Pith Number
pith:F3W3LYK3
pith:2002:F3W3LYK3U4OX4SSWDZQ3KJG2R3
not attested
not anchored
not stored
refs pending
Two-dimensional kinematics and stellar populations of early-type galaxies: First results from the SAURON survey
arxiv:astro-ph/0204129 v1 · 2002-04-08 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{F3W3LYK3U4OX4SSWDZQ3KJG2R3}
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.
Receipt and verification
| First computed | 2026-07-04T14:11:58.895715Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2eedb5e15ba71d7e4a561e61b524da8efbfcd269051d3e20106a9cb39450d74a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/F3W3LYK3U4OX4SSWDZQ3KJG2R3 \
| 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: 2eedb5e15ba71d7e4a561e61b524da8efbfcd269051d3e20106a9cb39450d74a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "82aba725267144d963b3b0ca88d1f4450dcece5c31fd7fcbe4420454071290dc",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2002-04-08T15:44:59Z",
"title_canon_sha256": "08f8a4b3b4471cc3dcc21cd758fc4e1a3dbe2a0d7ac0775d16b95c4961f33935"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0204129",
"kind": "arxiv",
"version": 1
}
}