Pith Number
pith:K5MV7KLG
pith:2005:K5MV7KLGDV4EKDKZPXJZEJYZXC
not attested
not anchored
not stored
refs pending
Probing the formation of intermediate- to high-mass stars in protoclusters: A detailed millimeter study of the NGC 2264 clumps
arxiv:astro-ph/0508619 v1 · 2005-08-29 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{K5MV7KLGDV4EKDKZPXJZEJYZXC}
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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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 | 2026-07-04T16:52:50.502895Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
57595fa9661d78450d597dd3922719b89a880a99f2ce55e6ef1d2ed6964652dd
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/K5MV7KLGDV4EKDKZPXJZEJYZXC \
| 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: 57595fa9661d78450d597dd3922719b89a880a99f2ce55e6ef1d2ed6964652dd
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e3317f156e9c3c60c4d49412a2c694043382d5256ca8819d01e7cda176fb7b2e",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2005-08-29T15:34:44Z",
"title_canon_sha256": "d75b3bca50a5f79014a2d6794f4e23c2186a0b58215ee07826d9824eb6043461"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0508619",
"kind": "arxiv",
"version": 1
}
}