{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:26QIMMNHE7UFHFPU2YFNWZZORW","short_pith_number":"pith:26QIMMNH","schema_version":"1.0","canonical_sha256":"d7a08631a727e85395f4d60adb672e8da30d71d258771fd3da1e30efc38307ee","source":{"kind":"arxiv","id":"1005.2409","version":1},"attestation_state":"computed","paper":{"title":"The Herschel-ATLAS: Extragalactic Number Counts from 250 to 500 Microns","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Cava, A. Cooray, A. Dariush, A. Mortier, A. Verma, B. Sibthorpe, C. Pearson, D. Bonfield, D. Burgarella, D. Frayer, D. Herranz, D.J.B. Smith, D.L. Clements, Douglas Scott, E. Ibar, E. Pascale, E. Rigby, G. de Zotti, G. Lagache, G. Rodighiero, I. Valtchanov, J. Fritz, J. Gonzalez-Nuevo, Jonathan P. Gardner, L. Dunne, L. Leeuw, M. Baes, M.J. Jarvis, M. Lopez-Caniego, M. Negrello, M. Pohlen, M. Thompson, P. Temi, P. van der Werf, R. Auld, R. Ivison, S. Buttiglione, S. Dye, S. Eales, S. Maddox, S. Samui, S. Serjeant","submitted_at":"2010-05-13T20:00:08Z","abstract_excerpt":"Aims. The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 microns when completed, reaching flux limits (5 sigma) from 32 to 145mJy. We here present galaxy number counts obtained for SPIRE observations of the first ~14 sq. deg. observed at 250, 350 and 500 microns. Methods. Number counts are a fundamental tool in constraining models of galaxy evolution. We use source catalogs extracted from the H-ATLAS maps as the basis for such an anal"},"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":"1005.2409","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-05-13T20:00:08Z","cross_cats_sorted":[],"title_canon_sha256":"a4760e1fc5755aeb0abc28f1a2af59b6fcaf3ac08474ea7aad54bbd36d0bed9f","abstract_canon_sha256":"602ce3451d15c507f1fd328226c05d8ba57792f47ec689eb5e463032d239c383"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:33.080823Z","signature_b64":"QR2LFfRBI5JiYAPGUKJE/CJGyP6OVXCQ47HSrh/kh4bXFO9rpW3VHbqBwDssmYX83SBXR66SKqHtZ7oI+YzsCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d7a08631a727e85395f4d60adb672e8da30d71d258771fd3da1e30efc38307ee","last_reissued_at":"2026-05-18T02:07:33.080190Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:33.080190Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Herschel-ATLAS: Extragalactic Number Counts from 250 to 500 Microns","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Cava, A. Cooray, A. Dariush, A. Mortier, A. Verma, B. Sibthorpe, C. Pearson, D. Bonfield, D. Burgarella, D. Frayer, D. Herranz, D.J.B. Smith, D.L. Clements, Douglas Scott, E. Ibar, E. Pascale, E. Rigby, G. de Zotti, G. Lagache, G. Rodighiero, I. Valtchanov, J. Fritz, J. Gonzalez-Nuevo, Jonathan P. Gardner, L. Dunne, L. Leeuw, M. Baes, M.J. Jarvis, M. Lopez-Caniego, M. Negrello, M. Pohlen, M. Thompson, P. Temi, P. van der Werf, R. Auld, R. Ivison, S. Buttiglione, S. Dye, S. Eales, S. Maddox, S. Samui, S. Serjeant","submitted_at":"2010-05-13T20:00:08Z","abstract_excerpt":"Aims. The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 microns when completed, reaching flux limits (5 sigma) from 32 to 145mJy. We here present galaxy number counts obtained for SPIRE observations of the first ~14 sq. deg. observed at 250, 350 and 500 microns. Methods. Number counts are a fundamental tool in constraining models of galaxy evolution. We use source catalogs extracted from the H-ATLAS maps as the basis for such an anal"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.2409","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":"1005.2409","created_at":"2026-05-18T02:07:33.080286+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.2409v1","created_at":"2026-05-18T02:07:33.080286+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.2409","created_at":"2026-05-18T02:07:33.080286+00:00"},{"alias_kind":"pith_short_12","alias_value":"26QIMMNHE7UF","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"26QIMMNHE7UFHFPU","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"26QIMMNH","created_at":"2026-05-18T12:26:03.138858+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/26QIMMNHE7UFHFPU2YFNWZZORW","json":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW.json","graph_json":"https://pith.science/api/pith-number/26QIMMNHE7UFHFPU2YFNWZZORW/graph.json","events_json":"https://pith.science/api/pith-number/26QIMMNHE7UFHFPU2YFNWZZORW/events.json","paper":"https://pith.science/paper/26QIMMNH"},"agent_actions":{"view_html":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW","download_json":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW.json","view_paper":"https://pith.science/paper/26QIMMNH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.2409&json=true","fetch_graph":"https://pith.science/api/pith-number/26QIMMNHE7UFHFPU2YFNWZZORW/graph.json","fetch_events":"https://pith.science/api/pith-number/26QIMMNHE7UFHFPU2YFNWZZORW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW/action/storage_attestation","attest_author":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW/action/author_attestation","sign_citation":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW/action/citation_signature","submit_replication":"https://pith.science/pith/26QIMMNHE7UFHFPU2YFNWZZORW/action/replication_record"}},"created_at":"2026-05-18T02:07:33.080286+00:00","updated_at":"2026-05-18T02:07:33.080286+00:00"}