{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:ZUERCEGFPAPV65SFZGG6DO4KUJ","short_pith_number":"pith:ZUERCEGF","schema_version":"1.0","canonical_sha256":"cd091110c5781f5f7645c98de1bb8aa2610341f1a7c2a7ca8f624615552a4b7b","source":{"kind":"arxiv","id":"1303.1178","version":1},"attestation_state":"computed","paper":{"title":"Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Boselli, A. Cooray, C. D. Wilson, G. Bendo, I. De Looze, J. Koda, L. Ciesla, L. Cortese, L. Spinoglio, M. Baes, M. Boquien, M. W. L. Smith, S. Boissier, S. Eales, V. Buat, V. Lebouteiller","submitted_at":"2013-03-05T21:00:00Z","abstract_excerpt":"[abridged]\n  Aims. The aim of the present paper is to provide new and more detailed relations at the kpc scale between the gas surface density and the face-on optical depth directly calibrated on galaxies, in order to compute the attenuation not only for semi-analytic models but also observationally as new and upcoming radio observatories are able to trace gas ever farther in the Universe.\n  Methods. We have selected a sample of 4 nearby resolved galaxies and a sample of 27 unresolved galaxies from the Herschel Reference Survey and the Very Nearby Galaxies Survey, for which we have a large set"},"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":"1303.1178","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-03-05T21:00:00Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"8884b83af7a286f4ba525649f5535b06bd38acd386420ded35bab44b06641ab7","abstract_canon_sha256":"94a51a00bb71221ce94652428c76bcb5bb214a881ca2f4bae752e521cdee5974"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:16.641107Z","signature_b64":"yyWTCO5NkL0Owg2OrO6+YfwsOhbaDy+1VwU5+vJEkMvIACI9YX5B3Ru1W4m57Z2n3dsm62g6LSqoYRKiMuO7Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cd091110c5781f5f7645c98de1bb8aa2610341f1a7c2a7ca8f624615552a4b7b","last_reissued_at":"2026-05-18T01:51:16.640509Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:16.640509Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. Boselli, A. Cooray, C. D. Wilson, G. Bendo, I. De Looze, J. Koda, L. Ciesla, L. Cortese, L. Spinoglio, M. Baes, M. Boquien, M. W. L. Smith, S. Boissier, S. Eales, V. Buat, V. Lebouteiller","submitted_at":"2013-03-05T21:00:00Z","abstract_excerpt":"[abridged]\n  Aims. The aim of the present paper is to provide new and more detailed relations at the kpc scale between the gas surface density and the face-on optical depth directly calibrated on galaxies, in order to compute the attenuation not only for semi-analytic models but also observationally as new and upcoming radio observatories are able to trace gas ever farther in the Universe.\n  Methods. We have selected a sample of 4 nearby resolved galaxies and a sample of 27 unresolved galaxies from the Herschel Reference Survey and the Very Nearby Galaxies Survey, for which we have a large set"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.1178","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":"1303.1178","created_at":"2026-05-18T01:51:16.640602+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.1178v1","created_at":"2026-05-18T01:51:16.640602+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.1178","created_at":"2026-05-18T01:51:16.640602+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZUERCEGFPAPV","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZUERCEGFPAPV65SF","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZUERCEGF","created_at":"2026-05-18T12:28:09.283467+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/ZUERCEGFPAPV65SFZGG6DO4KUJ","json":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ.json","graph_json":"https://pith.science/api/pith-number/ZUERCEGFPAPV65SFZGG6DO4KUJ/graph.json","events_json":"https://pith.science/api/pith-number/ZUERCEGFPAPV65SFZGG6DO4KUJ/events.json","paper":"https://pith.science/paper/ZUERCEGF"},"agent_actions":{"view_html":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ","download_json":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ.json","view_paper":"https://pith.science/paper/ZUERCEGF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.1178&json=true","fetch_graph":"https://pith.science/api/pith-number/ZUERCEGFPAPV65SFZGG6DO4KUJ/graph.json","fetch_events":"https://pith.science/api/pith-number/ZUERCEGFPAPV65SFZGG6DO4KUJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ/action/storage_attestation","attest_author":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ/action/author_attestation","sign_citation":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ/action/citation_signature","submit_replication":"https://pith.science/pith/ZUERCEGFPAPV65SFZGG6DO4KUJ/action/replication_record"}},"created_at":"2026-05-18T01:51:16.640602+00:00","updated_at":"2026-05-18T01:51:16.640602+00:00"}