{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:JJPSOB735G2ZGTE4MHQOBAIA2C","short_pith_number":"pith:JJPSOB73","schema_version":"1.0","canonical_sha256":"4a5f2707fbe9b5934c9c61e0e08100d0af93dccf520e85ce51e3b157e9721a4e","source":{"kind":"arxiv","id":"1308.6091","version":1},"attestation_state":"computed","paper":{"title":"Suzaku Studies of Luminosity-Dependent Changes in the Low-Mass X-ray Binary Aquila X-1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hirofumi Noda, Hiromitsu Takahashi, Kazuhiro Nakazawa, Kazuo Makishima, Ko Ono, Masaru Matsuoka, Shinya Yamada, Shunsuke Torii, Soki Sakurai, Zhongli Zhang","submitted_at":"2013-08-28T08:32:38Z","abstract_excerpt":"The neutron-star Low-Mass X-ray Binary Aquila X-1 was observed by Suzaku for seven times, from 2007 September 28 to October 30. The observations successfully traced an outburst decay in which the source luminosity decreased almost monotonically from $\\sim 10^{37}$ erg s$^{-1}$ to $\\sim 10^{34}$ erg s$^{-1}$, by $\\sim 3$ orders of magnitude. To investigate luminosity-dependent changes in the accretion geometry, five of the seven data sets with a typical exposure of $\\sim 18$ ks each were analyzed; the other two were utilized in a previous work \\citep{Sakurai2012}. The source was detected up to "},"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":"1308.6091","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-08-28T08:32:38Z","cross_cats_sorted":[],"title_canon_sha256":"7cf4893b5d93addb3efb11bed89addddbb4ea7e8859232d21c45dba07426fbae","abstract_canon_sha256":"6a25a31bee1f94cb697a27b98338e564c50df0fc3daf67912b80f4713a9fe039"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:57.595561Z","signature_b64":"aI2w0Q2Ehua9HJvIEJHEdu6y9y0SOGPPN8mWC/Bg+947WgU5slb/+vNvK3pWWrP3MIO0zttKmBB3FrQc4+y2DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a5f2707fbe9b5934c9c61e0e08100d0af93dccf520e85ce51e3b157e9721a4e","last_reissued_at":"2026-05-18T01:47:57.594914Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:57.594914Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Suzaku Studies of Luminosity-Dependent Changes in the Low-Mass X-ray Binary Aquila X-1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hirofumi Noda, Hiromitsu Takahashi, Kazuhiro Nakazawa, Kazuo Makishima, Ko Ono, Masaru Matsuoka, Shinya Yamada, Shunsuke Torii, Soki Sakurai, Zhongli Zhang","submitted_at":"2013-08-28T08:32:38Z","abstract_excerpt":"The neutron-star Low-Mass X-ray Binary Aquila X-1 was observed by Suzaku for seven times, from 2007 September 28 to October 30. The observations successfully traced an outburst decay in which the source luminosity decreased almost monotonically from $\\sim 10^{37}$ erg s$^{-1}$ to $\\sim 10^{34}$ erg s$^{-1}$, by $\\sim 3$ orders of magnitude. To investigate luminosity-dependent changes in the accretion geometry, five of the seven data sets with a typical exposure of $\\sim 18$ ks each were analyzed; the other two were utilized in a previous work \\citep{Sakurai2012}. The source was detected up to "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.6091","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":"1308.6091","created_at":"2026-05-18T01:47:57.595003+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.6091v1","created_at":"2026-05-18T01:47:57.595003+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.6091","created_at":"2026-05-18T01:47:57.595003+00:00"},{"alias_kind":"pith_short_12","alias_value":"JJPSOB735G2Z","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_16","alias_value":"JJPSOB735G2ZGTE4","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_8","alias_value":"JJPSOB73","created_at":"2026-05-18T12:27:49.015174+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/JJPSOB735G2ZGTE4MHQOBAIA2C","json":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C.json","graph_json":"https://pith.science/api/pith-number/JJPSOB735G2ZGTE4MHQOBAIA2C/graph.json","events_json":"https://pith.science/api/pith-number/JJPSOB735G2ZGTE4MHQOBAIA2C/events.json","paper":"https://pith.science/paper/JJPSOB73"},"agent_actions":{"view_html":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C","download_json":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C.json","view_paper":"https://pith.science/paper/JJPSOB73","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.6091&json=true","fetch_graph":"https://pith.science/api/pith-number/JJPSOB735G2ZGTE4MHQOBAIA2C/graph.json","fetch_events":"https://pith.science/api/pith-number/JJPSOB735G2ZGTE4MHQOBAIA2C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C/action/storage_attestation","attest_author":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C/action/author_attestation","sign_citation":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C/action/citation_signature","submit_replication":"https://pith.science/pith/JJPSOB735G2ZGTE4MHQOBAIA2C/action/replication_record"}},"created_at":"2026-05-18T01:47:57.595003+00:00","updated_at":"2026-05-18T01:47:57.595003+00:00"}