{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:CFNEHNKZMZQ23FCPKUAK7MMVBK","short_pith_number":"pith:CFNEHNKZ","schema_version":"1.0","canonical_sha256":"115a43b5596661ad944f5500afb1950a991ca8bbfb4382236869eefd9061ff32","source":{"kind":"arxiv","id":"1408.4896","version":2},"attestation_state":"computed","paper":{"title":"CMB distortion from circumgalactic gas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Biman B. Nath, Joseph Silk, Priyanka Singh, Subhabrata Majumdar","submitted_at":"2014-08-21T06:26:34Z","abstract_excerpt":"We study the Sunyaev-Zel'dovich (SZ) distortion of the cosmic microwave background radiation (CMBR) from extensive circumgalactic gas (CGM) in massive galactic halos. Recent observations have shown that galactic halos contain a large amount of X-ray emitting gas at the virial temperature, as well as a significant amount of warm OVI absorbing gas. We consider the SZ distortion from the hot gas in those galactic halos in which the gas cooling time is longer than the halo destruction time scale. We show that the SZ distortion signal from the hot gas in these galactic halos at redshifts $z\\approx "},"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":"1408.4896","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-08-21T06:26:34Z","cross_cats_sorted":[],"title_canon_sha256":"7b0f6a25c4fb79119f5f5c5c706bc57c1b21ae2c18e5c10648282c60b6e5a924","abstract_canon_sha256":"fa18da9ef14053a8dd1194ddcef83fa1785c58bef18ea172f1677f559ff37c2e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:16.305781Z","signature_b64":"9FeBSuJCbxjOQ+Q5kCiUyx7p/Xkq/L2uZp2UfxM2NG1+sRZZKB7kG9vCM3AqXIUVyqO+oz82Qe4Vi9aWbXHHDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"115a43b5596661ad944f5500afb1950a991ca8bbfb4382236869eefd9061ff32","last_reissued_at":"2026-05-18T01:42:16.305105Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:16.305105Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CMB distortion from circumgalactic gas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Biman B. Nath, Joseph Silk, Priyanka Singh, Subhabrata Majumdar","submitted_at":"2014-08-21T06:26:34Z","abstract_excerpt":"We study the Sunyaev-Zel'dovich (SZ) distortion of the cosmic microwave background radiation (CMBR) from extensive circumgalactic gas (CGM) in massive galactic halos. Recent observations have shown that galactic halos contain a large amount of X-ray emitting gas at the virial temperature, as well as a significant amount of warm OVI absorbing gas. We consider the SZ distortion from the hot gas in those galactic halos in which the gas cooling time is longer than the halo destruction time scale. We show that the SZ distortion signal from the hot gas in these galactic halos at redshifts $z\\approx "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.4896","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":""},"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":"1408.4896","created_at":"2026-05-18T01:42:16.305192+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.4896v2","created_at":"2026-05-18T01:42:16.305192+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.4896","created_at":"2026-05-18T01:42:16.305192+00:00"},{"alias_kind":"pith_short_12","alias_value":"CFNEHNKZMZQ2","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"CFNEHNKZMZQ23FCP","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"CFNEHNKZ","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2503.16355","citing_title":"DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy","ref_index":65,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK","json":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK.json","graph_json":"https://pith.science/api/pith-number/CFNEHNKZMZQ23FCPKUAK7MMVBK/graph.json","events_json":"https://pith.science/api/pith-number/CFNEHNKZMZQ23FCPKUAK7MMVBK/events.json","paper":"https://pith.science/paper/CFNEHNKZ"},"agent_actions":{"view_html":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK","download_json":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK.json","view_paper":"https://pith.science/paper/CFNEHNKZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.4896&json=true","fetch_graph":"https://pith.science/api/pith-number/CFNEHNKZMZQ23FCPKUAK7MMVBK/graph.json","fetch_events":"https://pith.science/api/pith-number/CFNEHNKZMZQ23FCPKUAK7MMVBK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK/action/storage_attestation","attest_author":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK/action/author_attestation","sign_citation":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK/action/citation_signature","submit_replication":"https://pith.science/pith/CFNEHNKZMZQ23FCPKUAK7MMVBK/action/replication_record"}},"created_at":"2026-05-18T01:42:16.305192+00:00","updated_at":"2026-05-18T01:42:16.305192+00:00"}