{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:3TEGVNV4YGDKZMTY4Z7YMCONGL","short_pith_number":"pith:3TEGVNV4","schema_version":"1.0","canonical_sha256":"dcc86ab6bcc186acb278e67f8609cd32d19408c4a9890ecdc73686712b104929","source":{"kind":"arxiv","id":"astro-ph/0508661","version":1},"attestation_state":"computed","paper":{"title":"Warm-Hot Gas in and around the Milky Way: Detection and Implications of OVII Absorption toward LMC X-3","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Nicastro, L. Song, Q. D. Wang, R. Croft, R. J. Williams, S. Mathur, T. M. Tripp, T.-T. Fang, W. Cui, Y. Yao","submitted_at":"2005-08-30T20:14:49Z","abstract_excerpt":"X-ray absorption lines of highly-ionized species such as OVII at about zero redshift have been firmly detected in the spectra of several active galactic nuclei. However, the location of the absorbing gas remains a subject of debate. To separate the Galactic and extragalactic contributions to the absorption, we have obtained Chandra LETG-HRC and FUSE observations of the black hole X-ray binary LMC X--3. A joint analysis of the detected OVII and Ne IX Kalpha lines, together with the non-detection of the OVII Kbeta and OVIII Kalpha lines, gives the measurements of the temperature, velocity disper"},"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":"astro-ph/0508661","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-08-30T20:14:49Z","cross_cats_sorted":[],"title_canon_sha256":"5c83d378202167dd13594fec8467a849cf21c88d1425b39e3f7425e06341b14b","abstract_canon_sha256":"05c1ea2ac8e99cdb4688bc8c2cd5e9b8002b189d3df3183067018054bd8668e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:15:05.063624Z","signature_b64":"o0xH/ihscHlzlPa/HmPgiaB9j5rmLR9zxWjXkO/gQRzPhsBiC2H6hOIlebHJL9V/FH5oxyGTlbllpVHogJE3Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dcc86ab6bcc186acb278e67f8609cd32d19408c4a9890ecdc73686712b104929","last_reissued_at":"2026-07-04T17:15:05.063199Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:15:05.063199Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Warm-Hot Gas in and around the Milky Way: Detection and Implications of OVII Absorption toward LMC X-3","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Nicastro, L. Song, Q. D. Wang, R. Croft, R. J. Williams, S. Mathur, T. M. Tripp, T.-T. Fang, W. Cui, Y. Yao","submitted_at":"2005-08-30T20:14:49Z","abstract_excerpt":"X-ray absorption lines of highly-ionized species such as OVII at about zero redshift have been firmly detected in the spectra of several active galactic nuclei. However, the location of the absorbing gas remains a subject of debate. To separate the Galactic and extragalactic contributions to the absorption, we have obtained Chandra LETG-HRC and FUSE observations of the black hole X-ray binary LMC X--3. A joint analysis of the detected OVII and Ne IX Kalpha lines, together with the non-detection of the OVII Kbeta and OVIII Kalpha lines, gives the measurements of the temperature, velocity disper"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0508661","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0508661/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0508661","created_at":"2026-07-04T17:15:05.063258+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0508661v1","created_at":"2026-07-04T17:15:05.063258+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0508661","created_at":"2026-07-04T17:15:05.063258+00:00"},{"alias_kind":"pith_short_12","alias_value":"3TEGVNV4YGDK","created_at":"2026-07-04T17:15:05.063258+00:00"},{"alias_kind":"pith_short_16","alias_value":"3TEGVNV4YGDKZMTY","created_at":"2026-07-04T17:15:05.063258+00:00"},{"alias_kind":"pith_short_8","alias_value":"3TEGVNV4","created_at":"2026-07-04T17:15:05.063258+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/3TEGVNV4YGDKZMTY4Z7YMCONGL","json":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL.json","graph_json":"https://pith.science/api/pith-number/3TEGVNV4YGDKZMTY4Z7YMCONGL/graph.json","events_json":"https://pith.science/api/pith-number/3TEGVNV4YGDKZMTY4Z7YMCONGL/events.json","paper":"https://pith.science/paper/3TEGVNV4"},"agent_actions":{"view_html":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL","download_json":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL.json","view_paper":"https://pith.science/paper/3TEGVNV4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0508661&json=true","fetch_graph":"https://pith.science/api/pith-number/3TEGVNV4YGDKZMTY4Z7YMCONGL/graph.json","fetch_events":"https://pith.science/api/pith-number/3TEGVNV4YGDKZMTY4Z7YMCONGL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL/action/storage_attestation","attest_author":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL/action/author_attestation","sign_citation":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL/action/citation_signature","submit_replication":"https://pith.science/pith/3TEGVNV4YGDKZMTY4Z7YMCONGL/action/replication_record"}},"created_at":"2026-07-04T17:15:05.063258+00:00","updated_at":"2026-07-04T17:15:05.063258+00:00"}