{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:D35K2P4QWPGND62D77MJA66SEN","short_pith_number":"pith:D35K2P4Q","schema_version":"1.0","canonical_sha256":"1efaad3f90b3ccd1fb43ffd8907bd22361519b3ca9135617e9617e26ed00d3f8","source":{"kind":"arxiv","id":"1711.04330","version":2},"attestation_state":"computed","paper":{"title":"Multiwavelength observations of the black hole X-ray binary A0620-00 in quiescence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Charles D. Bailyn, James C. A. Miller-Jones, Michelle Buxton, Rachel K. D. MacDonald, Tolga Dincer","submitted_at":"2017-11-12T17:59:30Z","abstract_excerpt":"We present results from simultaneous multiwavelength X-ray, radio, and optical/near-infrared observations of the quiescent black hole X-ray binary A0620-00 performed in 2013 December. We find that the Chandra flux has brightened by a factor of 2 since 2005, and by a factor of 7 since 2000. The spectrum has not changed significantly over this time, being consistent with a power law of $\\Gamma = 2.07\\pm 0.13$ and a hydrogen column of $N_H=3.0 \\pm 0.5\\times 10^{21}\\rm{cm}^{-2}$. Very Large Array observations of A0620-00 at three frequencies, over the interval of 5.25--22.0 GHz, have provided us w"},"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":"1711.04330","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-12T17:59:30Z","cross_cats_sorted":[],"title_canon_sha256":"5c131a72c25e476e04f3e6197d6d52fc5f66bb0f2e8f2fcea97db1f978fdd0f1","abstract_canon_sha256":"4fa6f6c86619477e1dd54348624a29d97c49ec68b0cc5cf780330549abe49889"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:24.053012Z","signature_b64":"7XcIXqRuaK9nTVUhlSYv89fijucePTdRhKQkCN0AWVnvIpWzwwas0QA+tU39Y9E6z2bVY2KjXjJnI0jIJOlxCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1efaad3f90b3ccd1fb43ffd8907bd22361519b3ca9135617e9617e26ed00d3f8","last_reissued_at":"2026-05-18T00:26:24.052345Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:24.052345Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwavelength observations of the black hole X-ray binary A0620-00 in quiescence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Charles D. Bailyn, James C. A. Miller-Jones, Michelle Buxton, Rachel K. D. MacDonald, Tolga Dincer","submitted_at":"2017-11-12T17:59:30Z","abstract_excerpt":"We present results from simultaneous multiwavelength X-ray, radio, and optical/near-infrared observations of the quiescent black hole X-ray binary A0620-00 performed in 2013 December. We find that the Chandra flux has brightened by a factor of 2 since 2005, and by a factor of 7 since 2000. The spectrum has not changed significantly over this time, being consistent with a power law of $\\Gamma = 2.07\\pm 0.13$ and a hydrogen column of $N_H=3.0 \\pm 0.5\\times 10^{21}\\rm{cm}^{-2}$. Very Large Array observations of A0620-00 at three frequencies, over the interval of 5.25--22.0 GHz, have provided us w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.04330","kind":"arxiv","version":2},"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":"1711.04330","created_at":"2026-05-18T00:26:24.052442+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.04330v2","created_at":"2026-05-18T00:26:24.052442+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.04330","created_at":"2026-05-18T00:26:24.052442+00:00"},{"alias_kind":"pith_short_12","alias_value":"D35K2P4QWPGN","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"D35K2P4QWPGND62D","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"D35K2P4Q","created_at":"2026-05-18T12:31:10.602751+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/D35K2P4QWPGND62D77MJA66SEN","json":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN.json","graph_json":"https://pith.science/api/pith-number/D35K2P4QWPGND62D77MJA66SEN/graph.json","events_json":"https://pith.science/api/pith-number/D35K2P4QWPGND62D77MJA66SEN/events.json","paper":"https://pith.science/paper/D35K2P4Q"},"agent_actions":{"view_html":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN","download_json":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN.json","view_paper":"https://pith.science/paper/D35K2P4Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.04330&json=true","fetch_graph":"https://pith.science/api/pith-number/D35K2P4QWPGND62D77MJA66SEN/graph.json","fetch_events":"https://pith.science/api/pith-number/D35K2P4QWPGND62D77MJA66SEN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN/action/storage_attestation","attest_author":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN/action/author_attestation","sign_citation":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN/action/citation_signature","submit_replication":"https://pith.science/pith/D35K2P4QWPGND62D77MJA66SEN/action/replication_record"}},"created_at":"2026-05-18T00:26:24.052442+00:00","updated_at":"2026-05-18T00:26:24.052442+00:00"}