Pith Number
pith:GPIHS2Z4
pith:2013:GPIHS2Z4CVC7R4KD7MWSZJWJ5P
not attested
not anchored
not stored
refs pending
How Significant is Radiation Pressure in the Dynamics of the Gas Around Young Stellar Clusters?
arxiv:1301.2619 v1 · 2013-01-11 · astro-ph.GA · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GPIHS2Z4CVC7R4KD7MWSZJWJ5P}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
Author claim
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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.
Receipt and verification
| First computed | 2026-05-18T01:52:13.133850Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
33d0796b3c1545f8f143fb2d2ca6c9ebd0d4b73c338c51fce03d89a90719fb0b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GPIHS2Z4CVC7R4KD7MWSZJWJ5P \
| 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: 33d0796b3c1545f8f143fb2d2ca6c9ebd0d4b73c338c51fce03d89a90719fb0b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "577e97c63577c94f169786d6e5286341e6fd83b056756da532c7dfaa846f6215",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-01-11T22:05:17Z",
"title_canon_sha256": "ac65a50e0985050cff9460a5b7bd7d6d92aa42080df42f77ad798f25ac028045"
},
"schema_version": "1.0",
"source": {
"id": "1301.2619",
"kind": "arxiv",
"version": 1
}
}