{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:Y75ODDLQ6KFKPPGIZPQOYFIJNZ","short_pith_number":"pith:Y75ODDLQ","schema_version":"1.0","canonical_sha256":"c7fae18d70f28aa7bcc8cbe0ec15096e62b476a17d83a1f10cdf3753698ced16","source":{"kind":"arxiv","id":"astro-ph/0109136","version":1},"attestation_state":"computed","paper":{"title":"The quiescent light curve and evolutionary state of GRO J1655-40","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Martin E. Beer, Philipp Podsiadlowski (Oxford)","submitted_at":"2001-09-08T14:42:55Z","abstract_excerpt":"We present ellipsoidal light-curve fits to the quiescent B, V, R and I light curves of GRO J1655-40 (Nova Scorpii 1994). The fits are based on a simple model consisting of a Roche-lobe filling secondary and an accretion disc around the black-hole primary. Unlike previous studies, no assumptions are made about the interstellar extinction or the distance to the source; instead these are determined self-consistently from the observed light curves. In order to obtain tighter limits on the model parameters, we used the distance determination from the kinematics of the radio jet as an additional con"},"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":"astro-ph/0109136","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-09-08T14:42:55Z","cross_cats_sorted":[],"title_canon_sha256":"9861aa88b1d49386fabda798f02d51b74690c6af2ef547072edaebdf3ef4492d","abstract_canon_sha256":"275fb3aec562c0c893d1eaa4fd0372b28d61655c3ef7e3e16626e475ac1c921d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:24:05.430262Z","signature_b64":"ldjSz8Y37Fd5sxrxlmd2XmPzzr+t1XvpJBPl0guCU24hDiYbig7jJG2+QJpZg0cRuMtj6OJ4BGePsdXMqWhrCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c7fae18d70f28aa7bcc8cbe0ec15096e62b476a17d83a1f10cdf3753698ced16","last_reissued_at":"2026-07-04T16:24:05.429850Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:24:05.429850Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The quiescent light curve and evolutionary state of GRO J1655-40","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Martin E. Beer, Philipp Podsiadlowski (Oxford)","submitted_at":"2001-09-08T14:42:55Z","abstract_excerpt":"We present ellipsoidal light-curve fits to the quiescent B, V, R and I light curves of GRO J1655-40 (Nova Scorpii 1994). The fits are based on a simple model consisting of a Roche-lobe filling secondary and an accretion disc around the black-hole primary. Unlike previous studies, no assumptions are made about the interstellar extinction or the distance to the source; instead these are determined self-consistently from the observed light curves. In order to obtain tighter limits on the model parameters, we used the distance determination from the kinematics of the radio jet as an additional con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0109136","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0109136/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0109136","created_at":"2026-07-04T16:24:05.429912+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0109136v1","created_at":"2026-07-04T16:24:05.429912+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0109136","created_at":"2026-07-04T16:24:05.429912+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y75ODDLQ6KFK","created_at":"2026-07-04T16:24:05.429912+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y75ODDLQ6KFKPPGI","created_at":"2026-07-04T16:24:05.429912+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y75ODDLQ","created_at":"2026-07-04T16:24:05.429912+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/Y75ODDLQ6KFKPPGIZPQOYFIJNZ","json":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ.json","graph_json":"https://pith.science/api/pith-number/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/graph.json","events_json":"https://pith.science/api/pith-number/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/events.json","paper":"https://pith.science/paper/Y75ODDLQ"},"agent_actions":{"view_html":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ","download_json":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ.json","view_paper":"https://pith.science/paper/Y75ODDLQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0109136&json=true","fetch_graph":"https://pith.science/api/pith-number/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/graph.json","fetch_events":"https://pith.science/api/pith-number/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/action/storage_attestation","attest_author":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/action/author_attestation","sign_citation":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/action/citation_signature","submit_replication":"https://pith.science/pith/Y75ODDLQ6KFKPPGIZPQOYFIJNZ/action/replication_record"}},"created_at":"2026-07-04T16:24:05.429912+00:00","updated_at":"2026-07-04T16:24:05.429912+00:00"}