{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:2KX2QPANVU2RXJ4G63SE23F4HB","short_pith_number":"pith:2KX2QPAN","schema_version":"1.0","canonical_sha256":"d2afa83c0dad351ba786f6e44d6cbc3852d0a6ea6f4ddbf13d712d86cf91b6ad","source":{"kind":"arxiv","id":"1303.3834","version":2},"attestation_state":"computed","paper":{"title":"Towards modeling quasi-periodic oscillations of microquasars with oscillating slender tori","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"E. Sramkova, F. H. Vincent, G. P. Mazur, G. Torok, M. A. Abramowicz, M. Johansson, P. Bakala","submitted_at":"2013-03-15T17:18:54Z","abstract_excerpt":"Context. One of the often discussed models for X-ray binaries high-frequency quasi-periodic oscillations is the oscillating torus model that considers oscillation modes of slender accretion tori. Aims. Here, we aim at developing this model by considering the observable signature of an optically thick slender accretion torus subject to simple periodic deformations. Methods. We compute light curves and power spectra of a slender accretion torus subject to simple periodic deformations: vertical or radial translation, rotation, expansion and shear. Results. We show that different types of deformat"},"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":"1303.3834","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-03-15T17:18:54Z","cross_cats_sorted":[],"title_canon_sha256":"e991417b7d1b3a44738e5e35e63f95a7b0c1235b0c25cb4c3928a99a6f66e5ef","abstract_canon_sha256":"cae0033d96469bbd2f299644d8a095aa7e12510e0696ed9408db07e760842414"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:06.777437Z","signature_b64":"3nLeTMIhgXULxWAsPvJPnCsQofOU9mmRBs1ZIg+rop9DApNPIR0OyB7DjDO3LXjipPN417ZLCT9eDMlTEiHEAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d2afa83c0dad351ba786f6e44d6cbc3852d0a6ea6f4ddbf13d712d86cf91b6ad","last_reissued_at":"2026-05-18T01:51:06.776742Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:06.776742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Towards modeling quasi-periodic oscillations of microquasars with oscillating slender tori","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"E. Sramkova, F. H. Vincent, G. P. Mazur, G. Torok, M. A. Abramowicz, M. Johansson, P. Bakala","submitted_at":"2013-03-15T17:18:54Z","abstract_excerpt":"Context. One of the often discussed models for X-ray binaries high-frequency quasi-periodic oscillations is the oscillating torus model that considers oscillation modes of slender accretion tori. Aims. Here, we aim at developing this model by considering the observable signature of an optically thick slender accretion torus subject to simple periodic deformations. Methods. We compute light curves and power spectra of a slender accretion torus subject to simple periodic deformations: vertical or radial translation, rotation, expansion and shear. Results. We show that different types of deformat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.3834","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":"1303.3834","created_at":"2026-05-18T01:51:06.776842+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.3834v2","created_at":"2026-05-18T01:51:06.776842+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.3834","created_at":"2026-05-18T01:51:06.776842+00:00"},{"alias_kind":"pith_short_12","alias_value":"2KX2QPANVU2R","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"2KX2QPANVU2RXJ4G","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"2KX2QPAN","created_at":"2026-05-18T12:27:30.460161+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/2KX2QPANVU2RXJ4G63SE23F4HB","json":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB.json","graph_json":"https://pith.science/api/pith-number/2KX2QPANVU2RXJ4G63SE23F4HB/graph.json","events_json":"https://pith.science/api/pith-number/2KX2QPANVU2RXJ4G63SE23F4HB/events.json","paper":"https://pith.science/paper/2KX2QPAN"},"agent_actions":{"view_html":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB","download_json":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB.json","view_paper":"https://pith.science/paper/2KX2QPAN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.3834&json=true","fetch_graph":"https://pith.science/api/pith-number/2KX2QPANVU2RXJ4G63SE23F4HB/graph.json","fetch_events":"https://pith.science/api/pith-number/2KX2QPANVU2RXJ4G63SE23F4HB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB/action/storage_attestation","attest_author":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB/action/author_attestation","sign_citation":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB/action/citation_signature","submit_replication":"https://pith.science/pith/2KX2QPANVU2RXJ4G63SE23F4HB/action/replication_record"}},"created_at":"2026-05-18T01:51:06.776842+00:00","updated_at":"2026-05-18T01:51:06.776842+00:00"}