{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:DWRMWKK5HE4NXIDOVODHUOAA7V","short_pith_number":"pith:DWRMWKK5","schema_version":"1.0","canonical_sha256":"1da2cb295d3938dba06eab867a3800fd7c7d51c35bf7e26a10b9dd5de7fd6bb8","source":{"kind":"arxiv","id":"1309.3672","version":1},"attestation_state":"computed","paper":{"title":"Suzaku observations of the type 2 QSO in the central galaxy of the Phoenix cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Hiroshi Nakajima, Hiroshi Tsunemi, Katsuji Koyama, Kiyoshi Hayashida, Naohisa Anabuki, Shutaro Ueda","submitted_at":"2013-09-14T14:14:07Z","abstract_excerpt":"We report the \\Suzaku/XIS and HXD and \\Chandra/ACIS-I results on the X-ray spectra of the Phoenix cluster at the redshift $z=0.596$. The spectrum of the intracluster medium (ICM) is well-reproduced with the emissions from a low temperature ($\\sim3.0$\\,keV and $\\sim0.76$\\,solar) and a high temperature ($\\sim11$\\,keV and $\\sim0.33$\\,solar) plasmas; the former is localized at the cluster core, while the latter distributes over the cluster. In addition to these ICM emissions, a strongly absorbed power-law component is found, which is due to an active galactic nucleus (AGN) in the cluster center. T"},"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":"1309.3672","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-09-14T14:14:07Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"ad13e1ad757a1a6d7995c8c11330313172539e75d637aa7d503f17155dd0cf14","abstract_canon_sha256":"af1fba62bd8acb6f7de8af2b4cbf443d85cac9242028e761c45dc7ff5c92e4f3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:41.755978Z","signature_b64":"BTi4/3EzUsu/xg6riXwI+4Cikczpsn7sTeaR//Rxu7kE6rvJ4jUe43gR0B8E49p5WTj+w5IPBKMHkUJkf9IhAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1da2cb295d3938dba06eab867a3800fd7c7d51c35bf7e26a10b9dd5de7fd6bb8","last_reissued_at":"2026-05-18T01:47:41.755276Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:41.755276Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Suzaku observations of the type 2 QSO in the central galaxy of the Phoenix cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Hiroshi Nakajima, Hiroshi Tsunemi, Katsuji Koyama, Kiyoshi Hayashida, Naohisa Anabuki, Shutaro Ueda","submitted_at":"2013-09-14T14:14:07Z","abstract_excerpt":"We report the \\Suzaku/XIS and HXD and \\Chandra/ACIS-I results on the X-ray spectra of the Phoenix cluster at the redshift $z=0.596$. The spectrum of the intracluster medium (ICM) is well-reproduced with the emissions from a low temperature ($\\sim3.0$\\,keV and $\\sim0.76$\\,solar) and a high temperature ($\\sim11$\\,keV and $\\sim0.33$\\,solar) plasmas; the former is localized at the cluster core, while the latter distributes over the cluster. In addition to these ICM emissions, a strongly absorbed power-law component is found, which is due to an active galactic nucleus (AGN) in the cluster center. T"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.3672","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":"1309.3672","created_at":"2026-05-18T01:47:41.755368+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.3672v1","created_at":"2026-05-18T01:47:41.755368+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.3672","created_at":"2026-05-18T01:47:41.755368+00:00"},{"alias_kind":"pith_short_12","alias_value":"DWRMWKK5HE4N","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_16","alias_value":"DWRMWKK5HE4NXIDO","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_8","alias_value":"DWRMWKK5","created_at":"2026-05-18T12:27:43.054852+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/DWRMWKK5HE4NXIDOVODHUOAA7V","json":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V.json","graph_json":"https://pith.science/api/pith-number/DWRMWKK5HE4NXIDOVODHUOAA7V/graph.json","events_json":"https://pith.science/api/pith-number/DWRMWKK5HE4NXIDOVODHUOAA7V/events.json","paper":"https://pith.science/paper/DWRMWKK5"},"agent_actions":{"view_html":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V","download_json":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V.json","view_paper":"https://pith.science/paper/DWRMWKK5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.3672&json=true","fetch_graph":"https://pith.science/api/pith-number/DWRMWKK5HE4NXIDOVODHUOAA7V/graph.json","fetch_events":"https://pith.science/api/pith-number/DWRMWKK5HE4NXIDOVODHUOAA7V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V/action/storage_attestation","attest_author":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V/action/author_attestation","sign_citation":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V/action/citation_signature","submit_replication":"https://pith.science/pith/DWRMWKK5HE4NXIDOVODHUOAA7V/action/replication_record"}},"created_at":"2026-05-18T01:47:41.755368+00:00","updated_at":"2026-05-18T01:47:41.755368+00:00"}