{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:DCO4LMI4ICO36UCI3B6ERT6C5C","short_pith_number":"pith:DCO4LMI4","schema_version":"1.0","canonical_sha256":"189dc5b11c409dbf5048d87c48cfc2e880af628757f079b737d9b8caf217bd87","source":{"kind":"arxiv","id":"2202.00690","version":1},"attestation_state":"computed","paper":{"title":"The cold interstellar medium of galaxies in the Local Universe","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Amelie Saintonge, Barbara Catinella","submitted_at":"2022-02-01T19:00:02Z","abstract_excerpt":"The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is the reservoir that fuels galaxy growth via star formation, the repository of material formed by these stars, and a sensitive tracer of internal and external processes that affect entire galaxies. Consequently, significant efforts have gone into systematic surveys of the cold ISM of the galaxies in the local Universe. This review discusses the resulting network of scaling relations connecting the atomic and molecular gas masses of galaxies with their other global properties (stellar masses, morphologi"},"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":"2202.00690","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-02-01T19:00:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"d2f2521a93e0e9159249c786b8a8c540aad8bac6ec52be5b605fd80e75941d72","abstract_canon_sha256":"4516568c9f41b52810a13cf4749125773d21e84e92e542e9837956e1a3fd0c92"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:54:18.176016Z","signature_b64":"tISqAT+q2CEKOHKCNgyRXRYNqHWEqgFONDPeXPfvu88V5VeBraM11NxwttHw0nnrvycXhcUjqr/ibwOeRGi8Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"189dc5b11c409dbf5048d87c48cfc2e880af628757f079b737d9b8caf217bd87","last_reissued_at":"2026-07-05T04:54:18.175606Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:54:18.175606Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The cold interstellar medium of galaxies in the Local Universe","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Amelie Saintonge, Barbara Catinella","submitted_at":"2022-02-01T19:00:02Z","abstract_excerpt":"The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is the reservoir that fuels galaxy growth via star formation, the repository of material formed by these stars, and a sensitive tracer of internal and external processes that affect entire galaxies. Consequently, significant efforts have gone into systematic surveys of the cold ISM of the galaxies in the local Universe. This review discusses the resulting network of scaling relations connecting the atomic and molecular gas masses of galaxies with their other global properties (stellar masses, morphologi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2202.00690","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/2202.00690/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":"2202.00690","created_at":"2026-07-05T04:54:18.175672+00:00"},{"alias_kind":"arxiv_version","alias_value":"2202.00690v1","created_at":"2026-07-05T04:54:18.175672+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2202.00690","created_at":"2026-07-05T04:54:18.175672+00:00"},{"alias_kind":"pith_short_12","alias_value":"DCO4LMI4ICO3","created_at":"2026-07-05T04:54:18.175672+00:00"},{"alias_kind":"pith_short_16","alias_value":"DCO4LMI4ICO36UCI","created_at":"2026-07-05T04:54:18.175672+00:00"},{"alias_kind":"pith_short_8","alias_value":"DCO4LMI4","created_at":"2026-07-05T04:54:18.175672+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2607.07441","citing_title":"A machine learning approach to estimating HI deficiency in galaxies","ref_index":37,"is_internal_anchor":true},{"citing_arxiv_id":"2607.05326","citing_title":"Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years","ref_index":4,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C","json":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C.json","graph_json":"https://pith.science/api/pith-number/DCO4LMI4ICO36UCI3B6ERT6C5C/graph.json","events_json":"https://pith.science/api/pith-number/DCO4LMI4ICO36UCI3B6ERT6C5C/events.json","paper":"https://pith.science/paper/DCO4LMI4"},"agent_actions":{"view_html":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C","download_json":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C.json","view_paper":"https://pith.science/paper/DCO4LMI4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2202.00690&json=true","fetch_graph":"https://pith.science/api/pith-number/DCO4LMI4ICO36UCI3B6ERT6C5C/graph.json","fetch_events":"https://pith.science/api/pith-number/DCO4LMI4ICO36UCI3B6ERT6C5C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C/action/storage_attestation","attest_author":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C/action/author_attestation","sign_citation":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C/action/citation_signature","submit_replication":"https://pith.science/pith/DCO4LMI4ICO36UCI3B6ERT6C5C/action/replication_record"}},"created_at":"2026-07-05T04:54:18.175672+00:00","updated_at":"2026-07-05T04:54:18.175672+00:00"}