{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:ECVR45FWKVBRPTP5XWRHYQYMPW","short_pith_number":"pith:ECVR45FW","schema_version":"1.0","canonical_sha256":"20ab1e74b6554317cdfdbda27c430c7db6c5f701ea377005e91ad7f39d71a503","source":{"kind":"arxiv","id":"2504.12504","version":1},"attestation_state":"computed","paper":{"title":"CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anthony J. Taylor, Anton M. Koekemoer, Caitlin M. Casey, Callum T. Donnan, Casey Papovich, Derek McLeod, Emanuele Daddi, Fergus Cullen, Ho-Hin Leung, Hollis B. Akins, James S. Dunlop, Jeyhan S. Kartaltepe, John Chisholm, Jorge A. Zavala, Julian B.Mu\\~noz, Justin Cole, Kelcey Davis, Laura Pentericci, Lorenzo Napolitano, L. Y. Aaron Yung, Mark Dickinson, Mauro Giavalisco, Michaela Hirschmann, Nikko J. Cleri, Nimish Hathi, Norman A. Grogin, \\'Oscar A. Ch\\'avez Ortiz, Pablo Arrabal Haro, Pablo G. P\\'erez-Gonz\\'alez, Rachel S. Somerville, Ray A. Lucas, Ricardo Amori\\'in, Ryan Endsley, Seiji Fujimoto, Stephen M. Wilkins, Steven L. Finkelstein, Vasily Kokorev, Vital Fern\\'andez, Weida Hu, Xin Wang, Yingjie Cheng","submitted_at":"2025-04-16T21:45:04Z","abstract_excerpt":"We present the first results from the CAPERS survey, utilizing PRISM observations with the JWST/NIRSpec MSA in the PRIMER-UDS field. With just 14 % of the total planned data volume, we spectroscopically confirm two new bright galaxies ($M_{\\rm UV}\\sim -20.4$) at redshifts $z = 10.562\\pm0.034$ and $z = 11.013\\pm0.028$. We examine their physical properties, morphologies, and star formation histories, finding evidence for recent bursting star formation in at least one galaxy thanks to the detection of strong (EW$_0\\sim70$ A) H$\\gamma$ emission. Combining our findings with previous studies of simi"},"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":"2504.12504","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-04-16T21:45:04Z","cross_cats_sorted":[],"title_canon_sha256":"e05095d41baec8fee6fb6d6b1a4731c21c30a3bdfa45a09813ff6feb41f124a1","abstract_canon_sha256":"7dd3ebd697747e62b69a30a6c139eaf3465596ffd471ccb2cf1988bd9306518b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:50:17.555927Z","signature_b64":"H0Og/KcNSURQuD4qF0icMzFF6GFyFwsw5Uz0qNHNenMEzRNbfg/uIqZBnEdSKUYtawk/OGCrAs2980MznYQtDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"20ab1e74b6554317cdfdbda27c430c7db6c5f701ea377005e91ad7f39d71a503","last_reissued_at":"2026-07-05T10:50:17.555384Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:50:17.555384Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anthony J. Taylor, Anton M. Koekemoer, Caitlin M. Casey, Callum T. Donnan, Casey Papovich, Derek McLeod, Emanuele Daddi, Fergus Cullen, Ho-Hin Leung, Hollis B. Akins, James S. Dunlop, Jeyhan S. Kartaltepe, John Chisholm, Jorge A. Zavala, Julian B.Mu\\~noz, Justin Cole, Kelcey Davis, Laura Pentericci, Lorenzo Napolitano, L. Y. Aaron Yung, Mark Dickinson, Mauro Giavalisco, Michaela Hirschmann, Nikko J. Cleri, Nimish Hathi, Norman A. Grogin, \\'Oscar A. Ch\\'avez Ortiz, Pablo Arrabal Haro, Pablo G. P\\'erez-Gonz\\'alez, Rachel S. Somerville, Ray A. Lucas, Ricardo Amori\\'in, Ryan Endsley, Seiji Fujimoto, Stephen M. Wilkins, Steven L. Finkelstein, Vasily Kokorev, Vital Fern\\'andez, Weida Hu, Xin Wang, Yingjie Cheng","submitted_at":"2025-04-16T21:45:04Z","abstract_excerpt":"We present the first results from the CAPERS survey, utilizing PRISM observations with the JWST/NIRSpec MSA in the PRIMER-UDS field. With just 14 % of the total planned data volume, we spectroscopically confirm two new bright galaxies ($M_{\\rm UV}\\sim -20.4$) at redshifts $z = 10.562\\pm0.034$ and $z = 11.013\\pm0.028$. We examine their physical properties, morphologies, and star formation histories, finding evidence for recent bursting star formation in at least one galaxy thanks to the detection of strong (EW$_0\\sim70$ A) H$\\gamma$ emission. Combining our findings with previous studies of simi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.12504","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2504.12504/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2504.12504","created_at":"2026-07-05T10:50:17.555447+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.12504v1","created_at":"2026-07-05T10:50:17.555447+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.12504","created_at":"2026-07-05T10:50:17.555447+00:00"},{"alias_kind":"pith_short_12","alias_value":"ECVR45FWKVBR","created_at":"2026-07-05T10:50:17.555447+00:00"},{"alias_kind":"pith_short_16","alias_value":"ECVR45FWKVBRPTP5","created_at":"2026-07-05T10:50:17.555447+00:00"},{"alias_kind":"pith_short_8","alias_value":"ECVR45FW","created_at":"2026-07-05T10:50:17.555447+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08749","citing_title":"Deep Spectroscopic Follow-Up of Maisie's Galaxy -- A Typical Galaxy in the Early Universe","ref_index":63,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30787","citing_title":"JWST spectroscopy of galaxies at $z>10$: Damped Ly$\\alpha$ absorbers reveal efficient star formation and hidden redshift biases","ref_index":101,"is_internal_anchor":false},{"citing_arxiv_id":"2606.17271","citing_title":"Black Hole Stars Across the Universe: Identifying Central Engine Dominated Little Red Dots at $z\\sim1.5-9.5$","ref_index":83,"is_internal_anchor":false},{"citing_arxiv_id":"2605.22914","citing_title":"No Blue without Red: Evolutionary Properties of Super-Early Galaxies","ref_index":44,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW","json":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW.json","graph_json":"https://pith.science/api/pith-number/ECVR45FWKVBRPTP5XWRHYQYMPW/graph.json","events_json":"https://pith.science/api/pith-number/ECVR45FWKVBRPTP5XWRHYQYMPW/events.json","paper":"https://pith.science/paper/ECVR45FW"},"agent_actions":{"view_html":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW","download_json":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW.json","view_paper":"https://pith.science/paper/ECVR45FW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.12504&json=true","fetch_graph":"https://pith.science/api/pith-number/ECVR45FWKVBRPTP5XWRHYQYMPW/graph.json","fetch_events":"https://pith.science/api/pith-number/ECVR45FWKVBRPTP5XWRHYQYMPW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW/action/storage_attestation","attest_author":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW/action/author_attestation","sign_citation":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW/action/citation_signature","submit_replication":"https://pith.science/pith/ECVR45FWKVBRPTP5XWRHYQYMPW/action/replication_record"}},"created_at":"2026-07-05T10:50:17.555447+00:00","updated_at":"2026-07-05T10:50:17.555447+00:00"}