Pith Number

pith:P5CPN5XH

pith:2023:P5CPN5XHXRZKR4ES46V3IA6TL4

not attested not anchored not stored refs resolved

Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

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

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.

arxiv:2306.02465 v2 · 2023-06-04 · astro-ph.GA

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{P5CPN5XHXRZKR4ES46V3IA6TL4}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest 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.

C2weakest 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.

C3one 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.

References

119 extracted · 119 resolved · 1 Pith anchors

[1] Akins, H. B., Casey, C. M., Allen, N., et al. 2023, ApJ, 956, 61 2023

[2] 2022, Universe, 8, 554 2022

[3] H., Jagannathan, P., & Nyland, K 2020

[4] 2024, ApJ, 976, 224 2024

[5] 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 2023

Formal links

1 machine-checked theorem link

Cited by

32 papers in Pith

SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \sim 0$-7: Mass Dependence and Redshift Evolution

Hitting the slopes: A spectroscopic view of UV continuum slopes of galaxies reveals a reddening at z > 9.5

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8

The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\sim4$

Receipt and verification

First computed	2026-05-17T23:38:47.597829Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

7f44f6f6e7bc72a8f092e7abb403d35f15ca3dd556b43525dffbdc196b395af2

Aliases

arxiv: 2306.02465 · arxiv_version: 2306.02465v2 · doi: 10.48550/arxiv.2306.02465 · pith_short_12: P5CPN5XHXRZK · pith_short_16: P5CPN5XHXRZKR4ES · pith_short_8: P5CPN5XH

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/P5CPN5XHXRZKR4ES46V3IA6TL4 \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 7f44f6f6e7bc72a8f092e7abb403d35f15ca3dd556b43525dffbdc196b395af2

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "636ab457802e09f3c7cf687eb7fa3ec52b55cb46690ad62c6fa59a298929a30a",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2023-06-04T20:44:21Z",
    "title_canon_sha256": "6da326f9568fe7c9f209cc119afb193c629b129323540075ea3ba3774f63e1fa"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2306.02465",
    "kind": "arxiv",
    "version": 2
  }
}