{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:LPUQPHVKF34NJI7JKB26DACPQF","short_pith_number":"pith:LPUQPHVK","schema_version":"1.0","canonical_sha256":"5be9079eaa2ef8d4a3e95075e1804f814ca95b4c822e07c78a8a8799b3ea6ecf","source":{"kind":"arxiv","id":"1409.6283","version":1},"attestation_state":"computed","paper":{"title":"Energy Dependent Time Delays of kHz Oscillations due to Thermal Comptonization","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Nagendra Kumar, Ranjeev Misra","submitted_at":"2014-09-22T19:09:40Z","abstract_excerpt":"We study the energy dependent photon variability from a thermal Comptonizing plasma that is oscillating at kHz frequencies. In particular, we solve the linearised time dependent Kompaneets equation and consider the oscillatory perturbation to be either in the soft photon source or in the heating rate of the plasma. For each case, we self consistently consider the energy balance of the plasma and the soft photon source. The model incorporates the possibility of a fraction of the Comptonized photons impinging back into the soft photon source. We find that when the oscillation is due to the soft "},"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":"1409.6283","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-09-22T19:09:40Z","cross_cats_sorted":[],"title_canon_sha256":"328d581afa739829686aa55a14f6b62cc95283c2ff4d3e3f3925d7ba1ec97dab","abstract_canon_sha256":"2991d45fd68feddc4ec30caf52ee69c5693166bec077c9ed7e5244ce68e2bd82"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:59.041743Z","signature_b64":"EWdwO0jYEdXZGrwPtmmIpP4CCqTBALx4g+ywMiwRnQe0p4tx9hsDVCEeFhcwOUKty1EfjOge0lZQRjYGGX+dBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5be9079eaa2ef8d4a3e95075e1804f814ca95b4c822e07c78a8a8799b3ea6ecf","last_reissued_at":"2026-05-18T01:41:59.041148Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:59.041148Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Energy Dependent Time Delays of kHz Oscillations due to Thermal Comptonization","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Nagendra Kumar, Ranjeev Misra","submitted_at":"2014-09-22T19:09:40Z","abstract_excerpt":"We study the energy dependent photon variability from a thermal Comptonizing plasma that is oscillating at kHz frequencies. In particular, we solve the linearised time dependent Kompaneets equation and consider the oscillatory perturbation to be either in the soft photon source or in the heating rate of the plasma. For each case, we self consistently consider the energy balance of the plasma and the soft photon source. The model incorporates the possibility of a fraction of the Comptonized photons impinging back into the soft photon source. We find that when the oscillation is due to the soft "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.6283","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":"1409.6283","created_at":"2026-05-18T01:41:59.041231+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.6283v1","created_at":"2026-05-18T01:41:59.041231+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.6283","created_at":"2026-05-18T01:41:59.041231+00:00"},{"alias_kind":"pith_short_12","alias_value":"LPUQPHVKF34N","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_16","alias_value":"LPUQPHVKF34NJI7J","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_8","alias_value":"LPUQPHVK","created_at":"2026-05-18T12:28:38.356838+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.17344","citing_title":"Understanding corona and disk evolution in black hole X-ray binaries through a comprehensive study of their broadband variability and QPO characteristics","ref_index":60,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF","json":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF.json","graph_json":"https://pith.science/api/pith-number/LPUQPHVKF34NJI7JKB26DACPQF/graph.json","events_json":"https://pith.science/api/pith-number/LPUQPHVKF34NJI7JKB26DACPQF/events.json","paper":"https://pith.science/paper/LPUQPHVK"},"agent_actions":{"view_html":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF","download_json":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF.json","view_paper":"https://pith.science/paper/LPUQPHVK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.6283&json=true","fetch_graph":"https://pith.science/api/pith-number/LPUQPHVKF34NJI7JKB26DACPQF/graph.json","fetch_events":"https://pith.science/api/pith-number/LPUQPHVKF34NJI7JKB26DACPQF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF/action/storage_attestation","attest_author":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF/action/author_attestation","sign_citation":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF/action/citation_signature","submit_replication":"https://pith.science/pith/LPUQPHVKF34NJI7JKB26DACPQF/action/replication_record"}},"created_at":"2026-05-18T01:41:59.041231+00:00","updated_at":"2026-05-18T01:41:59.041231+00:00"}