{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:QSU2TOAN5L2JMC2736VVALRPJ5","short_pith_number":"pith:QSU2TOAN","schema_version":"1.0","canonical_sha256":"84a9a9b80deaf4960b5fdfab502e2f4f78cc9152ce7c6ceb972a3751768c2209","source":{"kind":"arxiv","id":"astro-ph/0608232","version":1},"attestation_state":"computed","paper":{"title":"Correlation between Flux and Spectral Index during Flares in Sagittarius A*","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Christopher L. Fryer, Jonathan M. Bittner, Siming Liu, Vahe Petrosian","submitted_at":"2006-08-10T21:43:50Z","abstract_excerpt":"Flares in Sagittarius A* are produced by hot plasmas within a few Schwarzschild radii of the supermassive black hole at the Galactic center. The recent detection of a correlation between the spectral index and flux during a near infrared (NIR) flare provides a means to conduct detailed investigations of the plasma heating and radiation processes. We study the evolution of the electron distribution function under the influence of a turbulent magnetic field in a hot collisionless plasma. The magnetic field, presumably generated through instabilities in the accretion flow, can both heat the plasm"},"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/0608232","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-08-10T21:43:50Z","cross_cats_sorted":[],"title_canon_sha256":"ffe567cc19948e00157cb5ef472a1c7b5f17c51b5e4f8487d5e94bddb3ab6132","abstract_canon_sha256":"485226f53ebe4cd3153ac68615899395916a49d6409e438629811c0b1b331ee0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:28:58.076483Z","signature_b64":"/Emx/TAfanlB5cjbKtYnV7m5ZATkn/7TGCHSNspBVuk9tkfmMg3AM8qX4Ti0Ppmm3VDi+9NKPnHzzsgLTHlaCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"84a9a9b80deaf4960b5fdfab502e2f4f78cc9152ce7c6ceb972a3751768c2209","last_reissued_at":"2026-05-18T04:28:58.076077Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:28:58.076077Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Correlation between Flux and Spectral Index during Flares in Sagittarius A*","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Christopher L. Fryer, Jonathan M. Bittner, Siming Liu, Vahe Petrosian","submitted_at":"2006-08-10T21:43:50Z","abstract_excerpt":"Flares in Sagittarius A* are produced by hot plasmas within a few Schwarzschild radii of the supermassive black hole at the Galactic center. The recent detection of a correlation between the spectral index and flux during a near infrared (NIR) flare provides a means to conduct detailed investigations of the plasma heating and radiation processes. We study the evolution of the electron distribution function under the influence of a turbulent magnetic field in a hot collisionless plasma. The magnetic field, presumably generated through instabilities in the accretion flow, can both heat the plasm"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0608232","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":"astro-ph/0608232","created_at":"2026-05-18T04:28:58.076146+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0608232v1","created_at":"2026-05-18T04:28:58.076146+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0608232","created_at":"2026-05-18T04:28:58.076146+00:00"},{"alias_kind":"pith_short_12","alias_value":"QSU2TOAN5L2J","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"QSU2TOAN5L2JMC27","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"QSU2TOAN","created_at":"2026-05-18T12:25:54.717736+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/QSU2TOAN5L2JMC2736VVALRPJ5","json":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5.json","graph_json":"https://pith.science/api/pith-number/QSU2TOAN5L2JMC2736VVALRPJ5/graph.json","events_json":"https://pith.science/api/pith-number/QSU2TOAN5L2JMC2736VVALRPJ5/events.json","paper":"https://pith.science/paper/QSU2TOAN"},"agent_actions":{"view_html":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5","download_json":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5.json","view_paper":"https://pith.science/paper/QSU2TOAN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0608232&json=true","fetch_graph":"https://pith.science/api/pith-number/QSU2TOAN5L2JMC2736VVALRPJ5/graph.json","fetch_events":"https://pith.science/api/pith-number/QSU2TOAN5L2JMC2736VVALRPJ5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5/action/storage_attestation","attest_author":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5/action/author_attestation","sign_citation":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5/action/citation_signature","submit_replication":"https://pith.science/pith/QSU2TOAN5L2JMC2736VVALRPJ5/action/replication_record"}},"created_at":"2026-05-18T04:28:58.076146+00:00","updated_at":"2026-05-18T04:28:58.076146+00:00"}