{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2001:K225HLAWQAZE47DTLNR3ZSFMHA","short_pith_number":"pith:K225HLAW","canonical_record":{"source":{"id":"astro-ph/0103362","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-03-22T09:23:43Z","cross_cats_sorted":[],"title_canon_sha256":"d6d079060f2ca2d9ca890c0fa3ed7a9bf93ca60cac9d0475971a92a5bdb290fa","abstract_canon_sha256":"b53ac3335df6ee558695098753aebccd6fc0c303033dc46bbe4ccaf69d164511"},"schema_version":"1.0"},"canonical_sha256":"56b5d3ac1680324e7c735b63bcc8ac38161bc722614fdca8d8ef5eb43da4d4e6","source":{"kind":"arxiv","id":"astro-ph/0103362","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0103362","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0103362v1","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0103362","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"pith_short_12","alias_value":"K225HLAWQAZE","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"pith_short_16","alias_value":"K225HLAWQAZE47DT","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"pith_short_8","alias_value":"K225HLAW","created_at":"2026-07-04T16:22:55Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2001:K225HLAWQAZE47DTLNR3ZSFMHA","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0103362","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-03-22T09:23:43Z","cross_cats_sorted":[],"title_canon_sha256":"d6d079060f2ca2d9ca890c0fa3ed7a9bf93ca60cac9d0475971a92a5bdb290fa","abstract_canon_sha256":"b53ac3335df6ee558695098753aebccd6fc0c303033dc46bbe4ccaf69d164511"},"schema_version":"1.0"},"canonical_sha256":"56b5d3ac1680324e7c735b63bcc8ac38161bc722614fdca8d8ef5eb43da4d4e6","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:22:55.313923Z","signature_b64":"gUjKQZIZMQI54ZiGarGDWEuOyEUrVLCtrMZeY/UNRt9O+HXcHvtA3voMHatUAByFpzsZouj8MkLaFLqsyZsoAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"56b5d3ac1680324e7c735b63bcc8ac38161bc722614fdca8d8ef5eb43da4d4e6","last_reissued_at":"2026-07-04T16:22:55.313491Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:22:55.313491Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0103362","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:22:55Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uoBdgrtYVJ2WTqcb5l5B+UnCrdG28a1GSFpZHkxCQxhPWZ6T6Ofmyb5fiAq/2n/VvZShx77Dpcun2wTgrYzBBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T01:56:59.682682Z"},"content_sha256":"51c3cafbd934d7feed921a12c41dbd6c69f2c5f56088bc5223c88120f57745b5","schema_version":"1.0","event_id":"sha256:51c3cafbd934d7feed921a12c41dbd6c69f2c5f56088bc5223c88120f57745b5"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2001:K225HLAWQAZE47DTLNR3ZSFMHA","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Application of a relativistic accretion disc model to X-ray spectra of LMC X-1 and GRO J1655-40","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Andrzej Maciolek-Niedzwiecki, Ken Ebisawa, Marek Gierlinski","submitted_at":"2001-03-22T09:23:43Z","abstract_excerpt":"We present a general relativistic accretion disc model and its application to the soft-state X-ray spectra of black hole binaries. The model assumes a flat, optically thick disc around a rotating Kerr black hole. The disc locally radiates away the dissipated energy as a blackbody. Special and general relativistic effects influencing photons emitted by the disc are taken into account. The emerging spectrum, as seen by a distant observer, is parametrized by the black hole mass and spin, the accretion rate, the disc inclination angle and the inner disc radius. We fit the ASCA soft state X-ray spe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0103362","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/0103362/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:22:55Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"z9IpoU8qXLMV3XQuhumKEt+DWTSnzu5ajQzl7s01gjCpneg5cA/8jTnzVjk2wBwwqEG7bs8cJiVdjqKxiUL2Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T01:56:59.683265Z"},"content_sha256":"810cf7ff7509a26b28246789291f07eebd8ea4a0da644e1cd2e1d7bde355c33a","schema_version":"1.0","event_id":"sha256:810cf7ff7509a26b28246789291f07eebd8ea4a0da644e1cd2e1d7bde355c33a"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/K225HLAWQAZE47DTLNR3ZSFMHA/bundle.json","state_url":"https://pith.science/pith/K225HLAWQAZE47DTLNR3ZSFMHA/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/K225HLAWQAZE47DTLNR3ZSFMHA/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-04T01:56:59Z","links":{"resolver":"https://pith.science/pith/K225HLAWQAZE47DTLNR3ZSFMHA","bundle":"https://pith.science/pith/K225HLAWQAZE47DTLNR3ZSFMHA/bundle.json","state":"https://pith.science/pith/K225HLAWQAZE47DTLNR3ZSFMHA/state.json","well_known_bundle":"https://pith.science/.well-known/pith/K225HLAWQAZE47DTLNR3ZSFMHA/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2001:K225HLAWQAZE47DTLNR3ZSFMHA","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"b53ac3335df6ee558695098753aebccd6fc0c303033dc46bbe4ccaf69d164511","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2001-03-22T09:23:43Z","title_canon_sha256":"d6d079060f2ca2d9ca890c0fa3ed7a9bf93ca60cac9d0475971a92a5bdb290fa"},"schema_version":"1.0","source":{"id":"astro-ph/0103362","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0103362","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0103362v1","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0103362","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"pith_short_12","alias_value":"K225HLAWQAZE","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"pith_short_16","alias_value":"K225HLAWQAZE47DT","created_at":"2026-07-04T16:22:55Z"},{"alias_kind":"pith_short_8","alias_value":"K225HLAW","created_at":"2026-07-04T16:22:55Z"}],"graph_snapshots":[{"event_id":"sha256:810cf7ff7509a26b28246789291f07eebd8ea4a0da644e1cd2e1d7bde355c33a","target":"graph","created_at":"2026-07-04T16:22:55Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/astro-ph/0103362/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We present a general relativistic accretion disc model and its application to the soft-state X-ray spectra of black hole binaries. The model assumes a flat, optically thick disc around a rotating Kerr black hole. The disc locally radiates away the dissipated energy as a blackbody. Special and general relativistic effects influencing photons emitted by the disc are taken into account. The emerging spectrum, as seen by a distant observer, is parametrized by the black hole mass and spin, the accretion rate, the disc inclination angle and the inner disc radius. We fit the ASCA soft state X-ray spe","authors_text":"Andrzej Maciolek-Niedzwiecki, Ken Ebisawa, Marek Gierlinski","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2001-03-22T09:23:43Z","title":"Application of a relativistic accretion disc model to X-ray spectra of LMC X-1 and GRO J1655-40"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0103362","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:51c3cafbd934d7feed921a12c41dbd6c69f2c5f56088bc5223c88120f57745b5","target":"record","created_at":"2026-07-04T16:22:55Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"b53ac3335df6ee558695098753aebccd6fc0c303033dc46bbe4ccaf69d164511","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2001-03-22T09:23:43Z","title_canon_sha256":"d6d079060f2ca2d9ca890c0fa3ed7a9bf93ca60cac9d0475971a92a5bdb290fa"},"schema_version":"1.0","source":{"id":"astro-ph/0103362","kind":"arxiv","version":1}},"canonical_sha256":"56b5d3ac1680324e7c735b63bcc8ac38161bc722614fdca8d8ef5eb43da4d4e6","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"56b5d3ac1680324e7c735b63bcc8ac38161bc722614fdca8d8ef5eb43da4d4e6","first_computed_at":"2026-07-04T16:22:55.313491Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T16:22:55.313491Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"gUjKQZIZMQI54ZiGarGDWEuOyEUrVLCtrMZeY/UNRt9O+HXcHvtA3voMHatUAByFpzsZouj8MkLaFLqsyZsoAA==","signature_status":"signed_v1","signed_at":"2026-07-04T16:22:55.313923Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0103362","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:51c3cafbd934d7feed921a12c41dbd6c69f2c5f56088bc5223c88120f57745b5","sha256:810cf7ff7509a26b28246789291f07eebd8ea4a0da644e1cd2e1d7bde355c33a"],"state_sha256":"d1a5b6fe3f4200eb30b0214651b18ad36b88c59f53c7fa0343e19b51bc04fe08"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AtN3JrnYQo/yXawmoUTynBMFSREAlaR5CFTBWh/FojKI8FeG0dIOFxCsMQVeJGxY4Zvj7WRaZT7xC9QuM7bVBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-04T01:56:59.686783Z","bundle_sha256":"52bb1832b879194e88d313fb5c49d1efabd6d2239d3dad6098ea8cf4b6963918"}}