Pith Number
pith:GGDU4HQY
pith:2014:GGDU4HQYC5Y2FM6TIRJP5T5SHQ
not attested
not anchored
not stored
refs pending
A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
arxiv:1407.1850 v2 · 2014-07-07 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GGDU4HQYC5Y2FM6TIRJP5T5SHQ}
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 | 2026-05-18T01:42:41.176663Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
31874e1e181771a2b3d34452fecfb23c18454b93ae3693c47333b609bbd36874
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GGDU4HQYC5Y2FM6TIRJP5T5SHQ \
| 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: 31874e1e181771a2b3d34452fecfb23c18454b93ae3693c47333b609bbd36874
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "5f96e7cab19a66a5a9be09bb0bd65afbd9793781a0a7505da02775081b5193f4",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-07-07T20:00:42Z",
"title_canon_sha256": "91e466640e314525ffa0d61e280f971326c4f40c426635cd32956490a4d8c9d8"
},
"schema_version": "1.0",
"source": {
"id": "1407.1850",
"kind": "arxiv",
"version": 2
}
}