{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:XD37LNAMSRGS2MBB2OQSW654VL","short_pith_number":"pith:XD37LNAM","schema_version":"1.0","canonical_sha256":"b8f7f5b40c944d2d3021d3a12b7bbcaafda443fda960b281501bc781a6422845","source":{"kind":"arxiv","id":"1212.6120","version":1},"attestation_state":"computed","paper":{"title":"Monitoring the photometric behavior of OmegaCAM with Astro-WISE","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Danny R. Boxhoorn, Edwin A. Valentijn, Erik R. Deul, Ewout M. Helmich, Gijs A. Verdoes Kleijn, Konrad H. Kuijken, Kor G. Begeman, Roeland Rengelink","submitted_at":"2012-12-26T06:16:18Z","abstract_excerpt":"The OmegaCAM wide-field optical imager is the sole instrument on the VLT Survey Telescope at ESO's Paranal Observatory. The instrument, as well as the telescope, have been designed for surveys with very good, natural seeing-limited image quality over a 1 square degree field. OmegaCAM was commissioned in 2011 and has been observing three ESO Public Surveys in parallel since October 15, 2011. We use the Astro-WISE information system to monitor the calibration of the observatory and to produce the Kilo Degree Survey (KiDS).\n  Here we describe the photometric monitoring procedures in Astro-WISE an"},"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":"1212.6120","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2012-12-26T06:16:18Z","cross_cats_sorted":[],"title_canon_sha256":"2428e37382b05e0061727c787c5e535ddb5ddbf3f47e47c19a60485066b4aaf0","abstract_canon_sha256":"8b5abe73e5dede579cd7ed606b6e70f7c2c6574255eb1728edfda2f738ce8d1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:27.461239Z","signature_b64":"HVjtQBDle6QQ28Gg1oii1GNqo1zCNwhMv/kHYM1vZKsAX4s4XNbk5F7gwgOKzXsk9tCtobsyMuaSxARY8UGZCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b8f7f5b40c944d2d3021d3a12b7bbcaafda443fda960b281501bc781a6422845","last_reissued_at":"2026-05-18T01:52:27.460818Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:27.460818Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Monitoring the photometric behavior of OmegaCAM with Astro-WISE","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Danny R. Boxhoorn, Edwin A. Valentijn, Erik R. Deul, Ewout M. Helmich, Gijs A. Verdoes Kleijn, Konrad H. Kuijken, Kor G. Begeman, Roeland Rengelink","submitted_at":"2012-12-26T06:16:18Z","abstract_excerpt":"The OmegaCAM wide-field optical imager is the sole instrument on the VLT Survey Telescope at ESO's Paranal Observatory. The instrument, as well as the telescope, have been designed for surveys with very good, natural seeing-limited image quality over a 1 square degree field. OmegaCAM was commissioned in 2011 and has been observing three ESO Public Surveys in parallel since October 15, 2011. We use the Astro-WISE information system to monitor the calibration of the observatory and to produce the Kilo Degree Survey (KiDS).\n  Here we describe the photometric monitoring procedures in Astro-WISE an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1212.6120","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":"1212.6120","created_at":"2026-05-18T01:52:27.460877+00:00"},{"alias_kind":"arxiv_version","alias_value":"1212.6120v1","created_at":"2026-05-18T01:52:27.460877+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1212.6120","created_at":"2026-05-18T01:52:27.460877+00:00"},{"alias_kind":"pith_short_12","alias_value":"XD37LNAMSRGS","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_16","alias_value":"XD37LNAMSRGS2MBB","created_at":"2026-05-18T12:27:27.928770+00:00"},{"alias_kind":"pith_short_8","alias_value":"XD37LNAM","created_at":"2026-05-18T12:27:27.928770+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/XD37LNAMSRGS2MBB2OQSW654VL","json":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL.json","graph_json":"https://pith.science/api/pith-number/XD37LNAMSRGS2MBB2OQSW654VL/graph.json","events_json":"https://pith.science/api/pith-number/XD37LNAMSRGS2MBB2OQSW654VL/events.json","paper":"https://pith.science/paper/XD37LNAM"},"agent_actions":{"view_html":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL","download_json":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL.json","view_paper":"https://pith.science/paper/XD37LNAM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1212.6120&json=true","fetch_graph":"https://pith.science/api/pith-number/XD37LNAMSRGS2MBB2OQSW654VL/graph.json","fetch_events":"https://pith.science/api/pith-number/XD37LNAMSRGS2MBB2OQSW654VL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL/action/storage_attestation","attest_author":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL/action/author_attestation","sign_citation":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL/action/citation_signature","submit_replication":"https://pith.science/pith/XD37LNAMSRGS2MBB2OQSW654VL/action/replication_record"}},"created_at":"2026-05-18T01:52:27.460877+00:00","updated_at":"2026-05-18T01:52:27.460877+00:00"}