{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:3CP6LUQB534OYCAL45ISGM2B3B","short_pith_number":"pith:3CP6LUQB","schema_version":"1.0","canonical_sha256":"d89fe5d201eef8ec080be751233341d87c54d9ac0fde0ba05f51907c891ef0b4","source":{"kind":"arxiv","id":"1612.01923","version":1},"attestation_state":"computed","paper":{"title":"XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bamba, F. Bocchino, M. Miceli, P. Zhou, S. Orlando, S. Safi-Harb, Y. Chen","submitted_at":"2016-12-06T17:49:26Z","abstract_excerpt":"The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray emission from the remnant has been recently revealed by Suzaku observations, which have shown indications for a hard X-ray component in the spectra, possibly associated with synchrotron radiation. We aim at describing the spatial distribution of the physical properties of the X-ray emitting plasma and at revealing the effects of the interaction of the remnant with the inhomogeneous ambient medium. We also aim at inves"},"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":"1612.01923","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-06T17:49:26Z","cross_cats_sorted":[],"title_canon_sha256":"3b2abfc5729afdbf053b688f55416f1ab578dbea79e566a9ddb97ecf120b90e4","abstract_canon_sha256":"90e00a1b064bc32ac2a52fab494063d1e7e0546e47aa91fff0d404202d78910f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:49:50.954126Z","signature_b64":"pnVgsZ4wHu3qNLuSlXb4y3lyyOADLYocL2NNXsROsvZwDmcTOkFO63ajMh65636/sukw8kp+mFPEex/IMadsCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d89fe5d201eef8ec080be751233341d87c54d9ac0fde0ba05f51907c891ef0b4","last_reissued_at":"2026-05-18T00:49:50.953770Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:49:50.953770Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"XMM-Newton observation of the supernova remnant Kes 78 (G32.8-0.1): Evidence for shock-cloud interaction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bamba, F. Bocchino, M. Miceli, P. Zhou, S. Orlando, S. Safi-Harb, Y. Chen","submitted_at":"2016-12-06T17:49:26Z","abstract_excerpt":"The Galactic supernova remnant Kes 78 is surrounded by dense molecular clouds, whose projected position overlaps with the extended HESS gamma-ray source HESS J1852-000. The X-ray emission from the remnant has been recently revealed by Suzaku observations, which have shown indications for a hard X-ray component in the spectra, possibly associated with synchrotron radiation. We aim at describing the spatial distribution of the physical properties of the X-ray emitting plasma and at revealing the effects of the interaction of the remnant with the inhomogeneous ambient medium. We also aim at inves"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.01923","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":"1612.01923","created_at":"2026-05-18T00:49:50.953827+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.01923v1","created_at":"2026-05-18T00:49:50.953827+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.01923","created_at":"2026-05-18T00:49:50.953827+00:00"},{"alias_kind":"pith_short_12","alias_value":"3CP6LUQB534O","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_16","alias_value":"3CP6LUQB534OYCAL","created_at":"2026-05-18T12:29:55.572404+00:00"},{"alias_kind":"pith_short_8","alias_value":"3CP6LUQB","created_at":"2026-05-18T12:29:55.572404+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/3CP6LUQB534OYCAL45ISGM2B3B","json":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B.json","graph_json":"https://pith.science/api/pith-number/3CP6LUQB534OYCAL45ISGM2B3B/graph.json","events_json":"https://pith.science/api/pith-number/3CP6LUQB534OYCAL45ISGM2B3B/events.json","paper":"https://pith.science/paper/3CP6LUQB"},"agent_actions":{"view_html":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B","download_json":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B.json","view_paper":"https://pith.science/paper/3CP6LUQB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.01923&json=true","fetch_graph":"https://pith.science/api/pith-number/3CP6LUQB534OYCAL45ISGM2B3B/graph.json","fetch_events":"https://pith.science/api/pith-number/3CP6LUQB534OYCAL45ISGM2B3B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B/action/storage_attestation","attest_author":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B/action/author_attestation","sign_citation":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B/action/citation_signature","submit_replication":"https://pith.science/pith/3CP6LUQB534OYCAL45ISGM2B3B/action/replication_record"}},"created_at":"2026-05-18T00:49:50.953827+00:00","updated_at":"2026-05-18T00:49:50.953827+00:00"}