{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:754W6RMRE4TVPXL66725FLFNA3","short_pith_number":"pith:754W6RMR","schema_version":"1.0","canonical_sha256":"ff796f4591272757dd7ef7f5d2acad06eabb0473aaf3d9e95e29cef930edf019","source":{"kind":"arxiv","id":"1001.0261","version":1},"attestation_state":"computed","paper":{"title":"The Inclination of the Soft X-ray Transient A0620--00 and the Mass of its Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew G. Cantrell, Charles D. Bailyn, Cynthia S. Froning, Dawn M. Gelino, Jeffrey E. McClintock, Jerome A. Orosz, Joseph Neilsen, Lijun Gou, Ronald A. Remillard","submitted_at":"2010-01-01T21:38:20Z","abstract_excerpt":"We analyze photometry of the Soft X-ray Transient A0620-00 spanning nearly 30 years, including previously published and previously unpublished data. Previous attempts to determine the inclination of A0620 using subsets of these data have yielded a wide range of measured values of i. Differences in the measured value of i have been due to changes in the shape of the light curve and uncertainty regarding the contamination from the disk. We give a new technique for estimating the disk fraction and find that disk light is significant in all light curves, even in the infrared. We also find that all"},"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":"1001.0261","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-01-01T21:38:20Z","cross_cats_sorted":[],"title_canon_sha256":"0e52fe4d969739cbea43addacc25b91acfc319c38af4e31754777663524616a0","abstract_canon_sha256":"11b8bce969031c2af3bce751b725fdcd7e2eafcbe18e842a93649b54a165d08c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:10:05.811711Z","signature_b64":"bUhrANyKIAc1N945xFemo4x4Z7m4TVtp+hkbFBV4YT0pM/EKWuLAoIJbMiDlvcE5ufyoj44g5qnTW9KUyJvEBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ff796f4591272757dd7ef7f5d2acad06eabb0473aaf3d9e95e29cef930edf019","last_reissued_at":"2026-05-18T02:10:05.810959Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:10:05.810959Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Inclination of the Soft X-ray Transient A0620--00 and the Mass of its Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew G. Cantrell, Charles D. Bailyn, Cynthia S. Froning, Dawn M. Gelino, Jeffrey E. McClintock, Jerome A. Orosz, Joseph Neilsen, Lijun Gou, Ronald A. Remillard","submitted_at":"2010-01-01T21:38:20Z","abstract_excerpt":"We analyze photometry of the Soft X-ray Transient A0620-00 spanning nearly 30 years, including previously published and previously unpublished data. Previous attempts to determine the inclination of A0620 using subsets of these data have yielded a wide range of measured values of i. Differences in the measured value of i have been due to changes in the shape of the light curve and uncertainty regarding the contamination from the disk. We give a new technique for estimating the disk fraction and find that disk light is significant in all light curves, even in the infrared. We also find that all"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1001.0261","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":"1001.0261","created_at":"2026-05-18T02:10:05.811079+00:00"},{"alias_kind":"arxiv_version","alias_value":"1001.0261v1","created_at":"2026-05-18T02:10:05.811079+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1001.0261","created_at":"2026-05-18T02:10:05.811079+00:00"},{"alias_kind":"pith_short_12","alias_value":"754W6RMRE4TV","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"754W6RMRE4TVPXL6","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"754W6RMR","created_at":"2026-05-18T12:26:04.259169+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/754W6RMRE4TVPXL66725FLFNA3","json":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3.json","graph_json":"https://pith.science/api/pith-number/754W6RMRE4TVPXL66725FLFNA3/graph.json","events_json":"https://pith.science/api/pith-number/754W6RMRE4TVPXL66725FLFNA3/events.json","paper":"https://pith.science/paper/754W6RMR"},"agent_actions":{"view_html":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3","download_json":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3.json","view_paper":"https://pith.science/paper/754W6RMR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1001.0261&json=true","fetch_graph":"https://pith.science/api/pith-number/754W6RMRE4TVPXL66725FLFNA3/graph.json","fetch_events":"https://pith.science/api/pith-number/754W6RMRE4TVPXL66725FLFNA3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3/action/storage_attestation","attest_author":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3/action/author_attestation","sign_citation":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3/action/citation_signature","submit_replication":"https://pith.science/pith/754W6RMRE4TVPXL66725FLFNA3/action/replication_record"}},"created_at":"2026-05-18T02:10:05.811079+00:00","updated_at":"2026-05-18T02:10:05.811079+00:00"}