Pith Number
pith:XPWHHUEY
pith:2011:XPWHHUEYST5C3A5EWCMXDV4DVZ
not attested
not anchored
not stored
refs pending
Multiple synchrotron self-Compton modeling of gamma-ray flares in 3C 279
arxiv:1109.2518 v1 · 2011-09-12 · astro-ph.HE · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XPWHHUEYST5C3A5EWCMXDV4DVZ}
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 | 2026-05-18T02:00:34.310028Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
bbec73d09894fa2d83a4b09971d783ae7514a9da8c91a2269f01bbf62a4e0bcd
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XPWHHUEYST5C3A5EWCMXDV4DVZ \
| 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: bbec73d09894fa2d83a4b09971d783ae7514a9da8c91a2269f01bbf62a4e0bcd
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "bc523624e687d4f2e3c23c69432084581eb97ec9c5d4c432a61ea3dd50343c26",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2011-09-12T16:07:23Z",
"title_canon_sha256": "dc9ca588bbb0c43d3f0292fe9d69bb38571da32910bbd6faff98e8af595f5bdd"
},
"schema_version": "1.0",
"source": {
"id": "1109.2518",
"kind": "arxiv",
"version": 1
}
}