Pith Number

pith:VTOLW33B

pith:2024:VTOLW33B4U7TOZDJGSPCOBTPSK

not attested not anchored not stored refs pending

JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields

Aayush Saxena, Alex J. Cameron, A. Lola Danhaive, Andrew J. Bunker, Benjamin D. Johnson, Brant E. Robertson, Bruno Rodr\'iguez Del Pino, Charlotte Simmonds, Chris J. Willott, Christina C. Williams, Christopher N. A. Willmer, Daniel J. Eisenstein, D\'avid Pusk\'as, Eiichi Egami, Eleonora Parlanti, Emma Curtis-Lake, Fengwu Sun, Francesco D'Eugenio, Gareth C. Jones, Giacomo Venturi, Hannah \"Ubler, Ignas Joud\v{z}balis, Irene Shivaei, Jacopo Chevallard, Jakob M. Helton, Jan Scholtz, Joris Witstok, Kevin N. Hainline, Kristan Boyett, Maddie S. Silcock, Marcia J. Rieke, Michael V. Maseda, Michele Perna, Mirko Curti, Natalia C. Villanueva, Nimisha Kumari, Nina Bonaventura, Pablo G. P\'erez-Gonz\'alez, Peter Jakobsen, Phillip A. Cargile, Rachana Bhatawdekar, Renske Smit, Roberto Maiolino, Ryan Hausen, Sandro Tacchella, Santiago Arribas, Stefano Carniani, St\'ephane Charlot, Tim Rawle, Tobias J. Looser, William M. Baker, Xihan Ji, Yongda Zhu, Zhiyuan Ji

arxiv:2404.06531 v1 · 2024-04-09 · astro-ph.GA

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{VTOLW33B4U7TOZDJGSPCOBTPSK}

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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.

Cited by

5 papers in Pith

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon

Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies

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

SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$

Receipt and verification

First computed	2026-07-05T08:06:13.874161Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

acdcbb6f61e53f376469349e27066f92a7eadf577788e89b706edf2dd38b3af9

Aliases

arxiv: 2404.06531 · arxiv_version: 2404.06531v1 · doi: 10.48550/arxiv.2404.06531 · pith_short_12: VTOLW33B4U7T · pith_short_16: VTOLW33B4U7TOZDJ · pith_short_8: VTOLW33B

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/VTOLW33B4U7TOZDJGSPCOBTPSK \
  | 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: acdcbb6f61e53f376469349e27066f92a7eadf577788e89b706edf2dd38b3af9

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "3946fab3092dfe8aa8425fac936655e9c3b50d485d5aaa4ea59d6adac0d0965d",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2024-04-09T18:00:00Z",
    "title_canon_sha256": "ace0ec2f6209df2819a131d6e6a9c7a73a25a3a9f6652aa11b2d5538d551332f"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2404.06531",
    "kind": "arxiv",
    "version": 1
  }
}