Pith Number

pith:EZQEOIEE

pith:2022:EZQEOIEEOQJZQOJJUPNVN2IVVZ

not attested not anchored not stored refs pending

The All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) Mission Concept

Amanda Steinhebel, Amy Lien, Andreas Zoglauer, Bernard Phlips, Carolyn Kierans, Chanda Prescod-Weinstein, Chris Fryer, Christopher Karwin, Clio Sleator, Daniel Kocevski, Daniel Shy, Dieter Hartmann, Donggeun Tak, Elisabetta Bissaldi, Eric Burns, Eric Charles, Eric Howell, Eric Wulf, Haocheng Zhang, Henrike Fleischhack, Hiroyasu Tajima, Israel Martinez-Castellanos, Janeth Valverde, Jeremy Perkins, J. Eric Grove, Jessica Metcalfe, Judith Racusin, Julie McEnery, Ke Fang, Kohta Murase, Lea Marcotulli, Luca Baldini, Luca Latronico, Lucas Parker, Manoj Jadhav, Marco Ajello, Mario Nicola Mazziotta, Matthew Barring, Michela Negro, Naoko Kurahashi, Nicolas Cannady, Nicolas Striebig, Peter Shawhan, Regina Caputo, Richard Leys, Richard Woolf, Rui Curado da Silva, Soebur Razzaque, Tiffany Lewis, Tom Shutt, Tonia Venters, Yasushi Fukazawa, Yong Sheng, Yusuke Suda, Zorawar Wadiasingh

arxiv:2208.04990 v2 · 2022-08-09 · astro-ph.IM · astro-ph.HE

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

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{EZQEOIEEOQJZQOJJUPNVN2IVVZ}

Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge

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

Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation

Electromagnetic Signatures From Primordial Black Holes in the Solar System

A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667

Ultra high-energy cosmic rays from relativistic outflows in accretion induced collapse of white dwarfs

Receipt and verification

First computed	2026-07-05T05:13:19.454755Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

26604720847413983929a3db56e915ae582c50f29235fffc106c038b9feda550

Aliases

arxiv: 2208.04990 · arxiv_version: 2208.04990v2 · doi: 10.48550/arxiv.2208.04990 · pith_short_12: EZQEOIEEOQJZ · pith_short_16: EZQEOIEEOQJZQOJJ · pith_short_8: EZQEOIEE

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/EZQEOIEEOQJZQOJJUPNVN2IVVZ \
  | 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: 26604720847413983929a3db56e915ae582c50f29235fffc106c038b9feda550

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "6fd1dca99e7c99b4a5b0cb770f574f1859d18b8b4e92e2776ff7eb5333a37cf8",
    "cross_cats_sorted": [
      "astro-ph.HE"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.IM",
    "submitted_at": "2022-08-09T18:33:23Z",
    "title_canon_sha256": "5f05aaa73ef1a5060ce874a2c6b4e9498767cc848be5e035c487df9ff509d11c"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2208.04990",
    "kind": "arxiv",
    "version": 2
  }
}