{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:72YNFWRTH22QBLZWSUOOTWBOPT","short_pith_number":"pith:72YNFWRT","schema_version":"1.0","canonical_sha256":"feb0d2da333eb500af36951ce9d82e7ce8009499a53ed5098ded613d52d28bb1","source":{"kind":"arxiv","id":"1903.10649","version":1},"attestation_state":"computed","paper":{"title":"The Panchromatic Circumgalactic Medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Dennis Zaritsky, Jason Tumlinson, J. E. G. Peek, Jessica Werk, John M. O'Meara, Joseph N. Burchett, Marc Rafelski, Molly S. Peeples, Nicolas Lehner, Q.Daniel Wang","submitted_at":"2019-03-26T01:25:40Z","abstract_excerpt":"Galaxies are surrounded by extended atmospheres, which are often called the circumgalactic medium (CGM) and are the least understood part of galactic ecosystems. The CGM serves as a reservoir of both diffuse, metal-poor gas accreted from the intergalactic medium, and metal-rich gas that is either ejected from galaxies by energetic feedback or stripped from infalling satellites. As such, the CGM is empirically multi-phased and complex in dynamics. Significant progress has been made in the past decade or so in observing the cosmic-ray/B-field, as well as various phases of the CGM. But basic ques"},"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":"1903.10649","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-03-26T01:25:40Z","cross_cats_sorted":[],"title_canon_sha256":"2de4d8d83ffbfb1ab83e18c4b25747eaf5a1511e89398f6c726130b46c69cc46","abstract_canon_sha256":"3266680a178b92071a3795d87e9f79a4963c92a52f08def7fd1d24cca4ea53f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:50:18.216260Z","signature_b64":"Pkop5LPJG5Tce2WeAktCbl4GGwK82RIwi4Qiz/2JUyX7/JutU92+3LPM/8OUI3hMeAz7zmeRgytIhOXbOslNDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"feb0d2da333eb500af36951ce9d82e7ce8009499a53ed5098ded613d52d28bb1","last_reissued_at":"2026-05-17T23:50:18.215494Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:50:18.215494Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Panchromatic Circumgalactic Medium","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Dennis Zaritsky, Jason Tumlinson, J. E. G. Peek, Jessica Werk, John M. O'Meara, Joseph N. Burchett, Marc Rafelski, Molly S. Peeples, Nicolas Lehner, Q.Daniel Wang","submitted_at":"2019-03-26T01:25:40Z","abstract_excerpt":"Galaxies are surrounded by extended atmospheres, which are often called the circumgalactic medium (CGM) and are the least understood part of galactic ecosystems. The CGM serves as a reservoir of both diffuse, metal-poor gas accreted from the intergalactic medium, and metal-rich gas that is either ejected from galaxies by energetic feedback or stripped from infalling satellites. As such, the CGM is empirically multi-phased and complex in dynamics. Significant progress has been made in the past decade or so in observing the cosmic-ray/B-field, as well as various phases of the CGM. But basic ques"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.10649","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":"1903.10649","created_at":"2026-05-17T23:50:18.215607+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.10649v1","created_at":"2026-05-17T23:50:18.215607+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.10649","created_at":"2026-05-17T23:50:18.215607+00:00"},{"alias_kind":"pith_short_12","alias_value":"72YNFWRTH22Q","created_at":"2026-05-18T12:33:10.108867+00:00"},{"alias_kind":"pith_short_16","alias_value":"72YNFWRTH22QBLZW","created_at":"2026-05-18T12:33:10.108867+00:00"},{"alias_kind":"pith_short_8","alias_value":"72YNFWRT","created_at":"2026-05-18T12:33:10.108867+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.01505","citing_title":"Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures","ref_index":89,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT","json":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT.json","graph_json":"https://pith.science/api/pith-number/72YNFWRTH22QBLZWSUOOTWBOPT/graph.json","events_json":"https://pith.science/api/pith-number/72YNFWRTH22QBLZWSUOOTWBOPT/events.json","paper":"https://pith.science/paper/72YNFWRT"},"agent_actions":{"view_html":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT","download_json":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT.json","view_paper":"https://pith.science/paper/72YNFWRT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.10649&json=true","fetch_graph":"https://pith.science/api/pith-number/72YNFWRTH22QBLZWSUOOTWBOPT/graph.json","fetch_events":"https://pith.science/api/pith-number/72YNFWRTH22QBLZWSUOOTWBOPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT/action/storage_attestation","attest_author":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT/action/author_attestation","sign_citation":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT/action/citation_signature","submit_replication":"https://pith.science/pith/72YNFWRTH22QBLZWSUOOTWBOPT/action/replication_record"}},"created_at":"2026-05-17T23:50:18.215607+00:00","updated_at":"2026-05-17T23:50:18.215607+00:00"}