{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:YWWS2TES2KNUPV3FNXA5ZBLE7M","short_pith_number":"pith:YWWS2TES","schema_version":"1.0","canonical_sha256":"c5ad2d4c92d29b47d7656dc1dc8564fb0183a5b849cfdee508294301e078478c","source":{"kind":"arxiv","id":"1201.1916","version":2},"attestation_state":"computed","paper":{"title":"Herschel-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cava, A. Cooray, A. Dariush, A. Lapi, A. M. Hopkins, A. S. G. Robotham, B. Madore, C. C. Popescu, C. J. Conselice, D. G. Bonfield, D. H. Jones, D. J. B. Smith, D. L. Clements, E. E. Rigby, E. Ibar, G. de Zotti, G. Rodighiero, H. L. Gomez, I. K. Baldry, J. Fritz, J. Gonzalez-Nuevo, J. Liske, J. Loveday, L. Dunne, L. S. Kelvin, M. Baes, M. J. Jarvis, M. J. Michalowski, M. Pohlen, M. Seibert, N. Bourne, P. Norberg, P. Temi, P. van der Werf, R. Auld, R. Hopwood, R. J. Ivison, R. J. Tuffs, S. Brough, S. Buttiglione, S. Dye, S. Eales, S. J. Maddox, S. M. Croom, S. P. Driver","submitted_at":"2012-01-09T21:00:06Z","abstract_excerpt":"We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the submm properties of optically selected galaxies. Using ~80,000 r-band selected galaxies from 126 deg^2 of the GAMA survey, we stack into submm imaging at 250, 350 and 500{\\mu}m to gain unprecedented statistics on the dust emission from galaxies at z < 0.35. We find that low redshift galaxies account for 5% of the cosmic 250{\\mu}m background (4% at 350{\\mu}m; 3% at 500{\\mu}m), of which approximately 60% comes from 'blue' and 20% from 'red' galaxies (rest-frame g - r). We compare the dust properties of dif"},"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":"1201.1916","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-01-09T21:00:06Z","cross_cats_sorted":[],"title_canon_sha256":"67fa3d9cf0c2d7b72debd3406c2404720cdd5dc221158e8452ccb70c32ae84a9","abstract_canon_sha256":"bed231ba776ed3cc4e19f2d4ebee0fe4f82349cbf5d0fda61b50668c9282aa57"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:58:04.242992Z","signature_b64":"4aRZ5K7/bhKrQxe0uds9Q4aVXcDpUiwNs7AkfORAh0bS4AGtXTxb4QXuSeyS9jV8rUCxDnrB/FY1a8nd93pJCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c5ad2d4c92d29b47d7656dc1dc8564fb0183a5b849cfdee508294301e078478c","last_reissued_at":"2026-05-18T03:58:04.242394Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:58:04.242394Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cava, A. Cooray, A. Dariush, A. Lapi, A. M. Hopkins, A. S. G. Robotham, B. Madore, C. C. Popescu, C. J. Conselice, D. G. Bonfield, D. H. Jones, D. J. B. Smith, D. L. Clements, E. E. Rigby, E. Ibar, G. de Zotti, G. Rodighiero, H. L. Gomez, I. K. Baldry, J. Fritz, J. Gonzalez-Nuevo, J. Liske, J. Loveday, L. Dunne, L. S. Kelvin, M. Baes, M. J. Jarvis, M. J. Michalowski, M. Pohlen, M. Seibert, N. Bourne, P. Norberg, P. Temi, P. van der Werf, R. Auld, R. Hopwood, R. J. Ivison, R. J. Tuffs, S. Brough, S. Buttiglione, S. Dye, S. Eales, S. J. Maddox, S. M. Croom, S. P. Driver","submitted_at":"2012-01-09T21:00:06Z","abstract_excerpt":"We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the submm properties of optically selected galaxies. Using ~80,000 r-band selected galaxies from 126 deg^2 of the GAMA survey, we stack into submm imaging at 250, 350 and 500{\\mu}m to gain unprecedented statistics on the dust emission from galaxies at z < 0.35. We find that low redshift galaxies account for 5% of the cosmic 250{\\mu}m background (4% at 350{\\mu}m; 3% at 500{\\mu}m), of which approximately 60% comes from 'blue' and 20% from 'red' galaxies (rest-frame g - r). We compare the dust properties of dif"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.1916","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":"1201.1916","created_at":"2026-05-18T03:58:04.242489+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.1916v2","created_at":"2026-05-18T03:58:04.242489+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.1916","created_at":"2026-05-18T03:58:04.242489+00:00"},{"alias_kind":"pith_short_12","alias_value":"YWWS2TES2KNU","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"YWWS2TES2KNUPV3F","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"YWWS2TES","created_at":"2026-05-18T12:27:30.460161+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/YWWS2TES2KNUPV3FNXA5ZBLE7M","json":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M.json","graph_json":"https://pith.science/api/pith-number/YWWS2TES2KNUPV3FNXA5ZBLE7M/graph.json","events_json":"https://pith.science/api/pith-number/YWWS2TES2KNUPV3FNXA5ZBLE7M/events.json","paper":"https://pith.science/paper/YWWS2TES"},"agent_actions":{"view_html":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M","download_json":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M.json","view_paper":"https://pith.science/paper/YWWS2TES","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.1916&json=true","fetch_graph":"https://pith.science/api/pith-number/YWWS2TES2KNUPV3FNXA5ZBLE7M/graph.json","fetch_events":"https://pith.science/api/pith-number/YWWS2TES2KNUPV3FNXA5ZBLE7M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M/action/storage_attestation","attest_author":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M/action/author_attestation","sign_citation":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M/action/citation_signature","submit_replication":"https://pith.science/pith/YWWS2TES2KNUPV3FNXA5ZBLE7M/action/replication_record"}},"created_at":"2026-05-18T03:58:04.242489+00:00","updated_at":"2026-05-18T03:58:04.242489+00:00"}