{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:47NJNGYZOJQC74C5MF3ZHDTA7E","short_pith_number":"pith:47NJNGYZ","schema_version":"1.0","canonical_sha256":"e7da969b1972602ff05d6177938e60f929ccf36284bd40bb3950822a4fa23ce3","source":{"kind":"arxiv","id":"1602.06414","version":2},"attestation_state":"computed","paper":{"title":"A \"high-hard\" outburst of the black hole X-ray binary GS 1354-64","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. M. Russell, F. E. Bauer, F. Lewis, J. M. Corral-Santana, K. I. I. Koljonen, M. Armas Padilla, M. Coriat, T. Mu\\~noz-Darias","submitted_at":"2016-02-20T14:50:20Z","abstract_excerpt":"We study in detail the evolution of the 2015 outburst of GS 1354-64 (BW Cir) at optical, UV and X-ray wavelengths using Faulkes Telescope South/LCOGT, SMARTS and Swift. The outburst was found to stay in the hard X-ray state, albeit being anomalously luminous with a peak luminosity of L$_{X} >$ 0.15 L$_{Edd}$, which could be the most luminous hard state observed in a black hole X-ray binary. We found that the optical/UV emission is tightly correlated with the X-ray emission, consistent with accretion disc irradiation and/or a jet producing the optical emission. The X-ray spectra can be fitted 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":"1602.06414","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-02-20T14:50:20Z","cross_cats_sorted":[],"title_canon_sha256":"048b37709a9e0701ffa18649b4817a3836436940eb3556aaf5014637c1311960","abstract_canon_sha256":"6bc7afeea4f571c0d98cbedfd7cc390153ab39daecbb3851804d1bdf39eb23bf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:55.353784Z","signature_b64":"fE4LmZHzANB12/NZmAv4CM0ZGHvcG1RkednVDQplyhWq06rQQcxkSIrFpecPwZhG0Pp6TU8Ss67xRdCOc4hEBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7da969b1972602ff05d6177938e60f929ccf36284bd40bb3950822a4fa23ce3","last_reissued_at":"2026-05-18T01:13:55.353118Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:55.353118Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A \"high-hard\" outburst of the black hole X-ray binary GS 1354-64","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. M. Russell, F. E. Bauer, F. Lewis, J. M. Corral-Santana, K. I. I. Koljonen, M. Armas Padilla, M. Coriat, T. Mu\\~noz-Darias","submitted_at":"2016-02-20T14:50:20Z","abstract_excerpt":"We study in detail the evolution of the 2015 outburst of GS 1354-64 (BW Cir) at optical, UV and X-ray wavelengths using Faulkes Telescope South/LCOGT, SMARTS and Swift. The outburst was found to stay in the hard X-ray state, albeit being anomalously luminous with a peak luminosity of L$_{X} >$ 0.15 L$_{Edd}$, which could be the most luminous hard state observed in a black hole X-ray binary. We found that the optical/UV emission is tightly correlated with the X-ray emission, consistent with accretion disc irradiation and/or a jet producing the optical emission. The X-ray spectra can be fitted w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.06414","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":"1602.06414","created_at":"2026-05-18T01:13:55.353210+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.06414v2","created_at":"2026-05-18T01:13:55.353210+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.06414","created_at":"2026-05-18T01:13:55.353210+00:00"},{"alias_kind":"pith_short_12","alias_value":"47NJNGYZOJQC","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_16","alias_value":"47NJNGYZOJQC74C5","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_8","alias_value":"47NJNGYZ","created_at":"2026-05-18T12:29:58.707656+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/47NJNGYZOJQC74C5MF3ZHDTA7E","json":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E.json","graph_json":"https://pith.science/api/pith-number/47NJNGYZOJQC74C5MF3ZHDTA7E/graph.json","events_json":"https://pith.science/api/pith-number/47NJNGYZOJQC74C5MF3ZHDTA7E/events.json","paper":"https://pith.science/paper/47NJNGYZ"},"agent_actions":{"view_html":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E","download_json":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E.json","view_paper":"https://pith.science/paper/47NJNGYZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.06414&json=true","fetch_graph":"https://pith.science/api/pith-number/47NJNGYZOJQC74C5MF3ZHDTA7E/graph.json","fetch_events":"https://pith.science/api/pith-number/47NJNGYZOJQC74C5MF3ZHDTA7E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E/action/storage_attestation","attest_author":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E/action/author_attestation","sign_citation":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E/action/citation_signature","submit_replication":"https://pith.science/pith/47NJNGYZOJQC74C5MF3ZHDTA7E/action/replication_record"}},"created_at":"2026-05-18T01:13:55.353210+00:00","updated_at":"2026-05-18T01:13:55.353210+00:00"}