{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:P23VYBFCDFTKZ4U32GXUTZ4FRD","short_pith_number":"pith:P23VYBFC","schema_version":"1.0","canonical_sha256":"7eb75c04a21966acf29bd1af49e78588d3744a3d3952ddf60dc7202c50836ac0","source":{"kind":"arxiv","id":"1308.4567","version":2},"attestation_state":"computed","paper":{"title":"Is the `disappearance' of low-frequency QPOs in the power spectra a general phenomenon for Disk-Jet symbiosis?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Nandi, Radhika. D, S. Seetha","submitted_at":"2013-08-21T13:25:18Z","abstract_excerpt":"One of the best possible ways to look for disk-Jet symbiosis in galactic Black Holes is to study the correlation between X-ray and radio emissions. Beyond this study, is there any alternative way to trace the symbiosis? To answer, we investigated the X-ray features of few black hole candidates based on the archival data of PCA/RXTE. We found evidences of `disappearance' of QPOs in the power density spectra and subsequent spectral softening of the energy spectra during the radio flares (i.e., `transient' Jets). We delve deep into the nature of the accretion dynamics to understand the disk-Jet s"},"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":"1308.4567","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-08-21T13:25:18Z","cross_cats_sorted":[],"title_canon_sha256":"1ffe6421f6528f97b43ae5782a0e9864b4efc3b2ffe6378059c02361d6aa5d58","abstract_canon_sha256":"0367446253fb79c38dc21bd309af2cd23a2ae57eca2ce1874cea160745fe62f3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:13:57.671571Z","signature_b64":"ZND4bX0JyBjWCIXzHQbO2H+QTIgIOThAuF2xDG62snq1NG0z31ZsvVPlIUCThCJF4JP+ES1PqbZ+CrmLlskDCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7eb75c04a21966acf29bd1af49e78588d3744a3d3952ddf60dc7202c50836ac0","last_reissued_at":"2026-05-18T03:13:57.670608Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:13:57.670608Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Is the `disappearance' of low-frequency QPOs in the power spectra a general phenomenon for Disk-Jet symbiosis?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Nandi, Radhika. D, S. Seetha","submitted_at":"2013-08-21T13:25:18Z","abstract_excerpt":"One of the best possible ways to look for disk-Jet symbiosis in galactic Black Holes is to study the correlation between X-ray and radio emissions. Beyond this study, is there any alternative way to trace the symbiosis? To answer, we investigated the X-ray features of few black hole candidates based on the archival data of PCA/RXTE. We found evidences of `disappearance' of QPOs in the power density spectra and subsequent spectral softening of the energy spectra during the radio flares (i.e., `transient' Jets). We delve deep into the nature of the accretion dynamics to understand the disk-Jet s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.4567","kind":"arxiv","version":2},"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":"1308.4567","created_at":"2026-05-18T03:13:57.670766+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.4567v2","created_at":"2026-05-18T03:13:57.670766+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.4567","created_at":"2026-05-18T03:13:57.670766+00:00"},{"alias_kind":"pith_short_12","alias_value":"P23VYBFCDFTK","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"P23VYBFCDFTKZ4U3","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"P23VYBFC","created_at":"2026-05-18T12:27:54.935989+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/P23VYBFCDFTKZ4U32GXUTZ4FRD","json":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD.json","graph_json":"https://pith.science/api/pith-number/P23VYBFCDFTKZ4U32GXUTZ4FRD/graph.json","events_json":"https://pith.science/api/pith-number/P23VYBFCDFTKZ4U32GXUTZ4FRD/events.json","paper":"https://pith.science/paper/P23VYBFC"},"agent_actions":{"view_html":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD","download_json":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD.json","view_paper":"https://pith.science/paper/P23VYBFC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.4567&json=true","fetch_graph":"https://pith.science/api/pith-number/P23VYBFCDFTKZ4U32GXUTZ4FRD/graph.json","fetch_events":"https://pith.science/api/pith-number/P23VYBFCDFTKZ4U32GXUTZ4FRD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD/action/storage_attestation","attest_author":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD/action/author_attestation","sign_citation":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD/action/citation_signature","submit_replication":"https://pith.science/pith/P23VYBFCDFTKZ4U32GXUTZ4FRD/action/replication_record"}},"created_at":"2026-05-18T03:13:57.670766+00:00","updated_at":"2026-05-18T03:13:57.670766+00:00"}