{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:QTZCQA5XFAHHVSPBHHHPDGJIAB","short_pith_number":"pith:QTZCQA5X","schema_version":"1.0","canonical_sha256":"84f22803b7280e7ac9e139cef19928005ee19af6d917335fdc46d9c8e8963d02","source":{"kind":"arxiv","id":"1509.05867","version":3},"attestation_state":"computed","paper":{"title":"Spectral and Temporal Properties of MAXI J1836-194 during 2011 Outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Molla, A. Jana, D. Chatterjee, D. Debnath, S. K. Chakrabarti, S. Mondal","submitted_at":"2015-09-19T10:21:59Z","abstract_excerpt":"We study black hole candidate (BHC) MAXI~J1836-194 during its 2011 outburst with Two Component Advective Flow (TCAF) model using RXTE/PCU2 data in $2.5-25$~keV band. From spectral fit, accretion flow parameters such as Keplerian disk rate ($\\dot{m_d}$), sub-Keplerian halo rate ($\\dot{m_h}$), shock location ($X_{s}$) and compression ratio (R) are extracted directly. During the entire phase of the outburst, quasi-periodic oscillations (QPOs) are observed sporadically. From the nature of the variation of accretion rate ratio (ARR=$\\dot{m_h}$ / $\\dot{m_d}$) and QPOs, entire period of the outburst "},"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":"1509.05867","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-09-19T10:21:59Z","cross_cats_sorted":[],"title_canon_sha256":"d2e9de011be85d27894b77df86bb2ab1a536d26db2305ea32bf1ae14e597355b","abstract_canon_sha256":"ccec69a1f3f88fa57893a2fcc3f690ea0a1a036a73c96cf20ba84e4508d0e108"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:07.969214Z","signature_b64":"YdR68Jh6BTD/T2lafrMLxbyDzpdxhnw5OYpArYeWTAvoD3CgrEgKJ7X6vfVjEKb1FKxUmV3C+touzj52fMeYDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"84f22803b7280e7ac9e139cef19928005ee19af6d917335fdc46d9c8e8963d02","last_reissued_at":"2026-05-18T01:17:07.968509Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:07.968509Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectral and Temporal Properties of MAXI J1836-194 during 2011 Outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Molla, A. Jana, D. Chatterjee, D. Debnath, S. K. Chakrabarti, S. Mondal","submitted_at":"2015-09-19T10:21:59Z","abstract_excerpt":"We study black hole candidate (BHC) MAXI~J1836-194 during its 2011 outburst with Two Component Advective Flow (TCAF) model using RXTE/PCU2 data in $2.5-25$~keV band. From spectral fit, accretion flow parameters such as Keplerian disk rate ($\\dot{m_d}$), sub-Keplerian halo rate ($\\dot{m_h}$), shock location ($X_{s}$) and compression ratio (R) are extracted directly. During the entire phase of the outburst, quasi-periodic oscillations (QPOs) are observed sporadically. From the nature of the variation of accretion rate ratio (ARR=$\\dot{m_h}$ / $\\dot{m_d}$) and QPOs, entire period of the outburst "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1509.05867","kind":"arxiv","version":3},"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":"1509.05867","created_at":"2026-05-18T01:17:07.968612+00:00"},{"alias_kind":"arxiv_version","alias_value":"1509.05867v3","created_at":"2026-05-18T01:17:07.968612+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1509.05867","created_at":"2026-05-18T01:17:07.968612+00:00"},{"alias_kind":"pith_short_12","alias_value":"QTZCQA5XFAHH","created_at":"2026-05-18T12:29:39.896362+00:00"},{"alias_kind":"pith_short_16","alias_value":"QTZCQA5XFAHHVSPB","created_at":"2026-05-18T12:29:39.896362+00:00"},{"alias_kind":"pith_short_8","alias_value":"QTZCQA5X","created_at":"2026-05-18T12:29:39.896362+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/QTZCQA5XFAHHVSPBHHHPDGJIAB","json":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB.json","graph_json":"https://pith.science/api/pith-number/QTZCQA5XFAHHVSPBHHHPDGJIAB/graph.json","events_json":"https://pith.science/api/pith-number/QTZCQA5XFAHHVSPBHHHPDGJIAB/events.json","paper":"https://pith.science/paper/QTZCQA5X"},"agent_actions":{"view_html":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB","download_json":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB.json","view_paper":"https://pith.science/paper/QTZCQA5X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1509.05867&json=true","fetch_graph":"https://pith.science/api/pith-number/QTZCQA5XFAHHVSPBHHHPDGJIAB/graph.json","fetch_events":"https://pith.science/api/pith-number/QTZCQA5XFAHHVSPBHHHPDGJIAB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB/action/storage_attestation","attest_author":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB/action/author_attestation","sign_citation":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB/action/citation_signature","submit_replication":"https://pith.science/pith/QTZCQA5XFAHHVSPBHHHPDGJIAB/action/replication_record"}},"created_at":"2026-05-18T01:17:07.968612+00:00","updated_at":"2026-05-18T01:17:07.968612+00:00"}