{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:R47WL3SLCRTYVWPWGGTM6AGXIW","short_pith_number":"pith:R47WL3SL","schema_version":"1.0","canonical_sha256":"8f3f65ee4b14678ad9f631a6cf00d74582aef79a0635534771070a455bf8400d","source":{"kind":"arxiv","id":"1201.2908","version":2},"attestation_state":"computed","paper":{"title":"A bright z=5.2 lensed submillimeter galaxy in the field of Abell 773: HLSJ091828.6+514223","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Berciano Alba (ASTRON), A.C. Edge (Durham), A.M. Swinbank (Durham), A. Omont (IAP-Paris), C.M. Casey (Hawaii), D. Schaerer (Geneva), E. Egami (Tucson), F. Boone (Toulouse), F. Combes (Obs-Paris), G.G. Fazio (Harvard), G.P. Smith (Birmingham), I. Smail (Durham), J-P. Kneib (Marseille), J. Richard (Lyon), M. Dessauges-Zavadsky (Geneva), M. Gurwell (Harvard), M. Rex (Tucson), N. Okabe (Taipei), P. G. Perez-Gonzalez (Madrid), P. van der Werf (Leiden), R.J. Ivison (Edinburgh), R. Pello (Toulouse), T. D. Rawle (Tucson)","submitted_at":"2012-01-13T18:38:06Z","abstract_excerpt":"During our Herschel Lensing Survey (HLS) of massive galaxy clusters, we have discovered an exceptionally bright source behind the z=0.22 cluster Abell 773, which appears to be a strongly lensed submillimeter galaxy (SMG) at z=5.2429. This source is unusual compared to most other lensed sources discovered by Herschel so far, because of its higher submm flux (\\sim 200mJy at 500\\micron) and its high redshift. The dominant lens is a foreground z=0.63 galaxy, not the cluster itself. The source has a far-infrared (FIR) luminosity of L_FIR= 1.1 10^{14}/\\mu Lo, where \\mu is the magnification factor, l"},"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":"1201.2908","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-01-13T18:38:06Z","cross_cats_sorted":[],"title_canon_sha256":"0a94c3967b9334ec1621a82080553d923d08e3179738d35cfe417add760002da","abstract_canon_sha256":"07e9dddd2dc85a343ab3d38dc795a7a7b666425bacc4f259f9e794ebff13d6b9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:49.513448Z","signature_b64":"wiY2pOXtuK69LoBsyBAMv81ZMvWHJgQkbsAROmzpK3bQtjsgbTp4pZrvHq73kJ014wHg9Y0HnR+hqM8EiHR+Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f3f65ee4b14678ad9f631a6cf00d74582aef79a0635534771070a455bf8400d","last_reissued_at":"2026-05-18T01:58:49.512804Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:49.512804Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A bright z=5.2 lensed submillimeter galaxy in the field of Abell 773: HLSJ091828.6+514223","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Berciano Alba (ASTRON), A.C. Edge (Durham), A.M. Swinbank (Durham), A. Omont (IAP-Paris), C.M. Casey (Hawaii), D. Schaerer (Geneva), E. Egami (Tucson), F. Boone (Toulouse), F. Combes (Obs-Paris), G.G. Fazio (Harvard), G.P. Smith (Birmingham), I. Smail (Durham), J-P. Kneib (Marseille), J. Richard (Lyon), M. Dessauges-Zavadsky (Geneva), M. Gurwell (Harvard), M. Rex (Tucson), N. Okabe (Taipei), P. G. Perez-Gonzalez (Madrid), P. van der Werf (Leiden), R.J. Ivison (Edinburgh), R. Pello (Toulouse), T. D. Rawle (Tucson)","submitted_at":"2012-01-13T18:38:06Z","abstract_excerpt":"During our Herschel Lensing Survey (HLS) of massive galaxy clusters, we have discovered an exceptionally bright source behind the z=0.22 cluster Abell 773, which appears to be a strongly lensed submillimeter galaxy (SMG) at z=5.2429. This source is unusual compared to most other lensed sources discovered by Herschel so far, because of its higher submm flux (\\sim 200mJy at 500\\micron) and its high redshift. The dominant lens is a foreground z=0.63 galaxy, not the cluster itself. The source has a far-infrared (FIR) luminosity of L_FIR= 1.1 10^{14}/\\mu Lo, where \\mu is the magnification factor, l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.2908","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":"1201.2908","created_at":"2026-05-18T01:58:49.512903+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.2908v2","created_at":"2026-05-18T01:58:49.512903+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.2908","created_at":"2026-05-18T01:58:49.512903+00:00"},{"alias_kind":"pith_short_12","alias_value":"R47WL3SLCRTY","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"R47WL3SLCRTYVWPW","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"R47WL3SL","created_at":"2026-05-18T12:27:20.899486+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/R47WL3SLCRTYVWPWGGTM6AGXIW","json":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW.json","graph_json":"https://pith.science/api/pith-number/R47WL3SLCRTYVWPWGGTM6AGXIW/graph.json","events_json":"https://pith.science/api/pith-number/R47WL3SLCRTYVWPWGGTM6AGXIW/events.json","paper":"https://pith.science/paper/R47WL3SL"},"agent_actions":{"view_html":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW","download_json":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW.json","view_paper":"https://pith.science/paper/R47WL3SL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.2908&json=true","fetch_graph":"https://pith.science/api/pith-number/R47WL3SLCRTYVWPWGGTM6AGXIW/graph.json","fetch_events":"https://pith.science/api/pith-number/R47WL3SLCRTYVWPWGGTM6AGXIW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW/action/storage_attestation","attest_author":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW/action/author_attestation","sign_citation":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW/action/citation_signature","submit_replication":"https://pith.science/pith/R47WL3SLCRTYVWPWGGTM6AGXIW/action/replication_record"}},"created_at":"2026-05-18T01:58:49.512903+00:00","updated_at":"2026-05-18T01:58:49.512903+00:00"}