{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:7GZSZHQFZPZPDC3QQ6FF6TSB7A","short_pith_number":"pith:7GZSZHQF","schema_version":"1.0","canonical_sha256":"f9b32c9e05cbf2f18b70878a5f4e41f83f801000fc66075db764b0e31af34562","source":{"kind":"arxiv","id":"1504.03495","version":1},"attestation_state":"computed","paper":{"title":"Exploring plasma evolution during Sagittarius A* flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"John A. Tomsick, Julien Malzac, Nicolas M. Barriere, Renaud Belmont, Salome Dibi, Sera Markoff","submitted_at":"2015-04-14T11:20:22Z","abstract_excerpt":"We present a new way of describing the flares from Sgr A* with a self-consistent calculation of the particle distribution. All relevant radiative processes are taken into account in the evolution of the electron distribution and resulting spectrum. We present spectral modelling for new X-ray flares observed by NuSTAR, together with older observations in different wavelengths, and discuss the changes in plasma parameters to produce a flare. We show that under certain conditions, the real particle distribution can differ significantly from standard distributions assumed in most studies. We concl"},"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":"1504.03495","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-04-14T11:20:22Z","cross_cats_sorted":[],"title_canon_sha256":"aaeba3b89a359a1b9357aaafe74f6951ea82586f675aeb9febc748bc27a66ee9","abstract_canon_sha256":"4d0ac75e0e9757e647a20dee966f66d9b518a4aefec0771edc1449446df2b7da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:18:50.721805Z","signature_b64":"vFaH8AxUSMl6BjubN2B6rxGQqgVMd1I6ycAK4B65j8bG7goF42JIXO54v/0dHEQCPO8vAfrTyv8tXVAtQZohBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f9b32c9e05cbf2f18b70878a5f4e41f83f801000fc66075db764b0e31af34562","last_reissued_at":"2026-05-18T02:18:50.721197Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:18:50.721197Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring plasma evolution during Sagittarius A* flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"John A. Tomsick, Julien Malzac, Nicolas M. Barriere, Renaud Belmont, Salome Dibi, Sera Markoff","submitted_at":"2015-04-14T11:20:22Z","abstract_excerpt":"We present a new way of describing the flares from Sgr A* with a self-consistent calculation of the particle distribution. All relevant radiative processes are taken into account in the evolution of the electron distribution and resulting spectrum. We present spectral modelling for new X-ray flares observed by NuSTAR, together with older observations in different wavelengths, and discuss the changes in plasma parameters to produce a flare. We show that under certain conditions, the real particle distribution can differ significantly from standard distributions assumed in most studies. We concl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.03495","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":"1504.03495","created_at":"2026-05-18T02:18:50.721278+00:00"},{"alias_kind":"arxiv_version","alias_value":"1504.03495v1","created_at":"2026-05-18T02:18:50.721278+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1504.03495","created_at":"2026-05-18T02:18:50.721278+00:00"},{"alias_kind":"pith_short_12","alias_value":"7GZSZHQFZPZP","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_16","alias_value":"7GZSZHQFZPZPDC3Q","created_at":"2026-05-18T12:29:10.953037+00:00"},{"alias_kind":"pith_short_8","alias_value":"7GZSZHQF","created_at":"2026-05-18T12:29:10.953037+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/7GZSZHQFZPZPDC3QQ6FF6TSB7A","json":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A.json","graph_json":"https://pith.science/api/pith-number/7GZSZHQFZPZPDC3QQ6FF6TSB7A/graph.json","events_json":"https://pith.science/api/pith-number/7GZSZHQFZPZPDC3QQ6FF6TSB7A/events.json","paper":"https://pith.science/paper/7GZSZHQF"},"agent_actions":{"view_html":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A","download_json":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A.json","view_paper":"https://pith.science/paper/7GZSZHQF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1504.03495&json=true","fetch_graph":"https://pith.science/api/pith-number/7GZSZHQFZPZPDC3QQ6FF6TSB7A/graph.json","fetch_events":"https://pith.science/api/pith-number/7GZSZHQFZPZPDC3QQ6FF6TSB7A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A/action/storage_attestation","attest_author":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A/action/author_attestation","sign_citation":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A/action/citation_signature","submit_replication":"https://pith.science/pith/7GZSZHQFZPZPDC3QQ6FF6TSB7A/action/replication_record"}},"created_at":"2026-05-18T02:18:50.721278+00:00","updated_at":"2026-05-18T02:18:50.721278+00:00"}