Pith Number
pith:GWI7NHF6
pith:2009:GWI7NHF6X3A4APO7BZOPKVG3D3
not attested
not anchored
not stored
refs pending
The Formation Rates of Population III Stars and Chemical Enrichment of Halos during the Reionization Era
arxiv:0901.0711 v1 · 2009-01-06 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GWI7NHF6X3A4APO7BZOPKVG3D3}
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
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claim
4
Citations
5
Replications
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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
Receipt and verification
| First computed | 2026-05-18T04:29:24.144034Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3591f69cbebec1c03ddf0e5cf554db1ef88b3eabe688990c25a1ab8928d8ad7a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GWI7NHF6X3A4APO7BZOPKVG3D3 \
| 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: 3591f69cbebec1c03ddf0e5cf554db1ef88b3eabe688990c25a1ab8928d8ad7a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a6cb1a66874f14d9f92f44f397c37f2c16dc19030594dda836453f6d378acd15",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2009-01-06T21:15:39Z",
"title_canon_sha256": "47d681b0104720cdbac66de79a51df7e1267fadeecbb055e8d080a21027f23db"
},
"schema_version": "1.0",
"source": {
"id": "0901.0711",
"kind": "arxiv",
"version": 1
}
}