Pith Number
pith:XE5MFUL2
pith:2010:XE5MFUL2FO34ZLKDQD3JBHCPGT
not attested
not anchored
not stored
refs pending
A cosmic-ray dominated ISM in Ultra Luminous Infrared Galaxies: new initial conditions for star formation
arxiv:1009.1134 v1 · 2010-09-06 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XE5MFUL2FO34ZLKDQD3JBHCPGT}
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 | 2026-05-18T02:05:36.083451Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b93ac2d17a2bb7ccad4380f6909c4f34da580ee9843a7bed74a6238c2ac50acf
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XE5MFUL2FO34ZLKDQD3JBHCPGT \
| 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: b93ac2d17a2bb7ccad4380f6909c4f34da580ee9843a7bed74a6238c2ac50acf
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e075b117d0776d2749d59f5c7073a9305c63cee5b710a0e9340e1e068efdb26a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2010-09-06T19:39:03Z",
"title_canon_sha256": "71316116cf0f5aceb2138bbcfbdfeb444ce711cc6adaa19748260a497c878147"
},
"schema_version": "1.0",
"source": {
"id": "1009.1134",
"kind": "arxiv",
"version": 1
}
}