Pith Number
pith:OBXVPYCB
pith:2008:OBXVPYCBINFWOF7ROMBGHKBMNL
not attested
not anchored
not stored
refs pending
Do the photometric colors of Type II-P Supernovae allow accurate determination of host galaxy extinction?
arxiv:0809.2591 v1 · 2008-09-15 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OBXVPYCBINFWOF7ROMBGHKBMNL}
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 | 2026-07-04T17:12:44.332505Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
706f57e041434b6717f1730263a82c6af3d4969b13140f68ba2cb4d56dd5d757
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OBXVPYCBINFWOF7ROMBGHKBMNL \
| 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: 706f57e041434b6717f1730263a82c6af3d4969b13140f68ba2cb4d56dd5d757
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "40152cb41c30684f2f4a12c437e6921ce184468152af30c65ed6ac01aa42dc8a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph",
"submitted_at": "2008-09-15T19:21:46Z",
"title_canon_sha256": "744c9d616a07e78e224b9a58646e0f3f47deee64888910aa84bb4f83896e1c06"
},
"schema_version": "1.0",
"source": {
"id": "0809.2591",
"kind": "arxiv",
"version": 1
}
}