Pith Number

pith:YZFDDUTA

pith:2023:YZFDDUTAGCNUI4C5TN4M7RMVDL

not attested not anchored not stored refs pending

The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5

Adriano Fontana, Alexa M. Morales, Alexander de la Vega, Anthony J. Taylor, Anton M. Koekemoer, Avishai Dekel, Bahram Mobasher, Benne W. Holwerda, Bren E. Backhaus, Caitlin M. Casey, Caroline V. Morley, Casey Papovich, Dale D. Kocevski, David Elbaz, Gene C. K. Leung, Giulia Rodighiero, Henry C. Ferguson, Hollis B. Akins, Intae Jung, Jeyhan S. Kartaltepe, Jonathan R. Trump, Kartheik G. Iyer, Katherine Chworowsky, Kelcey Davis, Laura Bisigello, L. Y. Aaron Yung, Marc Huertas-Company, Mark Dickinson, Mauro Giavalisco, Maximilien Franco, Melanie Rowland, Micaela B. Bagley, Michaela Hirschmann, Michael C. Cooper, Nikko J. Cleri, Norbert Pirzkal, Norman A. Grogin, Oscar A. Chavez Ortiz, Pablo Arrabal Haro, Pablo G. Perez-Gonzalez, Peter Behroozi, Rachel S. Somerville, Ray A. Lucas, Rebecca L. Larson, Ricardo Amorin, Romeel Dave, Sagnick Mukherjee, Sandro Tacchella, Seiji Fujimoto, Shardha Jogee, Stephen Wilkins, Steven L. Finkelstein, Swara Ravindranath, Volker Bromm, Yingjie Cheng

arxiv:2311.04279 v1 · 2023-11-07 · astro-ph.GA

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{YZFDDUTAGCNUI4C5TN4M7RMVDL}

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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

11 papers in Pith

Deep Spectroscopic Follow-Up of Maisie's Galaxy -- A Typical Galaxy in the Early Universe

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization

Raising the reionization optical depth with inflationary CMB features

A self-consistent analytical model for both the photoionization rate and reionization history

Extending Hubble into the 2030s to Resolve the Physics of LyC Escape

Receipt and verification

First computed	2026-07-05T07:10:32.731553Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

c64a31d260309b44705d9b78cfc5951ac10795c2448876b2f4633d404436b7ef

Aliases

arxiv: 2311.04279 · arxiv_version: 2311.04279v1 · doi: 10.48550/arxiv.2311.04279 · pith_short_12: YZFDDUTAGCNU · pith_short_16: YZFDDUTAGCNUI4C5 · pith_short_8: YZFDDUTA

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/YZFDDUTAGCNUI4C5TN4M7RMVDL \
  | 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: c64a31d260309b44705d9b78cfc5951ac10795c2448876b2f4633d404436b7ef

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "8923edcc4ac2d40b6cc9daedab4de403beb710b1e0208a0b89d3c5cca476b512",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2023-11-07T19:00:03Z",
    "title_canon_sha256": "360f24ed3aa81a873c69283692a626d6411d1613624d3ddb961e32656bcfc896"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2311.04279",
    "kind": "arxiv",
    "version": 1
  }
}