{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:7OEWQN5JX6EIP2OODJIVBHKY3M","short_pith_number":"pith:7OEWQN5J","schema_version":"1.0","canonical_sha256":"fb896837a9bf8887e9ce1a51509d58db1dda92f36c26cb30857956618f5bfa0a","source":{"kind":"arxiv","id":"astro-ph/0410602","version":1},"attestation_state":"computed","paper":{"title":"Abundances and Depletions of Interstellar Oxygen","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Adam G. Jensen, Brian L. Rachford, Theodore P. Snow","submitted_at":"2004-10-25T17:18:27Z","abstract_excerpt":"We report on the abundance of interstellar neutral oxygen (OI) for 26 sightlines, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE), the International Spectroscopic Explorer (IUE), and the Hubble Space Telescope (HST). OI column densities are derived by measuring the equivalent widths of several ultraviolet absorption lines, and subsequently fitting those to a curve of growth. We consider both our general sample of 26 sightlines and a more restrictive sample of 10 sightlines that utilize HST data for a measurement of the weak 1355 angstrom line of oxygen, and are thus better co"},"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/0410602","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-25T17:18:27Z","cross_cats_sorted":[],"title_canon_sha256":"55f38a1c33b8d7cf18845e06784063cfd899f41799e605f3482c36d2204b5c71","abstract_canon_sha256":"2b6dad7d8e39ccc942e665e70c2b3ce56f9be8ff0be001018a701f282b0268fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:45:02.684351Z","signature_b64":"4xnMvoxK91102660363GzIw/1ZX+z44vYa1QtIQOXbnaHXkiX3BTWoI75GHXutjs/DeUq70zR1Q7Y3FrBTu2Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fb896837a9bf8887e9ce1a51509d58db1dda92f36c26cb30857956618f5bfa0a","last_reissued_at":"2026-07-04T16:45:02.683987Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:45:02.683987Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Abundances and Depletions of Interstellar Oxygen","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Adam G. Jensen, Brian L. Rachford, Theodore P. Snow","submitted_at":"2004-10-25T17:18:27Z","abstract_excerpt":"We report on the abundance of interstellar neutral oxygen (OI) for 26 sightlines, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE), the International Spectroscopic Explorer (IUE), and the Hubble Space Telescope (HST). OI column densities are derived by measuring the equivalent widths of several ultraviolet absorption lines, and subsequently fitting those to a curve of growth. We consider both our general sample of 26 sightlines and a more restrictive sample of 10 sightlines that utilize HST data for a measurement of the weak 1355 angstrom line of oxygen, and are thus better co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410602","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/0410602/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/0410602","created_at":"2026-07-04T16:45:02.684048+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410602v1","created_at":"2026-07-04T16:45:02.684048+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410602","created_at":"2026-07-04T16:45:02.684048+00:00"},{"alias_kind":"pith_short_12","alias_value":"7OEWQN5JX6EI","created_at":"2026-07-04T16:45:02.684048+00:00"},{"alias_kind":"pith_short_16","alias_value":"7OEWQN5JX6EIP2OO","created_at":"2026-07-04T16:45:02.684048+00:00"},{"alias_kind":"pith_short_8","alias_value":"7OEWQN5J","created_at":"2026-07-04T16:45:02.684048+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/7OEWQN5JX6EIP2OODJIVBHKY3M","json":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M.json","graph_json":"https://pith.science/api/pith-number/7OEWQN5JX6EIP2OODJIVBHKY3M/graph.json","events_json":"https://pith.science/api/pith-number/7OEWQN5JX6EIP2OODJIVBHKY3M/events.json","paper":"https://pith.science/paper/7OEWQN5J"},"agent_actions":{"view_html":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M","download_json":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M.json","view_paper":"https://pith.science/paper/7OEWQN5J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0410602&json=true","fetch_graph":"https://pith.science/api/pith-number/7OEWQN5JX6EIP2OODJIVBHKY3M/graph.json","fetch_events":"https://pith.science/api/pith-number/7OEWQN5JX6EIP2OODJIVBHKY3M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M/action/storage_attestation","attest_author":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M/action/author_attestation","sign_citation":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M/action/citation_signature","submit_replication":"https://pith.science/pith/7OEWQN5JX6EIP2OODJIVBHKY3M/action/replication_record"}},"created_at":"2026-07-04T16:45:02.684048+00:00","updated_at":"2026-07-04T16:45:02.684048+00:00"}