{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:LUYF2WVFVTOHKQ5ASAAX6A6BJA","short_pith_number":"pith:LUYF2WVF","schema_version":"1.0","canonical_sha256":"5d305d5aa5acdc7543a090017f03c14813aa23050e7ae5d10119311aad68a5e6","source":{"kind":"arxiv","id":"2206.00211","version":3},"attestation_state":"computed","paper":{"title":"Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"E. M. Reynoso, G. Rowell, H. Sano, K. Tachihara, M. Aruga, Y. Fukui","submitted_at":"2022-06-01T03:34:55Z","abstract_excerpt":"We have carried out a study of the interstellar medium (ISM) toward a shell-like supernova remnant SNR Puppis A by using the NANTEN CO and ATCA HI data. We synthesized a comprehensive picture of the SNR radiation by combining the ISM data with the gamma-ray and X-ray distributions. The ISM, both atomic and molecular gas, is dense and highly clumpy, and is distributed all around the SNR, but mainly in the north-east. The CO distribution revealed an enhanced line intensity ratio of CO($J$ = 2-1)/($J$ = 1-0) transitions as well as CO line broadening, which indicate shock heating/acceleration. The"},"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":"2206.00211","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-06-01T03:34:55Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"2b2a3a42b7a7c35639bf9694895d5f2b865e3107e6a2ba80a285d1ed195b2a09","abstract_canon_sha256":"9cec2ae461d81fa982568d77b4e3ae68be11b1d1d5f0906c7333746a171a23eb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:10:00.463693Z","signature_b64":"XRQrk0bIyL1YRktPTrJcxMPwnKrODj/mMByqbid1aNqt81tOpnvQmm/PYwWHN9+GEwyAEUidHovftt9UOio+Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d305d5aa5acdc7543a090017f03c14813aa23050e7ae5d10119311aad68a5e6","last_reissued_at":"2026-07-05T05:10:00.463208Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:10:00.463208Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"E. M. Reynoso, G. Rowell, H. Sano, K. Tachihara, M. Aruga, Y. Fukui","submitted_at":"2022-06-01T03:34:55Z","abstract_excerpt":"We have carried out a study of the interstellar medium (ISM) toward a shell-like supernova remnant SNR Puppis A by using the NANTEN CO and ATCA HI data. We synthesized a comprehensive picture of the SNR radiation by combining the ISM data with the gamma-ray and X-ray distributions. The ISM, both atomic and molecular gas, is dense and highly clumpy, and is distributed all around the SNR, but mainly in the north-east. The CO distribution revealed an enhanced line intensity ratio of CO($J$ = 2-1)/($J$ = 1-0) transitions as well as CO line broadening, which indicate shock heating/acceleration. The"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.00211","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2206.00211/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2206.00211","created_at":"2026-07-05T05:10:00.463278+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.00211v3","created_at":"2026-07-05T05:10:00.463278+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.00211","created_at":"2026-07-05T05:10:00.463278+00:00"},{"alias_kind":"pith_short_12","alias_value":"LUYF2WVFVTOH","created_at":"2026-07-05T05:10:00.463278+00:00"},{"alias_kind":"pith_short_16","alias_value":"LUYF2WVFVTOHKQ5A","created_at":"2026-07-05T05:10:00.463278+00:00"},{"alias_kind":"pith_short_8","alias_value":"LUYF2WVF","created_at":"2026-07-05T05:10:00.463278+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/LUYF2WVFVTOHKQ5ASAAX6A6BJA","json":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA.json","graph_json":"https://pith.science/api/pith-number/LUYF2WVFVTOHKQ5ASAAX6A6BJA/graph.json","events_json":"https://pith.science/api/pith-number/LUYF2WVFVTOHKQ5ASAAX6A6BJA/events.json","paper":"https://pith.science/paper/LUYF2WVF"},"agent_actions":{"view_html":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA","download_json":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA.json","view_paper":"https://pith.science/paper/LUYF2WVF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.00211&json=true","fetch_graph":"https://pith.science/api/pith-number/LUYF2WVFVTOHKQ5ASAAX6A6BJA/graph.json","fetch_events":"https://pith.science/api/pith-number/LUYF2WVFVTOHKQ5ASAAX6A6BJA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA/action/storage_attestation","attest_author":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA/action/author_attestation","sign_citation":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA/action/citation_signature","submit_replication":"https://pith.science/pith/LUYF2WVFVTOHKQ5ASAAX6A6BJA/action/replication_record"}},"created_at":"2026-07-05T05:10:00.463278+00:00","updated_at":"2026-07-05T05:10:00.463278+00:00"}