Pith. sign in
Pith Number

pith:GYZFGINV

pith:2025:GYZFGINVBA2K4GZA3ZMPFQM4QM
not attested not anchored not stored refs pending

CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288

Adam Carnall, Ansh R. Gupta, Anthony J. Taylor, Anton M. Koekemoer, Caitlin M. Casey, Callum T. Donnan, Casey Papovich, Dale D. Kocevski, Denis Burgarella, Derek J. McLeod, Fergus Cullen, Gene C. K. Leung, Guillermo Barro, Ho-Hin Leung, Hollis B. Akins, Intae Jung, James S. Dunlop, Jeyhan S. Kartaltepe, John Chisholm, Jonathan R. Trump, Jorge A. Zavala, Katherine Chworowsky, Kelcey Davis, Kohei Inayoshi, Lorenzo Napolitano, L. Y. Aaron Yung, Madisyn Brooks, Mario Llerena, Mark Dickinson, Mauro Giavalisco, Michaela Hirschmann, Nimish P. Hathi, Norman A. Grogin, Pablo Arrabal Haro, Pablo G. Perez-Gonzalez, Rachel S. Somerville, Ray A. Lucas, Rebecca L. Larson, Ricardo O. Amorin, Richard S. Ellis, Roberta Tripodi, Ross McLure, Seiji Fujimoto, Stephanie Juneau, Stephen M. Wilkins, Steven L. Finkelstein, Thomas M. Stanton, Vasily Kokorev, Vital Fernandez, Volker Bromm, Xin Wang, Yingjie Cheng

arxiv:2505.04609 v4 · 2025-05-07 · 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{GYZFGINVBA2K4GZA3ZMPFQM4QM}

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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

7 papers in Pith

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5
SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds
Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth
Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts
Impact of Primordial Black Hole population on 21 cm observables at high redshift
Receipt and verification
First computed 2026-07-05T11:26:30.842540Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

36325321b50834ae1b20de58f2c19c8328f4f1dfa31ca2490b6fb21a49d1e52a

Aliases

arxiv: 2505.04609 · arxiv_version: 2505.04609v4 · doi: 10.48550/arxiv.2505.04609 · pith_short_12: GYZFGINVBA2K · pith_short_16: GYZFGINVBA2K4GZA · pith_short_8: GYZFGINV
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/GYZFGINVBA2K4GZA3ZMPFQM4QM \
  | 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: 36325321b50834ae1b20de58f2c19c8328f4f1dfa31ca2490b6fb21a49d1e52a
Canonical record JSON 
{
  "metadata": {
    "abstract_canon_sha256": "73cf359c18c1b84920a74c332b9892482941f78010795718c2dec3c11e92abc4",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.GA",
    "submitted_at": "2025-05-07T17:53:48Z",
    "title_canon_sha256": "689b1ba176664758bd68c4bddf4f7c1d666ed0f802db54e50fee6e5412303949"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2505.04609",
    "kind": "arxiv",
    "version": 4
  }
}