{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:MZZJDOQLRINOVQA5YXDQGKNEHZ","short_pith_number":"pith:MZZJDOQL","schema_version":"1.0","canonical_sha256":"667291ba0b8a1aeac01dc5c70329a43e462cf3cababdcdb52a12a3d668bcfa77","source":{"kind":"arxiv","id":"1710.10901","version":1},"attestation_state":"computed","paper":{"title":"On one-parametric formula relating the frequencies of twin-peak quasi-periodic oscillations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Eva \\v{S}r\\'amkov\\'a, Gabriel T\\\"or\\\"ok, Ji\\v{r}\\'i Hor\\'ak, Kate\\v{r}ina Goluchov\\'a, Martin Urbanec, Pavel Bakala","submitted_at":"2017-10-30T12:35:44Z","abstract_excerpt":"Twin-peak quasi-periodic oscillations (QPOs) are observed in several low-mass X-ray binary systems containing neutron stars (NSs). Timing analysis of X-ray fluxes of more than dozen of such systems reveals remarkable correlations between the frequencies of two characteristic peaks present in the power density spectra. The individual correlations clearly differ, but they roughly follow a common individual pattern. High values of measured QPO frequencies and strong modulation of the X-ray flux both suggest that the observed correlations are connected to orbital motion in the innermost part of an"},"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":"1710.10901","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-30T12:35:44Z","cross_cats_sorted":[],"title_canon_sha256":"cc0d10cc8280ea528cf9e8e803a09b3591e94d9634d24fc48b6b96963fec5b39","abstract_canon_sha256":"2cfb8f43632a45bad7c6cd9e7ab9ba6496d534acf3dd0d14d1eb2b1f5fb8d72b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:27:18.481965Z","signature_b64":"it1Alpj50S5dm68heQ65HHskP+RKJd772dzJ/IcfYimbElsIqkBMOIFkS/I0wdc3Kl6bTg6Gr5UYiboac62uAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"667291ba0b8a1aeac01dc5c70329a43e462cf3cababdcdb52a12a3d668bcfa77","last_reissued_at":"2026-05-18T00:27:18.481562Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:27:18.481562Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On one-parametric formula relating the frequencies of twin-peak quasi-periodic oscillations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Eva \\v{S}r\\'amkov\\'a, Gabriel T\\\"or\\\"ok, Ji\\v{r}\\'i Hor\\'ak, Kate\\v{r}ina Goluchov\\'a, Martin Urbanec, Pavel Bakala","submitted_at":"2017-10-30T12:35:44Z","abstract_excerpt":"Twin-peak quasi-periodic oscillations (QPOs) are observed in several low-mass X-ray binary systems containing neutron stars (NSs). Timing analysis of X-ray fluxes of more than dozen of such systems reveals remarkable correlations between the frequencies of two characteristic peaks present in the power density spectra. The individual correlations clearly differ, but they roughly follow a common individual pattern. High values of measured QPO frequencies and strong modulation of the X-ray flux both suggest that the observed correlations are connected to orbital motion in the innermost part of an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.10901","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":"1710.10901","created_at":"2026-05-18T00:27:18.481611+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.10901v1","created_at":"2026-05-18T00:27:18.481611+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.10901","created_at":"2026-05-18T00:27:18.481611+00:00"},{"alias_kind":"pith_short_12","alias_value":"MZZJDOQLRINO","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"MZZJDOQLRINOVQA5","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"MZZJDOQL","created_at":"2026-05-18T12:31:31.346846+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/MZZJDOQLRINOVQA5YXDQGKNEHZ","json":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ.json","graph_json":"https://pith.science/api/pith-number/MZZJDOQLRINOVQA5YXDQGKNEHZ/graph.json","events_json":"https://pith.science/api/pith-number/MZZJDOQLRINOVQA5YXDQGKNEHZ/events.json","paper":"https://pith.science/paper/MZZJDOQL"},"agent_actions":{"view_html":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ","download_json":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ.json","view_paper":"https://pith.science/paper/MZZJDOQL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.10901&json=true","fetch_graph":"https://pith.science/api/pith-number/MZZJDOQLRINOVQA5YXDQGKNEHZ/graph.json","fetch_events":"https://pith.science/api/pith-number/MZZJDOQLRINOVQA5YXDQGKNEHZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ/action/storage_attestation","attest_author":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ/action/author_attestation","sign_citation":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ/action/citation_signature","submit_replication":"https://pith.science/pith/MZZJDOQLRINOVQA5YXDQGKNEHZ/action/replication_record"}},"created_at":"2026-05-18T00:27:18.481611+00:00","updated_at":"2026-05-18T00:27:18.481611+00:00"}