{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:GEMI356TIAOYH2B4DDBWFVAY77","short_pith_number":"pith:GEMI356T","schema_version":"1.0","canonical_sha256":"31188df7d3401d83e83c18c362d418fff58e404780dce74fcd1eae2120883a19","source":{"kind":"arxiv","id":"2208.01816","version":3},"attestation_state":"computed","paper":{"title":"Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adriano Fontana, Alexa M. Morales, Alexander de la Vega, Allison Kirkpatrick, Amber N. Straughn, Andrea Grazian, \\'Angela Garc\\'ia-Argum\\'anez, Anne E. Jaskot, Antonello Calabro, Anton M. Koekemoer, Arianna Long, Asantha R. Cooray, Aubrey Medrano, Aur\\'elien Le Bail, Avishai Dekel, Bahram Mobasher, Benjamin J. Weiner, Benjamin Magnelli, Benne W. Holwerda, Bren E. Backhaus, Brittany N. Vanderhoof, Caitlin M. Casey, Caitlin Rose, Carlos G\\'omez-Guijarro, Casey Papovich, Christopher N. A. Willmer, Dale D. Kocevski, Daniel H. McIntosh, Darren Croton, David C. Nicholls, David Elbaz, Denis Burgarella, E. F. Jim'enez-Andrade, E. J. Murphy, Ekta A. Shah, Elizabeth J. McGrath, Elizabeth R. Stanway, Emanuele Daddi, Emiliano Merlin, Eric F. Bell, Eric Gawiser, Fernando Buitrago, Gene C. K. Leung, Gregory F. Snyder, Guang Yang, Guillermo Barro, Harry I. Teplitz, Henry C. Ferguson, Intae Jung, Isabella G. Cox, Itziar Aretxaga, Jaclyn B. Champagne, Jasleen Matharu, Jeffrey A. Newman, Jennifer M. Lotz, Jes\\'us Vega-Ferrero, Jeyhan S. Kartaltepe, Jonathan Freundlich, Jonathan P. Gardner, Jonathan R. Trump, Jorge A. Zavala, Justin W. Cole, Kaila Ronayne, Kameswara Bharadwaj Mantha, Kartheik G. Iyer, Katherine Chworowsky, Keely D. Finkelstein, Kevin C. Cooke, Laura Bisigello, Laura Pentericci, Laure Ciesla, Lisa J. Kewley, Lise-Marie Seill\\'e, Luca Costantin, Lu Shen, L. Y. Aaron Yung, Marc Huertas-Company, Marco Castellano, Marc Rafelski, Marianna Annunziatella, Mark Dickinson, Mauro Giavalisco, Maximilien Franco, M. C. Cooper, Micaela B. Bagley, Michaela Hirschmann, Nikko J. Cleri, Nimish P. Hathi, Norman A. Grogin, Nor Pirzkal, Omar Almaini, Oscar A. Chavez Ortiz, Pablo Arrabal Haro, Pablo G. Perez-Gonzalez, Paola Santini, Peter Behroozi, Peter Kurczynski, Rachana Bhatawdekar, Rachel S. Somerville, Ray A. Lucas, Raymond C. Simons, Rebecca L. Larson, Ricardo O. Amorin, Romeel Dave, Russell E. Ryan Jr., Sandro Tacchella, Saurabh W. Jha, Seiji Fujimoto, Seth H. Cohen, Shardha Jogee, St\\'ephanie Juneau, Stephen M. Wilkins, Steven L. Finkelstein, Stijn Wuyts, Susan A. Kassin, Swara Ravindranath, Taylor A. Hutchison, Timothy S. Hamilton, Veronique Buat, Vicente Estrada-Carpenter, Viraj Pandya, Vital Fern\\'andez, Weichen Wang, Yuchen Guo","submitted_at":"2022-08-03T02:25:02Z","abstract_excerpt":"Lyman Break Galaxy (LBG) candidates at z>10 are rapidly being identified in JWST/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-frame UV photons, these sources are expected to drop out in the bluer filters while being well detected in redder filters. However, here we show that dust-enshrouded star-forming galaxies at lower redshifts (z<7) may also mimic the near-infrared (near-IR) colors of z>10 LBGs, representing potential contaminants in LBG candidate samples. First, we analyze CEERS-DSFG-1, a NIRCam dropout undetected in the F115W and F150"},"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":"2208.01816","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-08-03T02:25:02Z","cross_cats_sorted":[],"title_canon_sha256":"1984e82451a4cae3f7ef22ea7a91e05175a111c9641399fad362345fd4e53d89","abstract_canon_sha256":"db6159f6e91aaaf77f822884c57b8d3e7f8b8af37593f1d2c478634838859282"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:36:48.938491Z","signature_b64":"s3AN6+Y2N3AFsHpo9zyodJaS06NsJBoVf+zX3qfPfkOVTVKUY0O9MQS8fApCIn8AyovO/tDZnGb6Ty1/62TICg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"31188df7d3401d83e83c18c362d418fff58e404780dce74fcd1eae2120883a19","last_reissued_at":"2026-07-05T05:36:48.937925Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:36:48.937925Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adriano Fontana, Alexa M. Morales, Alexander de la Vega, Allison Kirkpatrick, Amber N. Straughn, Andrea Grazian, \\'Angela Garc\\'ia-Argum\\'anez, Anne E. Jaskot, Antonello Calabro, Anton M. Koekemoer, Arianna Long, Asantha R. Cooray, Aubrey Medrano, Aur\\'elien Le Bail, Avishai Dekel, Bahram Mobasher, Benjamin J. Weiner, Benjamin Magnelli, Benne W. Holwerda, Bren E. Backhaus, Brittany N. Vanderhoof, Caitlin M. Casey, Caitlin Rose, Carlos G\\'omez-Guijarro, Casey Papovich, Christopher N. A. Willmer, Dale D. Kocevski, Daniel H. McIntosh, Darren Croton, David C. Nicholls, David Elbaz, Denis Burgarella, E. F. Jim'enez-Andrade, E. J. Murphy, Ekta A. Shah, Elizabeth J. McGrath, Elizabeth R. Stanway, Emanuele Daddi, Emiliano Merlin, Eric F. Bell, Eric Gawiser, Fernando Buitrago, Gene C. K. Leung, Gregory F. Snyder, Guang Yang, Guillermo Barro, Harry I. Teplitz, Henry C. Ferguson, Intae Jung, Isabella G. Cox, Itziar Aretxaga, Jaclyn B. Champagne, Jasleen Matharu, Jeffrey A. Newman, Jennifer M. Lotz, Jes\\'us Vega-Ferrero, Jeyhan S. Kartaltepe, Jonathan Freundlich, Jonathan P. Gardner, Jonathan R. Trump, Jorge A. Zavala, Justin W. Cole, Kaila Ronayne, Kameswara Bharadwaj Mantha, Kartheik G. Iyer, Katherine Chworowsky, Keely D. Finkelstein, Kevin C. Cooke, Laura Bisigello, Laura Pentericci, Laure Ciesla, Lisa J. Kewley, Lise-Marie Seill\\'e, Luca Costantin, Lu Shen, L. Y. Aaron Yung, Marc Huertas-Company, Marco Castellano, Marc Rafelski, Marianna Annunziatella, Mark Dickinson, Mauro Giavalisco, Maximilien Franco, M. C. Cooper, Micaela B. Bagley, Michaela Hirschmann, Nikko J. Cleri, Nimish P. Hathi, Norman A. Grogin, Nor Pirzkal, Omar Almaini, Oscar A. Chavez Ortiz, Pablo Arrabal Haro, Pablo G. Perez-Gonzalez, Paola Santini, Peter Behroozi, Peter Kurczynski, Rachana Bhatawdekar, Rachel S. Somerville, Ray A. Lucas, Raymond C. Simons, Rebecca L. Larson, Ricardo O. Amorin, Romeel Dave, Russell E. Ryan Jr., Sandro Tacchella, Saurabh W. Jha, Seiji Fujimoto, Seth H. Cohen, Shardha Jogee, St\\'ephanie Juneau, Stephen M. Wilkins, Steven L. Finkelstein, Stijn Wuyts, Susan A. Kassin, Swara Ravindranath, Taylor A. Hutchison, Timothy S. Hamilton, Veronique Buat, Vicente Estrada-Carpenter, Viraj Pandya, Vital Fern\\'andez, Weichen Wang, Yuchen Guo","submitted_at":"2022-08-03T02:25:02Z","abstract_excerpt":"Lyman Break Galaxy (LBG) candidates at z>10 are rapidly being identified in JWST/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-frame UV photons, these sources are expected to drop out in the bluer filters while being well detected in redder filters. However, here we show that dust-enshrouded star-forming galaxies at lower redshifts (z<7) may also mimic the near-infrared (near-IR) colors of z>10 LBGs, representing potential contaminants in LBG candidate samples. First, we analyze CEERS-DSFG-1, a NIRCam dropout undetected in the F115W and F150"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.01816","kind":"arxiv","version":3},"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/2208.01816/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":"2208.01816","created_at":"2026-07-05T05:36:48.938003+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.01816v3","created_at":"2026-07-05T05:36:48.938003+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.01816","created_at":"2026-07-05T05:36:48.938003+00:00"},{"alias_kind":"pith_short_12","alias_value":"GEMI356TIAOY","created_at":"2026-07-05T05:36:48.938003+00:00"},{"alias_kind":"pith_short_16","alias_value":"GEMI356TIAOYH2B4","created_at":"2026-07-05T05:36:48.938003+00:00"},{"alias_kind":"pith_short_8","alias_value":"GEMI356T","created_at":"2026-07-05T05:36:48.938003+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.10005","citing_title":"On Cross-Correlating Line Intensity Maps from SPHEREx during Reionization","ref_index":57,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77","json":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77.json","graph_json":"https://pith.science/api/pith-number/GEMI356TIAOYH2B4DDBWFVAY77/graph.json","events_json":"https://pith.science/api/pith-number/GEMI356TIAOYH2B4DDBWFVAY77/events.json","paper":"https://pith.science/paper/GEMI356T"},"agent_actions":{"view_html":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77","download_json":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77.json","view_paper":"https://pith.science/paper/GEMI356T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.01816&json=true","fetch_graph":"https://pith.science/api/pith-number/GEMI356TIAOYH2B4DDBWFVAY77/graph.json","fetch_events":"https://pith.science/api/pith-number/GEMI356TIAOYH2B4DDBWFVAY77/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77/action/storage_attestation","attest_author":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77/action/author_attestation","sign_citation":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77/action/citation_signature","submit_replication":"https://pith.science/pith/GEMI356TIAOYH2B4DDBWFVAY77/action/replication_record"}},"created_at":"2026-07-05T05:36:48.938003+00:00","updated_at":"2026-07-05T05:36:48.938003+00:00"}