{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:P5CPN5XHXRZKR4ES46V3IA6TL4","short_pith_number":"pith:P5CPN5XH","schema_version":"1.0","canonical_sha256":"7f44f6f6e7bc72a8f092e7abb403d35f15ca3dd556b43525dffbdc196b395af2","source":{"kind":"arxiv","id":"2306.02465","version":2},"attestation_state":"computed","paper":{"title":"Overview of the JWST Advanced Deep Extragalactic Survey (JADES)","license":"http://creativecommons.org/licenses/by/4.0/","headline":"JADES allocates 770 hours of JWST time to deep NIRCam imaging over 42 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS fields.","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aayush Saxena, Alan Dressler, Alex J. Cameron, A. Lola Danhaive, Andrew J. Bunker, Anna de Graaff, Benjamin D. Johnson, Bernard J. Rauscher, Brant Robertson, Bruno Rodr\\'iguez Del Pino, Charity Woodrum, Charlotte Simmonds, Chiara Circosta, Christa DeCoursey, Christina C. Williams, Christopher N. A. Willmer, Chris Willott, Daniel J. Eisenstein, Daniel P. Stark, D\\'avid Pusk\\'as, Eiichi Egami, Eleonora Parlanti, Emma Curtis-Lake, Erica Nelson, Fengwu Sun, Francesco D'Eugenio, Gareth C. Jones, George Rieke, Giovanna Giardino, Hannah \\\"Ubler, Hans-Walter Rix, Imaan E. B. Wallace, Irene Shivaei, Isaac Laseter, Jacopo Chevallard, Jakob M. Helton, Jan Scholtz, Jianwei Lyu, Joris Witstok, Katherine A. Suess, Katherine Sharpe, Kevin Hainline, Kristan Boyett, Lester Sandles, Lily Whitler, Maddie S. Silcock, Marcia Rieke, Maya Skarbinski, Mengtao Tang, Meredith Stone, Michael V. Maseda, Michael W. Topping, Michele Perna, Mirko Curti, Natalia C. Villanueva, Nimisha Kumari, Nina Bonaventura, Nora L\\\"utzgendorf, Peter Jakobsen, Pierre Ferruit, Rachana Bhatawdekar, Raphael E. Hviding, Renske Smit, Roberto Maiolino, Ryan Endsley, Ryan Hausen, Sandro Tacchella, Santiago Arribas, Stacey Alberts, Stefano Carniani, Stefi Baum, Stephane Charlot, Tim Rawle, Tobias J. Looser, William M. Baker, Wiphu Rujopakarn, Zhiyuan Ji, Zuyi Chen","submitted_at":"2023-06-04T20:44:21Z","abstract_excerpt":"We present an overview of the James Webb Space Telescope (JWST) Advanced Deep Extragalactic Survey (JADES), an ambitious program of infrared imaging and spectroscopy in the GOODS-S and GOODS-N deep fields, designed to study galaxy evolution from high redshift to cosmic noon. JADES uses about 770 hours of Cycle 1 guaranteed time largely from the Near-Infrared Camera (NIRCam) and Near-Infrared Spectrograph (NIRSpec) instrument teams. In GOODS-S, in and around the Hubble Ultra Deep Field and Chandra Deep Field South, JADES produces a deep imaging region of ~42 arcmin^2 with over 100 hrs of exposu"},"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":true,"formal_links_present":true},"canonical_record":{"source":{"id":"2306.02465","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-06-04T20:44:21Z","cross_cats_sorted":[],"title_canon_sha256":"6da326f9568fe7c9f209cc119afb193c629b129323540075ea3ba3774f63e1fa","abstract_canon_sha256":"636ab457802e09f3c7cf687eb7fa3ec52b55cb46690ad62c6fa59a298929a30a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:38:47.598301Z","signature_b64":"CTF8OK1npxDsQPmLuN6NyNFpvMplXAGNtjG/3E5bu02+Wr5mZISoWA4QDA40+loEAR0kMZySM9mZBUCUr3RADg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7f44f6f6e7bc72a8f092e7abb403d35f15ca3dd556b43525dffbdc196b395af2","last_reissued_at":"2026-05-17T23:38:47.597829Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:38:47.597829Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Overview of the JWST Advanced Deep Extragalactic Survey (JADES)","license":"http://creativecommons.org/licenses/by/4.0/","headline":"JADES allocates 770 hours of JWST time to deep NIRCam imaging over 42 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS fields.","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aayush Saxena, Alan Dressler, Alex J. Cameron, A. Lola Danhaive, Andrew J. Bunker, Anna de Graaff, Benjamin D. Johnson, Bernard J. Rauscher, Brant Robertson, Bruno Rodr\\'iguez Del Pino, Charity Woodrum, Charlotte Simmonds, Chiara Circosta, Christa DeCoursey, Christina C. Williams, Christopher N. A. Willmer, Chris Willott, Daniel J. Eisenstein, Daniel P. Stark, D\\'avid Pusk\\'as, Eiichi Egami, Eleonora Parlanti, Emma Curtis-Lake, Erica Nelson, Fengwu Sun, Francesco D'Eugenio, Gareth C. Jones, George Rieke, Giovanna Giardino, Hannah \\\"Ubler, Hans-Walter Rix, Imaan E. B. Wallace, Irene Shivaei, Isaac Laseter, Jacopo Chevallard, Jakob M. Helton, Jan Scholtz, Jianwei Lyu, Joris Witstok, Katherine A. Suess, Katherine Sharpe, Kevin Hainline, Kristan Boyett, Lester Sandles, Lily Whitler, Maddie S. Silcock, Marcia Rieke, Maya Skarbinski, Mengtao Tang, Meredith Stone, Michael V. Maseda, Michael W. Topping, Michele Perna, Mirko Curti, Natalia C. Villanueva, Nimisha Kumari, Nina Bonaventura, Nora L\\\"utzgendorf, Peter Jakobsen, Pierre Ferruit, Rachana Bhatawdekar, Raphael E. Hviding, Renske Smit, Roberto Maiolino, Ryan Endsley, Ryan Hausen, Sandro Tacchella, Santiago Arribas, Stacey Alberts, Stefano Carniani, Stefi Baum, Stephane Charlot, Tim Rawle, Tobias J. Looser, William M. Baker, Wiphu Rujopakarn, Zhiyuan Ji, Zuyi Chen","submitted_at":"2023-06-04T20:44:21Z","abstract_excerpt":"We present an overview of the James Webb Space Telescope (JWST) Advanced Deep Extragalactic Survey (JADES), an ambitious program of infrared imaging and spectroscopy in the GOODS-S and GOODS-N deep fields, designed to study galaxy evolution from high redshift to cosmic noon. JADES uses about 770 hours of Cycle 1 guaranteed time largely from the Near-Infrared Camera (NIRCam) and Near-Infrared Spectrograph (NIRSpec) instrument teams. In GOODS-S, in and around the Hubble Ultra Deep Field and Chandra Deep Field South, JADES produces a deep imaging region of ~42 arcmin^2 with over 100 hrs of exposu"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"JADES uses about 770 hours of Cycle 1 guaranteed time largely from the Near-Infrared Camera (NIRCam) and Near-Infrared Spectrograph (NIRSpec) instrument teams. In GOODS-S, in and around the Hubble Ultra Deep Field and Chandra Deep Field South, JADES produces a deep imaging region of ~42 arcmin² with over 100 hrs of exposure time spread over 9 NIRCam filters... targeting over 5000 HST and JWST-detected faint sources.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The survey design assumes that the allocated JWST observing time, instrument performance, and scheduling will achieve the stated exposure depths, areas, and target yields without significant losses from overheads or technical issues.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"JADES is a 770-hour JWST Cycle 1 survey delivering deep multi-band NIRCam imaging over ~209 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS-S and GOODS-N fields to study galaxy evolution from high redshift to cosmic noon.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"JADES allocates 770 hours of JWST time to deep NIRCam imaging over 42 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS fields.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"16836ccfd4b0eb8f5afb34df2cab33589a6d52d89761371c7e86e2e4a906706e"},"source":{"id":"2306.02465","kind":"arxiv","version":2},"verdict":{"id":"a7d81093-669f-4741-9fa8-736e63d027a3","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-16T14:28:11.923827Z","strongest_claim":"JADES uses about 770 hours of Cycle 1 guaranteed time largely from the Near-Infrared Camera (NIRCam) and Near-Infrared Spectrograph (NIRSpec) instrument teams. In GOODS-S, in and around the Hubble Ultra Deep Field and Chandra Deep Field South, JADES produces a deep imaging region of ~42 arcmin² with over 100 hrs of exposure time spread over 9 NIRCam filters... targeting over 5000 HST and JWST-detected faint sources.","one_line_summary":"JADES is a 770-hour JWST Cycle 1 survey delivering deep multi-band NIRCam imaging over ~209 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS-S and GOODS-N fields to study galaxy evolution from high redshift to cosmic noon.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The survey design assumes that the allocated JWST observing time, instrument performance, and scheduling will achieve the stated exposure depths, areas, and target yields without significant losses from overheads or technical issues.","pith_extraction_headline":"JADES allocates 770 hours of JWST time to deep NIRCam imaging over 42 arcmin² and NIRSpec spectroscopy of over 5000 sources in the GOODS fields."},"references":{"count":119,"sample":[{"doi":"","year":2023,"title":"Akins, H. B., Casey, C. M., Allen, N., et al. 2023, ApJ, 956, 61","work_id":"f99b1c7b-ee2c-4c18-a7b3-361be359b766","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2022,"title":"2022, Universe, 8, 554","work_id":"3b80a5b9-1946-4968-a1ca-1f2e94fd3054","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2020,"title":"H., Jagannathan, P., & Nyland, K","work_id":"fd37bbe9-757d-4a60-955b-3437335ce44d","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2024,"title":"2024, ApJ, 976, 224","work_id":"54f191f4-7b2c-437e-b405-db9ab7bbeebe","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2023,"title":"Algera, H. S. B., Inami, H., Oesch, P. A., et al. 2023, MNRAS, 518, 6142 Arrabal Haro, P., Dickinson, M., Finkelstein, S. L., et al. 2023, Nature, 622, 707","work_id":"718ac296-f2b4-4dbc-ba36-96e0202e084e","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":119,"snapshot_sha256":"5b1d6a51ebb1bae4147c6e7bf7ac0b2987e16e8f71e7c7cc2b1ff2199b91ac6f","internal_anchors":1},"formal_canon":{"evidence_count":1,"snapshot_sha256":"50ee39232ea79f6d602a4cb58f9a603150f0a014113bd0170efe5e6223f11325"},"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":"2306.02465","created_at":"2026-05-17T23:38:47.597899+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.02465v2","created_at":"2026-05-17T23:38:47.597899+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.02465","created_at":"2026-05-17T23:38:47.597899+00:00"},{"alias_kind":"pith_short_12","alias_value":"P5CPN5XHXRZK","created_at":"2026-05-18T12:33:37.589309+00:00"},{"alias_kind":"pith_short_16","alias_value":"P5CPN5XHXRZKR4ES","created_at":"2026-05-18T12:33:37.589309+00:00"},{"alias_kind":"pith_short_8","alias_value":"P5CPN5XH","created_at":"2026-05-18T12:33:37.589309+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":32,"internal_anchor_count":32,"sample":[{"citing_arxiv_id":"2605.23049","citing_title":"SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \\sim 0$-7: Mass Dependence and Redshift Evolution","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2411.14532","citing_title":"Hitting the slopes: A spectroscopic view of UV continuum slopes of galaxies reveals a reddening at z > 9.5","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21599","citing_title":"JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S","ref_index":118,"is_internal_anchor":true},{"citing_arxiv_id":"2601.15959","citing_title":"JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8","ref_index":47,"is_internal_anchor":true},{"citing_arxiv_id":"2602.12548","citing_title":"The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\\sim4$","ref_index":28,"is_internal_anchor":true},{"citing_arxiv_id":"2605.20887","citing_title":"Difference Between Half-mass Radius and Half-light Radius of Galaxies at 0.2 $< z <$ 2.5 Revealed by JWST/NIRCam Data","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15263","citing_title":"On the quenching of LRD X-ray emission by both Compton-thick gas and high accretion rates","ref_index":126,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15361","citing_title":"Clumps in spiral galaxies at $z \\lesssim 3$: Disentangling two spatial modes of star formation","ref_index":40,"is_internal_anchor":true},{"citing_arxiv_id":"2508.14972","citing_title":"The Fraction of Clumpy Galaxies in JADES over $2<z<9$","ref_index":47,"is_internal_anchor":true},{"citing_arxiv_id":"2511.00975","citing_title":"The Atacama Cosmology Telescope: stellar mass growth in massive galaxy clusters from DR5 over the past 7 billion years","ref_index":56,"is_internal_anchor":true},{"citing_arxiv_id":"2511.08685","citing_title":"Kinematic scaling relations of disc galaxies from ionised gas at $z\\sim1$ and their connection with dark matter haloes","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2511.19600","citing_title":"Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback","ref_index":26,"is_internal_anchor":true},{"citing_arxiv_id":"2512.01684","citing_title":"Transition from Outside-in to Inside-Out at $z\\sim 2$: Evidence from Radial Profiles of Specific Star Formation Rate based on JWST/HST","ref_index":32,"is_internal_anchor":true},{"citing_arxiv_id":"2512.07955","citing_title":"Tracing nitrogen enrichment across cosmic time with JWST","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"2601.08931","citing_title":"Expanding the High-z Supernova Frontier: \"Wide-Area\" JWST Discoveries from the First Two Years of COSMOS-Web","ref_index":30,"is_internal_anchor":true},{"citing_arxiv_id":"2602.02702","citing_title":"Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation","ref_index":32,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15096","citing_title":"Impact of stellar population models on the estimated physical properties of galaxies","ref_index":26,"is_internal_anchor":true},{"citing_arxiv_id":"2605.03442","citing_title":"High-Redshift Gravitational Lens Discoveries in JWST NIRCam Using AnomalyMatch","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2604.22917","citing_title":"Diffusion-based Galaxy Simulations for the Roman High Latitude Survey","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2604.18731","citing_title":"Stellar feedback SPICEs up [C II] emission in the first galaxies","ref_index":271,"is_internal_anchor":true},{"citing_arxiv_id":"2604.18503","citing_title":"NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2604.11899","citing_title":"Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0","ref_index":21,"is_internal_anchor":true},{"citing_arxiv_id":"2604.05024","citing_title":"Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\\mathbf{z\\sim7}$","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2604.07138","citing_title":"The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2604.09399","citing_title":"Paschen Jumps in Little Red Dots: Evidence for Nebular Continua","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":1,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4","json":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4.json","graph_json":"https://pith.science/api/pith-number/P5CPN5XHXRZKR4ES46V3IA6TL4/graph.json","events_json":"https://pith.science/api/pith-number/P5CPN5XHXRZKR4ES46V3IA6TL4/events.json","paper":"https://pith.science/paper/P5CPN5XH"},"agent_actions":{"view_html":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4","download_json":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4.json","view_paper":"https://pith.science/paper/P5CPN5XH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.02465&json=true","fetch_graph":"https://pith.science/api/pith-number/P5CPN5XHXRZKR4ES46V3IA6TL4/graph.json","fetch_events":"https://pith.science/api/pith-number/P5CPN5XHXRZKR4ES46V3IA6TL4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4/action/storage_attestation","attest_author":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4/action/author_attestation","sign_citation":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4/action/citation_signature","submit_replication":"https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4/action/replication_record"}},"created_at":"2026-05-17T23:38:47.597899+00:00","updated_at":"2026-05-17T23:38:47.597899+00:00"}