{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:ITNCX352HR7O2N5LTO3UD2NVSU","short_pith_number":"pith:ITNCX352","schema_version":"1.0","canonical_sha256":"44da2befba3c7eed37ab9bb741e9b5952ea7beb583346e8c446186cab0040614","source":{"kind":"arxiv","id":"0802.3742","version":3},"attestation_state":"computed","paper":{"title":"X-ray observations of the Coma Cluster in a broad energy band with INTEGRAL, RXTE, and ROSAT observatories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A.A. Lutovinov, A. Vikhlinin, E.M. Churazov, M.G. Revnivtsev, R.A. Sunyaev","submitted_at":"2008-02-26T04:46:11Z","abstract_excerpt":"We present results of X-ray observations of the Coma cluster with multiple instruments over a broad energy band. Using the data from INTEGRAL, RXTE and ROSAT observatories, we find that the Coma spectrum in the 0.5-107 keV energy band can be well approximated by a thermal plasma emission model with a temperature of T=8.2 keV. INTEGRAL was used to image the cluster emission in the hard energy band. The cluster is only marginally detectable ~1.6sigma in the 44-107 keV energy band; however, the raw flux in this band is consistent with the previous results from Beppo-SAX and RXTE observatories. We"},"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":"0802.3742","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-02-26T04:46:11Z","cross_cats_sorted":[],"title_canon_sha256":"2fc85faa58ae141dcd5aba5d2b59d04da10a2e9567802b4ee24b641eaee88af3","abstract_canon_sha256":"bdd7c0b90fc3f10f83e9e5ad056e862c1762ead16d7d9d8eb7364af0ca87f1f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:09:34.761720Z","signature_b64":"heN+E2tcR2abj87ID8Dv7vfp/DhIiQWMAxcIKng+XXEw+oirKaCNSobjzTY+ts0wnf4Gp0rKnPw1lMcV7AYLBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"44da2befba3c7eed37ab9bb741e9b5952ea7beb583346e8c446186cab0040614","last_reissued_at":"2026-07-04T17:09:34.761332Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:09:34.761332Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray observations of the Coma Cluster in a broad energy band with INTEGRAL, RXTE, and ROSAT observatories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A.A. Lutovinov, A. Vikhlinin, E.M. Churazov, M.G. Revnivtsev, R.A. Sunyaev","submitted_at":"2008-02-26T04:46:11Z","abstract_excerpt":"We present results of X-ray observations of the Coma cluster with multiple instruments over a broad energy band. Using the data from INTEGRAL, RXTE and ROSAT observatories, we find that the Coma spectrum in the 0.5-107 keV energy band can be well approximated by a thermal plasma emission model with a temperature of T=8.2 keV. INTEGRAL was used to image the cluster emission in the hard energy band. The cluster is only marginally detectable ~1.6sigma in the 44-107 keV energy band; however, the raw flux in this band is consistent with the previous results from Beppo-SAX and RXTE observatories. We"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0802.3742","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/0802.3742/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":"0802.3742","created_at":"2026-07-04T17:09:34.761387+00:00"},{"alias_kind":"arxiv_version","alias_value":"0802.3742v3","created_at":"2026-07-04T17:09:34.761387+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0802.3742","created_at":"2026-07-04T17:09:34.761387+00:00"},{"alias_kind":"pith_short_12","alias_value":"ITNCX352HR7O","created_at":"2026-07-04T17:09:34.761387+00:00"},{"alias_kind":"pith_short_16","alias_value":"ITNCX352HR7O2N5L","created_at":"2026-07-04T17:09:34.761387+00:00"},{"alias_kind":"pith_short_8","alias_value":"ITNCX352","created_at":"2026-07-04T17:09:34.761387+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/ITNCX352HR7O2N5LTO3UD2NVSU","json":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU.json","graph_json":"https://pith.science/api/pith-number/ITNCX352HR7O2N5LTO3UD2NVSU/graph.json","events_json":"https://pith.science/api/pith-number/ITNCX352HR7O2N5LTO3UD2NVSU/events.json","paper":"https://pith.science/paper/ITNCX352"},"agent_actions":{"view_html":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU","download_json":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU.json","view_paper":"https://pith.science/paper/ITNCX352","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0802.3742&json=true","fetch_graph":"https://pith.science/api/pith-number/ITNCX352HR7O2N5LTO3UD2NVSU/graph.json","fetch_events":"https://pith.science/api/pith-number/ITNCX352HR7O2N5LTO3UD2NVSU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU/action/storage_attestation","attest_author":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU/action/author_attestation","sign_citation":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU/action/citation_signature","submit_replication":"https://pith.science/pith/ITNCX352HR7O2N5LTO3UD2NVSU/action/replication_record"}},"created_at":"2026-07-04T17:09:34.761387+00:00","updated_at":"2026-07-04T17:09:34.761387+00:00"}