{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:R4WJDW3DYIX3G7O2O5WPJJ3LT4","short_pith_number":"pith:R4WJDW3D","schema_version":"1.0","canonical_sha256":"8f2c91db63c22fb37dda776cf4a76b9f14bea06e87800bfb714f704415bf40f9","source":{"kind":"arxiv","id":"1401.3228","version":1},"attestation_state":"computed","paper":{"title":"Search for [CII] emission in z=6.5-11 star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alberto D. Bolatto, Andrea Ferrara, Christopher L. Carilli, Dominik A. Riechers, Elisabete da Cunha, Fabian Walter, Frank Bertoldi, Jorge Gonz\\'alez-L\\'opez, Leopoldo Infante, Livia Vallini, Pierre Cox, Roberto Decarli, Roberto Neri, Simona Gallerani","submitted_at":"2014-01-14T15:44:13Z","abstract_excerpt":"We present the search for the [CII] emission line in three $z>6.5$ Lyman-alpha emitters (LAEs) and one J-Dropout galaxy using the Combined Array for Research in Millimeter-wave Astronomy (CARMA) and the Plateau de Bure Interferometer (PdBI). We observed three bright $z\\sim6.5-7$ LAEs discovered in the SUBARU deep field (SDF) and the Multiple Imaged lensed $z\\sim 11$ galaxy candidate found behind the galaxy cluster MACSJ0647.7+7015. For the LAEs IOK-1 ($z=6.965$), SDF J132415.7+273058 ($z=6.541$) and SDF J132408.3+271543 ($z=6.554$) we find upper limits for the [CII] line luminosity of $<2.05$,"},"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":"1401.3228","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-01-14T15:44:13Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"75c714aa294f4791fee47fc8dee8182914a6a3050e32a2a486c5b57a9f006db6","abstract_canon_sha256":"8c401798b74c19bd10e76524c8e8ebfceb0efe6f21deee769e5d0c9d200ee647"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:25.683936Z","signature_b64":"zBQyUIPfGsKP5EI7nnsxZu9TeKIPKuHp5WdORf1l1Y8DPPZTdyYTZ94beguo8GYYMEAvs1xvawIoCMqxlGWMCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f2c91db63c22fb37dda776cf4a76b9f14bea06e87800bfb714f704415bf40f9","last_reissued_at":"2026-05-18T01:45:25.683198Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:25.683198Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for [CII] emission in z=6.5-11 star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alberto D. Bolatto, Andrea Ferrara, Christopher L. Carilli, Dominik A. Riechers, Elisabete da Cunha, Fabian Walter, Frank Bertoldi, Jorge Gonz\\'alez-L\\'opez, Leopoldo Infante, Livia Vallini, Pierre Cox, Roberto Decarli, Roberto Neri, Simona Gallerani","submitted_at":"2014-01-14T15:44:13Z","abstract_excerpt":"We present the search for the [CII] emission line in three $z>6.5$ Lyman-alpha emitters (LAEs) and one J-Dropout galaxy using the Combined Array for Research in Millimeter-wave Astronomy (CARMA) and the Plateau de Bure Interferometer (PdBI). We observed three bright $z\\sim6.5-7$ LAEs discovered in the SUBARU deep field (SDF) and the Multiple Imaged lensed $z\\sim 11$ galaxy candidate found behind the galaxy cluster MACSJ0647.7+7015. For the LAEs IOK-1 ($z=6.965$), SDF J132415.7+273058 ($z=6.541$) and SDF J132408.3+271543 ($z=6.554$) we find upper limits for the [CII] line luminosity of $<2.05$,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.3228","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":"1401.3228","created_at":"2026-05-18T01:45:25.683335+00:00"},{"alias_kind":"arxiv_version","alias_value":"1401.3228v1","created_at":"2026-05-18T01:45:25.683335+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.3228","created_at":"2026-05-18T01:45:25.683335+00:00"},{"alias_kind":"pith_short_12","alias_value":"R4WJDW3DYIX3","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"R4WJDW3DYIX3G7O2","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"R4WJDW3D","created_at":"2026-05-18T12:28:46.137349+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/R4WJDW3DYIX3G7O2O5WPJJ3LT4","json":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4.json","graph_json":"https://pith.science/api/pith-number/R4WJDW3DYIX3G7O2O5WPJJ3LT4/graph.json","events_json":"https://pith.science/api/pith-number/R4WJDW3DYIX3G7O2O5WPJJ3LT4/events.json","paper":"https://pith.science/paper/R4WJDW3D"},"agent_actions":{"view_html":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4","download_json":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4.json","view_paper":"https://pith.science/paper/R4WJDW3D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1401.3228&json=true","fetch_graph":"https://pith.science/api/pith-number/R4WJDW3DYIX3G7O2O5WPJJ3LT4/graph.json","fetch_events":"https://pith.science/api/pith-number/R4WJDW3DYIX3G7O2O5WPJJ3LT4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4/action/storage_attestation","attest_author":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4/action/author_attestation","sign_citation":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4/action/citation_signature","submit_replication":"https://pith.science/pith/R4WJDW3DYIX3G7O2O5WPJJ3LT4/action/replication_record"}},"created_at":"2026-05-18T01:45:25.683335+00:00","updated_at":"2026-05-18T01:45:25.683335+00:00"}