Pith Number
pith:W7FOBGX5
pith:1996:W7FOBGX57WORPW6LNQPW4QGWTT
not attested
not anchored
not stored
refs pending
Ultraviolet Imaging Observations of the cD Galaxy in Abell 1795: Further Evidence for Massive Star Formation in a Cooling Flow
arxiv:astro-ph/9611024 v1 · 1996-11-04 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{W7FOBGX57WORPW6LNQPW4QGWTT}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-07-04T16:00:18.084746Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b7cae09afdfd9d17dbcb6c1f6e40d69cf5bf1e58529f158ba9b8c16b1ddd40de
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/W7FOBGX57WORPW6LNQPW4QGWTT \
| 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: b7cae09afdfd9d17dbcb6c1f6e40d69cf5bf1e58529f158ba9b8c16b1ddd40de
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "36d743c4fe6b20e82656f3155d9eafb2b7550d15758003879f99908607e59067",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1996-11-04T21:15:09Z",
"title_canon_sha256": "4bb5676b93c9ab693e1c21c30a8ee9df85763ee765b98d49c9b249f22b4ad01b"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9611024",
"kind": "arxiv",
"version": 1
}
}