{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:LUOSY23EIL5RUGKTS357MX6Q3K","short_pith_number":"pith:LUOSY23E","schema_version":"1.0","canonical_sha256":"5d1d2c6b6442fb1a195396fbf65fd0da9bf3dfe87a1079cf79ba0014474894ab","source":{"kind":"arxiv","id":"1303.3634","version":1},"attestation_state":"computed","paper":{"title":"The Pan-STARRS 1 Photometric Reference Ladder, Release 12.0","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"C. W. Stubbs, D. Finkbeiner, E. A. Magnier, E. Schlafly, H. A. Flewelling, J. L. Tonry, J. S. Morgan, K. C. Chambers, M. Juric, N. Kaiser, P. A. Price, R.-P. Kudritzki, W. E. Sweeney, W. S. Burgett","submitted_at":"2013-03-14T22:45:49Z","abstract_excerpt":"As of 2012 Jan 21, the Pan-STARRS 1 3\\pi Survey has observed the 3/4 of the sky visible from Hawaii with a minimum of 2 and mean of 7.6 observations in 5 filters, g_p1, r_p1, i_p1, z_p1, y_p1. Now at the end of the second year of the mission, we are in a position to make an initial public release of a portion of this unprecedented dataset. This article describes the PS1 Photometric Ladder, Release 12.01 This is the first of a series of data releases to be generated as the survey coverage increases and the data analysis improves. The Photometric Ladder has rungs every hour in RA and at 4 interv"},"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":"1303.3634","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2013-03-14T22:45:49Z","cross_cats_sorted":[],"title_canon_sha256":"630e61fe8f04f48f0900876ed71a07e3dbbb05fe73c115cb0b5762a52fc16af5","abstract_canon_sha256":"20497c05e9194b1b4d0387e074697d8cfed00a25ff6de582a625c0f26d90cf3f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:07.030907Z","signature_b64":"V/kXtU8ZmEjiaTyix+1IxP5WP3HkdgJS/ZapnQOc8uSAU8FbAFQ/DoamUbShCoDd0+/hDBhZVreBpok7/Nw/Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d1d2c6b6442fb1a195396fbf65fd0da9bf3dfe87a1079cf79ba0014474894ab","last_reissued_at":"2026-05-18T01:51:07.030304Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:07.030304Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Pan-STARRS 1 Photometric Reference Ladder, Release 12.0","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"C. W. Stubbs, D. Finkbeiner, E. A. Magnier, E. Schlafly, H. A. Flewelling, J. L. Tonry, J. S. Morgan, K. C. Chambers, M. Juric, N. Kaiser, P. A. Price, R.-P. Kudritzki, W. E. Sweeney, W. S. Burgett","submitted_at":"2013-03-14T22:45:49Z","abstract_excerpt":"As of 2012 Jan 21, the Pan-STARRS 1 3\\pi Survey has observed the 3/4 of the sky visible from Hawaii with a minimum of 2 and mean of 7.6 observations in 5 filters, g_p1, r_p1, i_p1, z_p1, y_p1. Now at the end of the second year of the mission, we are in a position to make an initial public release of a portion of this unprecedented dataset. This article describes the PS1 Photometric Ladder, Release 12.01 This is the first of a series of data releases to be generated as the survey coverage increases and the data analysis improves. The Photometric Ladder has rungs every hour in RA and at 4 interv"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.3634","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":"1303.3634","created_at":"2026-05-18T01:51:07.030400+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.3634v1","created_at":"2026-05-18T01:51:07.030400+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.3634","created_at":"2026-05-18T01:51:07.030400+00:00"},{"alias_kind":"pith_short_12","alias_value":"LUOSY23EIL5R","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"LUOSY23EIL5RUGKT","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"LUOSY23E","created_at":"2026-05-18T12:27:51.066281+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.19413","citing_title":"Gaia21bja: pre-main sequence star with quasi-periodic bursts","ref_index":11,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13842","citing_title":"From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K","json":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K.json","graph_json":"https://pith.science/api/pith-number/LUOSY23EIL5RUGKTS357MX6Q3K/graph.json","events_json":"https://pith.science/api/pith-number/LUOSY23EIL5RUGKTS357MX6Q3K/events.json","paper":"https://pith.science/paper/LUOSY23E"},"agent_actions":{"view_html":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K","download_json":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K.json","view_paper":"https://pith.science/paper/LUOSY23E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.3634&json=true","fetch_graph":"https://pith.science/api/pith-number/LUOSY23EIL5RUGKTS357MX6Q3K/graph.json","fetch_events":"https://pith.science/api/pith-number/LUOSY23EIL5RUGKTS357MX6Q3K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K/action/storage_attestation","attest_author":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K/action/author_attestation","sign_citation":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K/action/citation_signature","submit_replication":"https://pith.science/pith/LUOSY23EIL5RUGKTS357MX6Q3K/action/replication_record"}},"created_at":"2026-05-18T01:51:07.030400+00:00","updated_at":"2026-05-18T01:51:07.030400+00:00"}