Pith Number
pith:VWHSPRXA
pith:2018:VWHSPRXA4NHL3Y4F2TCN5AXI52
not attested
not anchored
not stored
refs pending
The origins of the gamma-ray flux variations of NGC 1275 based on 8 years of Fermi-LAT observations
arxiv:1805.02361 v2 · 2018-05-07 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{VWHSPRXA4NHL3Y4F2TCN5AXI52}
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 | 2026-05-18T00:12:17.029428Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
ad8f27c6e0e34ebde385d4c4de82e8eeaeb2611090ebecb6c6f3e633795b929f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VWHSPRXA4NHL3Y4F2TCN5AXI52 \
| 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: ad8f27c6e0e34ebde385d4c4de82e8eeaeb2611090ebecb6c6f3e633795b929f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "58d992e25785e33fb6272e06e4a24993e822ab33052a284d9618eceadea680d0",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-05-07T06:25:36Z",
"title_canon_sha256": "cc7bedac87aff48df6661f3e6e52ecfdc20c2f6b37faa3ec1b2869491d2ed6ba"
},
"schema_version": "1.0",
"source": {
"id": "1805.02361",
"kind": "arxiv",
"version": 2
}
}