Pith Number
pith:SIEQQ3R4
pith:2017:SIEQQ3R4P262H2EUIEWDWDPVB5
not attested
not anchored
not stored
refs pending
$R$-band host galaxy contamination of TeV $\gamma$-ray blazar Mrk 501: effects of the aperture size and seeing
arxiv:1712.00217 v1 · 2017-12-01 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{SIEQQ3R4P262H2EUIEWDWDPVB5}
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 | 2026-05-18T00:21:21.221824Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9209086e3c7ebda3e894412c3b0df50f663a37d6b4a0225ebc6663aa50401812
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/SIEQQ3R4P262H2EUIEWDWDPVB5 \
| 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: 9209086e3c7ebda3e894412c3b0df50f663a37d6b4a0225ebc6663aa50401812
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "61465954e589a535da8afe40eec445ea672b658b6356b5e8a4c29f49145ef3b5",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-12-01T07:35:42Z",
"title_canon_sha256": "1faec4f68e3d59f91f76328b1472c6a1b76f75f484384b3fc0458d6a84f5d84f"
},
"schema_version": "1.0",
"source": {
"id": "1712.00217",
"kind": "arxiv",
"version": 1
}
}