Pith Number
pith:UWMO6RSL
pith:2019:UWMO6RSLASRRHUFL2SXE3L5CY6
not attested
not anchored
not stored
refs pending
The Astrochemical Impact of Cosmic Rays in Protoclusters II: CI-to-H$_2$ and CO-to-H$_2$ Conversion Factors
arxiv:1908.06999 v1 · 2019-08-19 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{UWMO6RSLASRRHUFL2SXE3L5CY6}
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 | 2026-07-05T00:10:42.150502Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a598ef464b04a313d0abd4ae4dafa2c78c36fd958d7f6c791f1a3000f69b5f54
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UWMO6RSLASRRHUFL2SXE3L5CY6 \
| 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: a598ef464b04a313d0abd4ae4dafa2c78c36fd958d7f6c791f1a3000f69b5f54
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "fffedc858ee15bd65da6bbf9c23f15298a0c138a35118dc0439bc9697cbf9cf6",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-08-19T18:00:42Z",
"title_canon_sha256": "152e0e840ae82d6a11b0a4f30ce577bd0fc2c5778f10e149f91eb1b87eda232b"
},
"schema_version": "1.0",
"source": {
"id": "1908.06999",
"kind": "arxiv",
"version": 1
}
}