{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:YEWBF4QLAUVANQHAHL557V7ZAS","short_pith_number":"pith:YEWBF4QL","schema_version":"1.0","canonical_sha256":"c12c12f20b052a06c0e03afbdfd7f90485daf54546192cf18d027f872f20fd2b","source":{"kind":"arxiv","id":"1106.0009","version":1},"attestation_state":"computed","paper":{"title":"Testing slim-disk models on the thermal spectra of LMC X-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aleksander Sadowski, James F. Steiner, Jeffrey E. McClintock, Marek A. Abramowicz, Michal Bursa, Odele Straub, Ramesh Narayan, Ronald A. Remillard, Wlodzimierz Kluzniak","submitted_at":"2011-05-31T20:00:24Z","abstract_excerpt":"Slim-disk models describe accretion flows at high luminosities, while reducing to the standard thin disk form in the low luminosity limit. We have developed a new spectral model, slimbb, within the framework of XSPEC, which describes fully relativistic slim-disk accretion and includes photon ray-tracing that starts from the disk photosphere, rather than the equatorial plane. We demonstrate the features of this model by applying it to RXTE spectra of the persistent black-hole X-ray binary LMC X-3. LMC X-3 has the virtues of exhibiting large intensity variations while maintaining itself in soft "},"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":"1106.0009","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-05-31T20:00:24Z","cross_cats_sorted":[],"title_canon_sha256":"c681f64e45623910725eef5800436b9d5d3c7604ab66a961a1a80bfef9ef003d","abstract_canon_sha256":"cbd7c31e147642d6730e8eb30c99a81ea42636c75c8add05ee321d9d705851a5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:33:26.678207Z","signature_b64":"il4jTF5q2eoOXrW9EeWwuaMHp6FsgT/X3Y2m+HzPX1bRPBNllFa8uLZmPWMKEFhKQtyJPqEKazDERf9UODg5DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c12c12f20b052a06c0e03afbdfd7f90485daf54546192cf18d027f872f20fd2b","last_reissued_at":"2026-05-18T03:33:26.677284Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:33:26.677284Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing slim-disk models on the thermal spectra of LMC X-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aleksander Sadowski, James F. Steiner, Jeffrey E. McClintock, Marek A. Abramowicz, Michal Bursa, Odele Straub, Ramesh Narayan, Ronald A. Remillard, Wlodzimierz Kluzniak","submitted_at":"2011-05-31T20:00:24Z","abstract_excerpt":"Slim-disk models describe accretion flows at high luminosities, while reducing to the standard thin disk form in the low luminosity limit. We have developed a new spectral model, slimbb, within the framework of XSPEC, which describes fully relativistic slim-disk accretion and includes photon ray-tracing that starts from the disk photosphere, rather than the equatorial plane. We demonstrate the features of this model by applying it to RXTE spectra of the persistent black-hole X-ray binary LMC X-3. LMC X-3 has the virtues of exhibiting large intensity variations while maintaining itself in soft "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.0009","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":"1106.0009","created_at":"2026-05-18T03:33:26.677464+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.0009v1","created_at":"2026-05-18T03:33:26.677464+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.0009","created_at":"2026-05-18T03:33:26.677464+00:00"},{"alias_kind":"pith_short_12","alias_value":"YEWBF4QLAUVA","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_16","alias_value":"YEWBF4QLAUVANQHA","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_8","alias_value":"YEWBF4QL","created_at":"2026-05-18T12:26:47.523578+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/YEWBF4QLAUVANQHAHL557V7ZAS","json":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS.json","graph_json":"https://pith.science/api/pith-number/YEWBF4QLAUVANQHAHL557V7ZAS/graph.json","events_json":"https://pith.science/api/pith-number/YEWBF4QLAUVANQHAHL557V7ZAS/events.json","paper":"https://pith.science/paper/YEWBF4QL"},"agent_actions":{"view_html":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS","download_json":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS.json","view_paper":"https://pith.science/paper/YEWBF4QL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.0009&json=true","fetch_graph":"https://pith.science/api/pith-number/YEWBF4QLAUVANQHAHL557V7ZAS/graph.json","fetch_events":"https://pith.science/api/pith-number/YEWBF4QLAUVANQHAHL557V7ZAS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS/action/storage_attestation","attest_author":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS/action/author_attestation","sign_citation":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS/action/citation_signature","submit_replication":"https://pith.science/pith/YEWBF4QLAUVANQHAHL557V7ZAS/action/replication_record"}},"created_at":"2026-05-18T03:33:26.677464+00:00","updated_at":"2026-05-18T03:33:26.677464+00:00"}