{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:J5Y574N33C2IES5SJKACBLBT6C","short_pith_number":"pith:J5Y574N3","schema_version":"1.0","canonical_sha256":"4f71dff1bbd8b4824bb24a8020ac33f094169ba241db72771f62e903634b8e10","source":{"kind":"arxiv","id":"1301.1112","version":1},"attestation_state":"computed","paper":{"title":"Timing and Spectral properties of Be/X-ray pulsar EXO 2030+375 during a Type I outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"(2) Raman Research Institute, 3), (3) Joint Astronomy Programme, Bangalore, Biswajit Paul (2)((1) Astronomy & Astrophysics Division, Chandreyee Maitra (2, C. V. Raman Avenue, Gaurava K. Jaisawal (1), India, India), Indian Institute of Science, Physical Research Laboratory, Sachindra Naik (1), Sadashivnagar","submitted_at":"2013-01-07T05:05:54Z","abstract_excerpt":"We present results from a study of broadband timing and spectral properties of EXO 2030+375 using a Suzaku observation. Pulsations with a period of 41.41 s and strong energy dependent pulse profiles were clearly detected up to ~100 keV. Narrow dips are seen in the profiles up to ~70 keV. Presence of prominent dips at several phases in the profiles up to such high energy ranges were not seen before. At higher energies, these dips gradually disappeared and the profile appeared single-peaked. The 1.0-200.0 keV broad-band spectrum is found to be well described by a partial covering high energy cut"},"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":"1301.1112","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-07T05:05:54Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"f5a2ffb19620b81600b1267780061aba0499bfa968d6eec7ad1074c5263e4a80","abstract_canon_sha256":"e19be3078b3d9f9a0cbc71f30fb3038ad74121fa5a2f823975b6d050d4cd04aa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:34:27.066733Z","signature_b64":"9N9r+Qnk2hGkw16gz9jQFvdrpphFubgPe+e+kQ95jF1l8jDsNm5xsxyyjNFs0di4yc2YvyM4vdKdpRNZd/AlAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4f71dff1bbd8b4824bb24a8020ac33f094169ba241db72771f62e903634b8e10","last_reissued_at":"2026-05-18T03:34:27.066235Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:34:27.066235Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Timing and Spectral properties of Be/X-ray pulsar EXO 2030+375 during a Type I outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"(2) Raman Research Institute, 3), (3) Joint Astronomy Programme, Bangalore, Biswajit Paul (2)((1) Astronomy & Astrophysics Division, Chandreyee Maitra (2, C. V. Raman Avenue, Gaurava K. Jaisawal (1), India, India), Indian Institute of Science, Physical Research Laboratory, Sachindra Naik (1), Sadashivnagar","submitted_at":"2013-01-07T05:05:54Z","abstract_excerpt":"We present results from a study of broadband timing and spectral properties of EXO 2030+375 using a Suzaku observation. Pulsations with a period of 41.41 s and strong energy dependent pulse profiles were clearly detected up to ~100 keV. Narrow dips are seen in the profiles up to ~70 keV. Presence of prominent dips at several phases in the profiles up to such high energy ranges were not seen before. At higher energies, these dips gradually disappeared and the profile appeared single-peaked. The 1.0-200.0 keV broad-band spectrum is found to be well described by a partial covering high energy cut"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.1112","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":"1301.1112","created_at":"2026-05-18T03:34:27.066305+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.1112v1","created_at":"2026-05-18T03:34:27.066305+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.1112","created_at":"2026-05-18T03:34:27.066305+00:00"},{"alias_kind":"pith_short_12","alias_value":"J5Y574N33C2I","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_16","alias_value":"J5Y574N33C2IES5S","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_8","alias_value":"J5Y574N3","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/J5Y574N33C2IES5SJKACBLBT6C","json":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C.json","graph_json":"https://pith.science/api/pith-number/J5Y574N33C2IES5SJKACBLBT6C/graph.json","events_json":"https://pith.science/api/pith-number/J5Y574N33C2IES5SJKACBLBT6C/events.json","paper":"https://pith.science/paper/J5Y574N3"},"agent_actions":{"view_html":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C","download_json":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C.json","view_paper":"https://pith.science/paper/J5Y574N3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.1112&json=true","fetch_graph":"https://pith.science/api/pith-number/J5Y574N33C2IES5SJKACBLBT6C/graph.json","fetch_events":"https://pith.science/api/pith-number/J5Y574N33C2IES5SJKACBLBT6C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C/action/storage_attestation","attest_author":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C/action/author_attestation","sign_citation":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C/action/citation_signature","submit_replication":"https://pith.science/pith/J5Y574N33C2IES5SJKACBLBT6C/action/replication_record"}},"created_at":"2026-05-18T03:34:27.066305+00:00","updated_at":"2026-05-18T03:34:27.066305+00:00"}