{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:EPK7BEMPINDQMSVHT4WTPUOBGA","short_pith_number":"pith:EPK7BEMP","schema_version":"1.0","canonical_sha256":"23d5f0918f4347064aa79f2d37d1c130254ebb44825cf99caf47465d3847f21f","source":{"kind":"arxiv","id":"1310.4338","version":1},"attestation_state":"computed","paper":{"title":"Alternating lags of QPO harmonics : A Generic model and its application to the 67 millihertz QPO of GRS 1915+105","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ranjeev Misra, Soma Mandal","submitted_at":"2013-10-16T11:53:23Z","abstract_excerpt":"A generic model for alternating lags in QPO harmonics is presented where variations in the photon spectrum are caused by oscillations in two parameters that characterize the spectrum. It is further assumed that variations in one of the parameters is linearly driven by variations in the other after a time delay $t_d$. It is shown that alternating lags will be observed for a range of $t_d$ values. A phenomenological model based on this generic one is developed which can explain the amplitude and phase lag variation with energy of the fundamental and the next three harmonics of the 67 mHz QPO obs"},"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":"1310.4338","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-16T11:53:23Z","cross_cats_sorted":[],"title_canon_sha256":"af2fa69a9d0a87cf0549cc7ec2a961cc6891650982fc1a35813e1cedf32fcd5d","abstract_canon_sha256":"5e7eebc098024f3b05b05d7bed3d702230bdb04ab900bca8b5395f12ea42e824"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:06:12.786864Z","signature_b64":"0VpHDkWmST097ETy1uRprgS/V81k5RHpW6wPNgpRR388M0e2E26Tgl0ucnUJPcv+4/SBZ3MoQFANr4GeuAOSBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23d5f0918f4347064aa79f2d37d1c130254ebb44825cf99caf47465d3847f21f","last_reissued_at":"2026-05-18T03:06:12.786234Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:06:12.786234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Alternating lags of QPO harmonics : A Generic model and its application to the 67 millihertz QPO of GRS 1915+105","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ranjeev Misra, Soma Mandal","submitted_at":"2013-10-16T11:53:23Z","abstract_excerpt":"A generic model for alternating lags in QPO harmonics is presented where variations in the photon spectrum are caused by oscillations in two parameters that characterize the spectrum. It is further assumed that variations in one of the parameters is linearly driven by variations in the other after a time delay $t_d$. It is shown that alternating lags will be observed for a range of $t_d$ values. A phenomenological model based on this generic one is developed which can explain the amplitude and phase lag variation with energy of the fundamental and the next three harmonics of the 67 mHz QPO obs"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4338","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":"1310.4338","created_at":"2026-05-18T03:06:12.786326+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.4338v1","created_at":"2026-05-18T03:06:12.786326+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.4338","created_at":"2026-05-18T03:06:12.786326+00:00"},{"alias_kind":"pith_short_12","alias_value":"EPK7BEMPINDQ","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_16","alias_value":"EPK7BEMPINDQMSVH","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_8","alias_value":"EPK7BEMP","created_at":"2026-05-18T12:27:43.054852+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":69,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA","json":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA.json","graph_json":"https://pith.science/api/pith-number/EPK7BEMPINDQMSVHT4WTPUOBGA/graph.json","events_json":"https://pith.science/api/pith-number/EPK7BEMPINDQMSVHT4WTPUOBGA/events.json","paper":"https://pith.science/paper/EPK7BEMP"},"agent_actions":{"view_html":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA","download_json":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA.json","view_paper":"https://pith.science/paper/EPK7BEMP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.4338&json=true","fetch_graph":"https://pith.science/api/pith-number/EPK7BEMPINDQMSVHT4WTPUOBGA/graph.json","fetch_events":"https://pith.science/api/pith-number/EPK7BEMPINDQMSVHT4WTPUOBGA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA/action/storage_attestation","attest_author":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA/action/author_attestation","sign_citation":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA/action/citation_signature","submit_replication":"https://pith.science/pith/EPK7BEMPINDQMSVHT4WTPUOBGA/action/replication_record"}},"created_at":"2026-05-18T03:06:12.786326+00:00","updated_at":"2026-05-18T03:06:12.786326+00:00"}