{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:2W3XMELJENKG2PR5JIV7NRMNCM","short_pith_number":"pith:2W3XMELJ","schema_version":"1.0","canonical_sha256":"d5b776116923546d3e3d4a2bf6c58d1322ec4db371305021ae2a267f21328134","source":{"kind":"arxiv","id":"1312.2084","version":1},"attestation_state":"computed","paper":{"title":"On the Origin of Highly Ionized X-ray Absorbers Detected in the Galactic X-ray Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Taotao Fang, Yang Luo","submitted_at":"2013-12-07T11:03:44Z","abstract_excerpt":"X-ray observations of the Galactic X-ray binaries (XRB) revealed numerous highly ionized metal absorption lines. However, it is unclear whether such lines are produced by the hot interstellar medium (ISM) or the circumstellar medium (CSM) intrinsic to the binaries. Here we present a Chandra X-ray absorption line study of 28 observations on 12 X-ray binaries, with a focus on the NeIX and FeXVII lines. We report the first detections of these lines in a significant amount of observations. We do not find significant dependence of the line equivalent width on the distance of the XRBs, but we do see"},"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":"1312.2084","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-12-07T11:03:44Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"41f28e7eec356873dfe4e580da72096b1b0285c35243e3efd817e37c70085ddc","abstract_canon_sha256":"1b509b6a729d04b9e723e4242310ea692ed2b07d6dc581702df0343220923617"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:57.552451Z","signature_b64":"DUpvr6VQult5fwgTJ1BVjQKabbeVWchsPIka0e5lS3Bod7Ts6WLJIsWL8ar3qrk+7Qlfj3o0hZsW2+vWa6OhAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d5b776116923546d3e3d4a2bf6c58d1322ec4db371305021ae2a267f21328134","last_reissued_at":"2026-05-18T01:45:57.551890Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:57.551890Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Origin of Highly Ionized X-ray Absorbers Detected in the Galactic X-ray Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Taotao Fang, Yang Luo","submitted_at":"2013-12-07T11:03:44Z","abstract_excerpt":"X-ray observations of the Galactic X-ray binaries (XRB) revealed numerous highly ionized metal absorption lines. However, it is unclear whether such lines are produced by the hot interstellar medium (ISM) or the circumstellar medium (CSM) intrinsic to the binaries. Here we present a Chandra X-ray absorption line study of 28 observations on 12 X-ray binaries, with a focus on the NeIX and FeXVII lines. We report the first detections of these lines in a significant amount of observations. We do not find significant dependence of the line equivalent width on the distance of the XRBs, but we do see"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.2084","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":"1312.2084","created_at":"2026-05-18T01:45:57.551966+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.2084v1","created_at":"2026-05-18T01:45:57.551966+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.2084","created_at":"2026-05-18T01:45:57.551966+00:00"},{"alias_kind":"pith_short_12","alias_value":"2W3XMELJENKG","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"2W3XMELJENKG2PR5","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"2W3XMELJ","created_at":"2026-05-18T12:27:32.513160+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/2W3XMELJENKG2PR5JIV7NRMNCM","json":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM.json","graph_json":"https://pith.science/api/pith-number/2W3XMELJENKG2PR5JIV7NRMNCM/graph.json","events_json":"https://pith.science/api/pith-number/2W3XMELJENKG2PR5JIV7NRMNCM/events.json","paper":"https://pith.science/paper/2W3XMELJ"},"agent_actions":{"view_html":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM","download_json":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM.json","view_paper":"https://pith.science/paper/2W3XMELJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.2084&json=true","fetch_graph":"https://pith.science/api/pith-number/2W3XMELJENKG2PR5JIV7NRMNCM/graph.json","fetch_events":"https://pith.science/api/pith-number/2W3XMELJENKG2PR5JIV7NRMNCM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM/action/storage_attestation","attest_author":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM/action/author_attestation","sign_citation":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM/action/citation_signature","submit_replication":"https://pith.science/pith/2W3XMELJENKG2PR5JIV7NRMNCM/action/replication_record"}},"created_at":"2026-05-18T01:45:57.551966+00:00","updated_at":"2026-05-18T01:45:57.551966+00:00"}