{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:OJHLI3K6WTVERV4MDLWQKL3PEU","short_pith_number":"pith:OJHLI3K6","schema_version":"1.0","canonical_sha256":"724eb46d5eb4ea48d78c1aed052f6f251af3c2de24ca43e8f9ec1b52f8d3f276","source":{"kind":"arxiv","id":"1103.2527","version":2},"attestation_state":"computed","paper":{"title":"Molecular Environment and an X-ray Spectroscopy of Supernova Remnant Kesteven 78","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ping Zhou, Yang Chen (Nanjing University)","submitted_at":"2011-03-13T16:19:50Z","abstract_excerpt":"We investigate the molecular environment of the Galactic supernova remnant (SNR) Kesteven 78 and perform an XMM-Newton X-ray spectroscopic study for the northeastern edge of the remnant. SNR Kes78 is found to interact with the molecular clouds (MCs) at a systemic local standard of rest velocity of 81km/s. At around this velocity, the SNR appears to contact a long molecular strip in the northeast and a large cloud in the east as revealed in the 13CO line, which may be responsible for the radio brightness peak and the OH maser, respectively. The 12CO-line bright region morphologically matches th"},"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":"1103.2527","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2011-03-13T16:19:50Z","cross_cats_sorted":[],"title_canon_sha256":"e7df5a2fc6182c9b532409f3560bb5a6a1f1047ef03621dfdccaa045f6ee3fb8","abstract_canon_sha256":"99179f37f69870a7490b7110c696844617f96172fa401f7ed81cdcf36cc53fe3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:54.145421Z","signature_b64":"Cs5xOaYLYBHyrLxuYVDXD8rl32xccWhQ07H3CgX90yudOFRK0wkSsFsBZHYbJN9ctIneh5nvs/JOPh7VNIGkAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"724eb46d5eb4ea48d78c1aed052f6f251af3c2de24ca43e8f9ec1b52f8d3f276","last_reissued_at":"2026-05-18T02:02:54.144460Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:54.144460Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Molecular Environment and an X-ray Spectroscopy of Supernova Remnant Kesteven 78","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ping Zhou, Yang Chen (Nanjing University)","submitted_at":"2011-03-13T16:19:50Z","abstract_excerpt":"We investigate the molecular environment of the Galactic supernova remnant (SNR) Kesteven 78 and perform an XMM-Newton X-ray spectroscopic study for the northeastern edge of the remnant. SNR Kes78 is found to interact with the molecular clouds (MCs) at a systemic local standard of rest velocity of 81km/s. At around this velocity, the SNR appears to contact a long molecular strip in the northeast and a large cloud in the east as revealed in the 13CO line, which may be responsible for the radio brightness peak and the OH maser, respectively. The 12CO-line bright region morphologically matches th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.2527","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":"1103.2527","created_at":"2026-05-18T02:02:54.144628+00:00"},{"alias_kind":"arxiv_version","alias_value":"1103.2527v2","created_at":"2026-05-18T02:02:54.144628+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1103.2527","created_at":"2026-05-18T02:02:54.144628+00:00"},{"alias_kind":"pith_short_12","alias_value":"OJHLI3K6WTVE","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_16","alias_value":"OJHLI3K6WTVERV4M","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_8","alias_value":"OJHLI3K6","created_at":"2026-05-18T12:26:37.096874+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/OJHLI3K6WTVERV4MDLWQKL3PEU","json":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU.json","graph_json":"https://pith.science/api/pith-number/OJHLI3K6WTVERV4MDLWQKL3PEU/graph.json","events_json":"https://pith.science/api/pith-number/OJHLI3K6WTVERV4MDLWQKL3PEU/events.json","paper":"https://pith.science/paper/OJHLI3K6"},"agent_actions":{"view_html":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU","download_json":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU.json","view_paper":"https://pith.science/paper/OJHLI3K6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1103.2527&json=true","fetch_graph":"https://pith.science/api/pith-number/OJHLI3K6WTVERV4MDLWQKL3PEU/graph.json","fetch_events":"https://pith.science/api/pith-number/OJHLI3K6WTVERV4MDLWQKL3PEU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU/action/storage_attestation","attest_author":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU/action/author_attestation","sign_citation":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU/action/citation_signature","submit_replication":"https://pith.science/pith/OJHLI3K6WTVERV4MDLWQKL3PEU/action/replication_record"}},"created_at":"2026-05-18T02:02:54.144628+00:00","updated_at":"2026-05-18T02:02:54.144628+00:00"}