Pith Number
pith:XH4CKNCI
pith:2004:XH4CKNCIYBEN7HDQL2O3RRB3IY
not attested
not anchored
not stored
refs pending
The Spectroscopically Determined Substellar Mass Function of the Orion Nebula Cluster
arxiv:astro-ph/0404292 v2 · 2004-04-15 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XH4CKNCIYBEN7HDQL2O3RRB3IY}
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 | 2026-07-04T16:43:34.858221Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b9f8253448c048df9c705e9db8c43b4639782b60bb7624ebb44475a267a9a252
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XH4CKNCIYBEN7HDQL2O3RRB3IY \
| 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: b9f8253448c048df9c705e9db8c43b4639782b60bb7624ebb44475a267a9a252
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "829a29a486c827ec2d7194dfc809a65daa6f5a4db9674a770f3ddf48dd0e2b81",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2004-04-15T00:41:16Z",
"title_canon_sha256": "ad86ab9cec0f33cf69af14b09e3ce5255a71560be604616a2167d40dedb93f9e"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0404292",
"kind": "arxiv",
"version": 2
}
}