{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:QJFREIVCMM3VBV2WTHIZJRKWHY","short_pith_number":"pith:QJFREIVC","schema_version":"1.0","canonical_sha256":"824b1222a2633750d75699d194c5563e1c84d009f7ddcdeec46153a03ece098a","source":{"kind":"arxiv","id":"1109.1607","version":1},"attestation_state":"computed","paper":{"title":"Implications of the SPEAR FUV Maps on Our Understanding of the ISM","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Eric J. Korpela (1), Jerry Edelstein (1), Kwangil Seon (2), Kyoung-Wook Min (3), Martin Sirk (1), Space Science Institute (3) Korea Advance Institute of Science, Technology), University of California (2) Korea Astronomy, Wonyong Han (2) ((1) Space Sciences Laboratory","submitted_at":"2011-09-08T01:01:56Z","abstract_excerpt":"The distribution of a low-density transition temperature (10^4.5 - 10^5.5 K) gas in the interstellar medium conveys the character and evolution of diffuse matter in the Galaxy. This difficult to observe component of the ISM emits mainly in the far-ultraviolet (FUV) (912-1800 {\\AA}) band. We describe spectral maps of FUV emission lines from the highly ionized species CIV and OVI likely to be the dominant cooling mechanisms of transition temperature gas in the ISM. The maps were obtained using an orbital spectrometer, SPEAR, that was launched in 2003 and has observed the FUV sky with a spectral "},"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":"1109.1607","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2011-09-08T01:01:56Z","cross_cats_sorted":[],"title_canon_sha256":"edff68a643fae526582b76dce72c4fb371cdf0abc7ef8dd27633ffb3cb235726","abstract_canon_sha256":"7cc0627cd36cdd36b0066bbd346d5020843e97a791d375525c449601ad028924"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:13:54.800729Z","signature_b64":"JNOTXyZY3qa2P3CWli0xOOU7XYgwHcYl1+9JpkODB4mtCMRjm6AqikvP9JqFjA/bCxrmQO2QpWdWxzds3GGEDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"824b1222a2633750d75699d194c5563e1c84d009f7ddcdeec46153a03ece098a","last_reissued_at":"2026-05-18T04:13:54.800098Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:13:54.800098Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Implications of the SPEAR FUV Maps on Our Understanding of the ISM","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Eric J. Korpela (1), Jerry Edelstein (1), Kwangil Seon (2), Kyoung-Wook Min (3), Martin Sirk (1), Space Science Institute (3) Korea Advance Institute of Science, Technology), University of California (2) Korea Astronomy, Wonyong Han (2) ((1) Space Sciences Laboratory","submitted_at":"2011-09-08T01:01:56Z","abstract_excerpt":"The distribution of a low-density transition temperature (10^4.5 - 10^5.5 K) gas in the interstellar medium conveys the character and evolution of diffuse matter in the Galaxy. This difficult to observe component of the ISM emits mainly in the far-ultraviolet (FUV) (912-1800 {\\AA}) band. We describe spectral maps of FUV emission lines from the highly ionized species CIV and OVI likely to be the dominant cooling mechanisms of transition temperature gas in the ISM. The maps were obtained using an orbital spectrometer, SPEAR, that was launched in 2003 and has observed the FUV sky with a spectral "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.1607","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":"1109.1607","created_at":"2026-05-18T04:13:54.800175+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.1607v1","created_at":"2026-05-18T04:13:54.800175+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.1607","created_at":"2026-05-18T04:13:54.800175+00:00"},{"alias_kind":"pith_short_12","alias_value":"QJFREIVCMM3V","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_16","alias_value":"QJFREIVCMM3VBV2W","created_at":"2026-05-18T12:26:39.201973+00:00"},{"alias_kind":"pith_short_8","alias_value":"QJFREIVC","created_at":"2026-05-18T12:26:39.201973+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/QJFREIVCMM3VBV2WTHIZJRKWHY","json":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY.json","graph_json":"https://pith.science/api/pith-number/QJFREIVCMM3VBV2WTHIZJRKWHY/graph.json","events_json":"https://pith.science/api/pith-number/QJFREIVCMM3VBV2WTHIZJRKWHY/events.json","paper":"https://pith.science/paper/QJFREIVC"},"agent_actions":{"view_html":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY","download_json":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY.json","view_paper":"https://pith.science/paper/QJFREIVC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.1607&json=true","fetch_graph":"https://pith.science/api/pith-number/QJFREIVCMM3VBV2WTHIZJRKWHY/graph.json","fetch_events":"https://pith.science/api/pith-number/QJFREIVCMM3VBV2WTHIZJRKWHY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY/action/storage_attestation","attest_author":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY/action/author_attestation","sign_citation":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY/action/citation_signature","submit_replication":"https://pith.science/pith/QJFREIVCMM3VBV2WTHIZJRKWHY/action/replication_record"}},"created_at":"2026-05-18T04:13:54.800175+00:00","updated_at":"2026-05-18T04:13:54.800175+00:00"}