{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:S246YMBC62B3T5XQHQ5MOQAPEH","short_pith_number":"pith:S246YMBC","schema_version":"1.0","canonical_sha256":"96b9ec3022f683b9f6f03c3ac7400f21fa18635ef863f94ce4a000108010b020","source":{"kind":"arxiv","id":"1306.1121","version":2},"attestation_state":"computed","paper":{"title":"Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"\\'A. Bongiovanni, A. Cimatti, A. Del Olmo, A. Ederoclite, A. Fernandez-Soto, A. Molino, A.M. P\\'erez-Garc\\'ia, A. Poglitsch, B. Altieri, B. Cedr\\'es, B. Magnelli, C. Husillos, D. Cristobal-Hornillos, D. Elbaz, D. Lutz, E. Daddi, E. J. Alfaro, E. Le Floc'h, E. Sturm, F. J. Castander, F. Pozzi, F. Prada, G. Magdis, H. Aussel, I. M\\'arquez, I. Matute, I. Oteo, I. Pintos-Castro, I. Valtchanov, J. A. L. Aguerri, J. Cabrera-Ca\\~no, J. Cepa, J. Masegosa, J. M. Quintana, J. Perea, J. Polednikova, K. Viironen, L. Infante, L. Riguccini, L. Tacconi, M. Cervi\\~no, M. Moles, M. Povi\\'c, M. S\\'anchez-Portal, N. Ben\\'itez, N. F\\\"orster Schreiber, P. Andreani, P. Popesso, R. Genzel, R. Maiolino, R. M. Gonzalez-Delgado, R. P\\'erez-Mart\\'inez, S. Berta, T. Aparicio-Villegas, T. Broadhurst, V. J. Mart\\'inez","submitted_at":"2013-06-05T14:40:58Z","abstract_excerpt":"We report the PACS-100um/160um detections of a sample of 42 GALEX-selected and FIR-detected Lyman break galaxies (LBGs) at z ~ 1 located in the COSMOS field and analyze their ultra-violet (UV) to far-infrared (FIR) properties. The detection of these LBGs in the FIR indicates that they have a dust content high enough so that its emission can be directly detected. According to a spectral energy distribution (SED) fitting with stellar population templates to their UV-to-near-IR observed photometry, PACS-detected LBGs tend to be bigger, more massive, dustier, redder in the UV continuum, and UV-bri"},"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":"1306.1121","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-06-05T14:40:58Z","cross_cats_sorted":[],"title_canon_sha256":"b55af286535393ada3bee8ae76bcfe6d6b47f35d0b1101a116fe1e79185c63e1","abstract_canon_sha256":"548c564af7d76cc88c5caf239f000c9fa624235efed33f37017e31f2e1d79097"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:32.498218Z","signature_b64":"+iVxe2Hrge/E2TEkFOyRDxqvx75+gQbMFpuyVT7vsKYQghnqJK1Ogr6WCkFWL+Zq2hf+qnMnvsYDZb18gisXCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96b9ec3022f683b9f6f03c3ac7400f21fa18635ef863f94ce4a000108010b020","last_reissued_at":"2026-05-18T01:49:32.497745Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:32.497745Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"\\'A. Bongiovanni, A. Cimatti, A. Del Olmo, A. Ederoclite, A. Fernandez-Soto, A. Molino, A.M. P\\'erez-Garc\\'ia, A. Poglitsch, B. Altieri, B. Cedr\\'es, B. Magnelli, C. Husillos, D. Cristobal-Hornillos, D. Elbaz, D. Lutz, E. Daddi, E. J. Alfaro, E. Le Floc'h, E. Sturm, F. J. Castander, F. Pozzi, F. Prada, G. Magdis, H. Aussel, I. M\\'arquez, I. Matute, I. Oteo, I. Pintos-Castro, I. Valtchanov, J. A. L. Aguerri, J. Cabrera-Ca\\~no, J. Cepa, J. Masegosa, J. M. Quintana, J. Perea, J. Polednikova, K. Viironen, L. Infante, L. Riguccini, L. Tacconi, M. Cervi\\~no, M. Moles, M. Povi\\'c, M. S\\'anchez-Portal, N. Ben\\'itez, N. F\\\"orster Schreiber, P. Andreani, P. Popesso, R. Genzel, R. Maiolino, R. M. Gonzalez-Delgado, R. P\\'erez-Mart\\'inez, S. Berta, T. Aparicio-Villegas, T. Broadhurst, V. J. Mart\\'inez","submitted_at":"2013-06-05T14:40:58Z","abstract_excerpt":"We report the PACS-100um/160um detections of a sample of 42 GALEX-selected and FIR-detected Lyman break galaxies (LBGs) at z ~ 1 located in the COSMOS field and analyze their ultra-violet (UV) to far-infrared (FIR) properties. The detection of these LBGs in the FIR indicates that they have a dust content high enough so that its emission can be directly detected. According to a spectral energy distribution (SED) fitting with stellar population templates to their UV-to-near-IR observed photometry, PACS-detected LBGs tend to be bigger, more massive, dustier, redder in the UV continuum, and UV-bri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.1121","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":"1306.1121","created_at":"2026-05-18T01:49:32.497822+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.1121v2","created_at":"2026-05-18T01:49:32.497822+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.1121","created_at":"2026-05-18T01:49:32.497822+00:00"},{"alias_kind":"pith_short_12","alias_value":"S246YMBC62B3","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"S246YMBC62B3T5XQ","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"S246YMBC","created_at":"2026-05-18T12:27:59.945178+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/S246YMBC62B3T5XQHQ5MOQAPEH","json":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH.json","graph_json":"https://pith.science/api/pith-number/S246YMBC62B3T5XQHQ5MOQAPEH/graph.json","events_json":"https://pith.science/api/pith-number/S246YMBC62B3T5XQHQ5MOQAPEH/events.json","paper":"https://pith.science/paper/S246YMBC"},"agent_actions":{"view_html":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH","download_json":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH.json","view_paper":"https://pith.science/paper/S246YMBC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.1121&json=true","fetch_graph":"https://pith.science/api/pith-number/S246YMBC62B3T5XQHQ5MOQAPEH/graph.json","fetch_events":"https://pith.science/api/pith-number/S246YMBC62B3T5XQHQ5MOQAPEH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH/action/storage_attestation","attest_author":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH/action/author_attestation","sign_citation":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH/action/citation_signature","submit_replication":"https://pith.science/pith/S246YMBC62B3T5XQHQ5MOQAPEH/action/replication_record"}},"created_at":"2026-05-18T01:49:32.497822+00:00","updated_at":"2026-05-18T01:49:32.497822+00:00"}