{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:TU3Z46TXKBTWWG6FPN5ODR3QYV","short_pith_number":"pith:TU3Z46TX","schema_version":"1.0","canonical_sha256":"9d379e7a7750676b1bc57b7ae1c770c5548712c4b74c7414ed684975375420b1","source":{"kind":"arxiv","id":"2403.02374","version":2},"attestation_state":"computed","paper":{"title":"The COS CGM Compendium V: The Dichotomy of OVI Associated with Low- and High-Metallicity Cool Gas at z < 1","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew J. Fox, Benjamin D. Oppenheimer, J. Christopher Howk, John M. O'Meara, Nicolas Lehner, Sameer","submitted_at":"2024-03-04T19:00:00Z","abstract_excerpt":"We analyze the \\ovi\\ content and kinematics for 126 {\\hi}-selected absorbers at $0.14 \\lesssim z \\lesssim 0.73$ for which the metallicities of their cool photoionized phase have been determined. We separate the absorbers into 100 strong {\\lya} forest systems (SLFSs with $15 \\la$\\,{\\colden}\\,$< 16.2$) and 26 partial Lyman Limit systems (pLLSs with $16.2\\le$\\,{\\colden}\\,$\\le 17.2$). The sample is drawn from the COS CGM Compendium (CCC) and has \\ovi\\ coverage in $\\sn \\geq 8$ {\\it HST}/COS G130M/G160M QSO spectra, yielding a $2\\sigma$ completeness level of {\\coldenovi}$\\,\\geq 13.6$. The \\ovi\\ dete"},"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":"2403.02374","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-03-04T19:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"668c4d83950840798cb08da444381a24cc338c2269ff7079737a91d08154a34a","abstract_canon_sha256":"533db5e6d3a1ccd1840ac1a8fab03fc9f211768b4196063ee0607ae105811319"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:04:08.972601Z","signature_b64":"ujA+P5fQ3gHs7o50+zl1tBRhLcxpGOfe478oFFnOgv6QLYFAV3uUAlQFBOQQv8bxLIcXTUou4z3GZNBf/ufBDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d379e7a7750676b1bc57b7ae1c770c5548712c4b74c7414ed684975375420b1","last_reissued_at":"2026-07-05T09:04:08.972084Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:04:08.972084Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The COS CGM Compendium V: The Dichotomy of OVI Associated with Low- and High-Metallicity Cool Gas at z < 1","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew J. Fox, Benjamin D. Oppenheimer, J. Christopher Howk, John M. O'Meara, Nicolas Lehner, Sameer","submitted_at":"2024-03-04T19:00:00Z","abstract_excerpt":"We analyze the \\ovi\\ content and kinematics for 126 {\\hi}-selected absorbers at $0.14 \\lesssim z \\lesssim 0.73$ for which the metallicities of their cool photoionized phase have been determined. We separate the absorbers into 100 strong {\\lya} forest systems (SLFSs with $15 \\la$\\,{\\colden}\\,$< 16.2$) and 26 partial Lyman Limit systems (pLLSs with $16.2\\le$\\,{\\colden}\\,$\\le 17.2$). The sample is drawn from the COS CGM Compendium (CCC) and has \\ovi\\ coverage in $\\sn \\geq 8$ {\\it HST}/COS G130M/G160M QSO spectra, yielding a $2\\sigma$ completeness level of {\\coldenovi}$\\,\\geq 13.6$. The \\ovi\\ dete"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.02374","kind":"arxiv","version":2},"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/2403.02374/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":"2403.02374","created_at":"2026-07-05T09:04:08.972148+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.02374v2","created_at":"2026-07-05T09:04:08.972148+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.02374","created_at":"2026-07-05T09:04:08.972148+00:00"},{"alias_kind":"pith_short_12","alias_value":"TU3Z46TXKBTW","created_at":"2026-07-05T09:04:08.972148+00:00"},{"alias_kind":"pith_short_16","alias_value":"TU3Z46TXKBTWWG6F","created_at":"2026-07-05T09:04:08.972148+00:00"},{"alias_kind":"pith_short_8","alias_value":"TU3Z46TX","created_at":"2026-07-05T09:04:08.972148+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.02348","citing_title":"Figuring Out Gas & Galaxies in Enzo (FOGGIE). XV. Examining the Spatial and Kinematic Relationship between Circumgalactic Mg II and O VI","ref_index":31,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV","json":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV.json","graph_json":"https://pith.science/api/pith-number/TU3Z46TXKBTWWG6FPN5ODR3QYV/graph.json","events_json":"https://pith.science/api/pith-number/TU3Z46TXKBTWWG6FPN5ODR3QYV/events.json","paper":"https://pith.science/paper/TU3Z46TX"},"agent_actions":{"view_html":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV","download_json":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV.json","view_paper":"https://pith.science/paper/TU3Z46TX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.02374&json=true","fetch_graph":"https://pith.science/api/pith-number/TU3Z46TXKBTWWG6FPN5ODR3QYV/graph.json","fetch_events":"https://pith.science/api/pith-number/TU3Z46TXKBTWWG6FPN5ODR3QYV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV/action/storage_attestation","attest_author":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV/action/author_attestation","sign_citation":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV/action/citation_signature","submit_replication":"https://pith.science/pith/TU3Z46TXKBTWWG6FPN5ODR3QYV/action/replication_record"}},"created_at":"2026-07-05T09:04:08.972148+00:00","updated_at":"2026-07-05T09:04:08.972148+00:00"}