Pith Number
pith:5TEEWW3Q
pith:2021:5TEEWW3Q7K674L4JQDQVREFYGT
not attested
not anchored
not stored
refs pending
The evolution of merger fraction of galaxies at z < 0.6 depending on the star formation mode in the AKARI NEP Wide field
arxiv:2108.07125 v1 · 2021-08-16 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5TEEWW3Q7K674L4JQDQVREFYGT}
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
· sign in to
claim
4
Citations
5
Replications
✓
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.
Receipt and verification
| First computed | 2026-07-05T03:19:20.510801Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ecc84b5b70fabdfe2f8980e15890b834d261a12a97f8de17c051d6f3d5ff3075
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5TEEWW3Q7K674L4JQDQVREFYGT \
| 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: ecc84b5b70fabdfe2f8980e15890b834d261a12a97f8de17c051d6f3d5ff3075
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8aa9ad6fd67f8d3f4990cd086a6e8eed456117c038e9b93fb63b3e007f087ba4",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2021-08-16T14:48:36Z",
"title_canon_sha256": "74bd702b527c9b1ca83ffbddab85f86a1f71102555e363f262bfbf5f1be0946f"
},
"schema_version": "1.0",
"source": {
"id": "2108.07125",
"kind": "arxiv",
"version": 1
}
}