{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:KMGQRXII5VDUFLOI3BRGUXLPA2","short_pith_number":"pith:KMGQRXII","schema_version":"1.0","canonical_sha256":"530d08dd08ed4742adc8d8626a5d6f0691f9e19f5f8a42db53a0812c7525c6dd","source":{"kind":"arxiv","id":"1412.2088","version":2},"attestation_state":"computed","paper":{"title":"A NuSTAR observation of the fast symbiotic nova V745 Sco in outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"F. Harrison, J. L. Sokoloski, K. L. Page, M. Orio, V. Rana","submitted_at":"2014-12-05T18:15:22Z","abstract_excerpt":"The fast recurrent nova V745 Sco was observed in the 3-79 keV X-rays band with NuSTAR 10 days after the optical discovery. The measured X-ray emission is consistent with a collisionally ionized optically thin plasma at temperature of about 2.7 keV. A prominent iron line observed at 6.7 keV does not require enhanced iron in the ejecta. We attribute the X-ray flux to shocked circumstellar material. No X-ray emission was observed at energies above 20 keV, and the flux in the 3-20 keV range was about 1.6 $\\times$ 10$^{-11}$ erg cm$^{-2}$ s$^{-1}$. The emission measure indicates an average electron"},"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":"1412.2088","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-12-05T18:15:22Z","cross_cats_sorted":[],"title_canon_sha256":"db65423985e6483fcef636d9364af774631e888b793d049c575ae3fd89b552ef","abstract_canon_sha256":"e92b1319426ed3a904846213860336a666de00e3899bd7ba30e8d904d875386f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:21.349446Z","signature_b64":"VnMCuoZVgi5Mb2pY0rV5nMdwbp6deVOxkeusWlxrh6KBXYIkoDgrGorZYMC/ahpfhEItWvHiTVqfRb43NUaqBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"530d08dd08ed4742adc8d8626a5d6f0691f9e19f5f8a42db53a0812c7525c6dd","last_reissued_at":"2026-05-18T01:41:21.348805Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:21.348805Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A NuSTAR observation of the fast symbiotic nova V745 Sco in outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"F. Harrison, J. L. Sokoloski, K. L. Page, M. Orio, V. Rana","submitted_at":"2014-12-05T18:15:22Z","abstract_excerpt":"The fast recurrent nova V745 Sco was observed in the 3-79 keV X-rays band with NuSTAR 10 days after the optical discovery. The measured X-ray emission is consistent with a collisionally ionized optically thin plasma at temperature of about 2.7 keV. A prominent iron line observed at 6.7 keV does not require enhanced iron in the ejecta. We attribute the X-ray flux to shocked circumstellar material. No X-ray emission was observed at energies above 20 keV, and the flux in the 3-20 keV range was about 1.6 $\\times$ 10$^{-11}$ erg cm$^{-2}$ s$^{-1}$. The emission measure indicates an average electron"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.2088","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":"1412.2088","created_at":"2026-05-18T01:41:21.348908+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.2088v2","created_at":"2026-05-18T01:41:21.348908+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.2088","created_at":"2026-05-18T01:41:21.348908+00:00"},{"alias_kind":"pith_short_12","alias_value":"KMGQRXII5VDU","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"KMGQRXII5VDUFLOI","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"KMGQRXII","created_at":"2026-05-18T12:28:35.611951+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21837","citing_title":"The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review","ref_index":160,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2","json":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2.json","graph_json":"https://pith.science/api/pith-number/KMGQRXII5VDUFLOI3BRGUXLPA2/graph.json","events_json":"https://pith.science/api/pith-number/KMGQRXII5VDUFLOI3BRGUXLPA2/events.json","paper":"https://pith.science/paper/KMGQRXII"},"agent_actions":{"view_html":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2","download_json":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2.json","view_paper":"https://pith.science/paper/KMGQRXII","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.2088&json=true","fetch_graph":"https://pith.science/api/pith-number/KMGQRXII5VDUFLOI3BRGUXLPA2/graph.json","fetch_events":"https://pith.science/api/pith-number/KMGQRXII5VDUFLOI3BRGUXLPA2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2/action/storage_attestation","attest_author":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2/action/author_attestation","sign_citation":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2/action/citation_signature","submit_replication":"https://pith.science/pith/KMGQRXII5VDUFLOI3BRGUXLPA2/action/replication_record"}},"created_at":"2026-05-18T01:41:21.348908+00:00","updated_at":"2026-05-18T01:41:21.348908+00:00"}