. E. Schwamb, M. Everett, M. Meixner, P. Knezek, P. M. Garnavich E. Glikman, R. D. Mathieu, R. E. Anderson, R. R. Joyce, S. B. Howell, S. Jha, T. L. Beck, T. Matheson, W. M. Wood-Vasey, W. S. Binkert","submitted_at":"2012-05-16T23:07:06Z","abstract_excerpt":"We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera (WHIRC). When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 \\pm 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.3828","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":""},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1205.3828","created_at":"2026-05-18T01:57:31.037880+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.3828v1","created_at":"2026-05-18T01:57:31.037880+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.3828","created_at":"2026-05-18T01:57:31.037880+00:00"},{"alias_kind":"pith_short_12","alias_value":"GRH44OOXD5T6","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_16","alias_value":"GRH44OOXD5T6FJ3C","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_8","alias_value":"GRH44OOX","created_at":"2026-05-18T12:27:06.952714+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK","json":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK.json","graph_json":"https://pith.science/api/pith-number/GRH44OOXD5T6FJ3C3AT6JF44WK/graph.json","events_json":"https://pith.science/api/pith-number/GRH44OOXD5T6FJ3C3AT6JF44WK/events.json","paper":"https://pith.science/paper/GRH44OOX"},"agent_actions":{"view_html":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK","download_json":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK.json","view_paper":"https://pith.science/paper/GRH44OOX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.3828&json=true","fetch_graph":"https://pith.science/api/pith-number/GRH44OOXD5T6FJ3C3AT6JF44WK/graph.json","fetch_events":"https://pith.science/api/pith-number/GRH44OOXD5T6FJ3C3AT6JF44WK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK/action/storage_attestation","attest_author":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK/action/author_attestation","sign_citation":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK/action/citation_signature","submit_replication":"https://pith.science/pith/GRH44OOXD5T6FJ3C3AT6JF44WK/action/replication_record"}},"created_at":"2026-05-18T01:57:31.037880+00:00","updated_at":"2026-05-18T01:57:31.037880+00:00"}