Pith Number
pith:P5GZJWQF
pith:2017:P5GZJWQFZX5R62RJ3IRP5WWU3L
not attested
not anchored
not stored
refs pending
The Optical Counterpart to the Accreting Millisecond X-ray Pulsar SAX J1748.9-2021 in the Globular Cluster NGC 6440
arxiv:1706.07061 v1 · 2017-06-21 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{P5GZJWQFZX5R62RJ3IRP5WWU3L}
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 | 2026-05-18T00:38:50.612702Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
7f4d94da05cdfb1f6a29da22fedad4daccc54ae9d22a5da04de20198bb58df86
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/P5GZJWQFZX5R62RJ3IRP5WWU3L \
| 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: 7f4d94da05cdfb1f6a29da22fedad4daccc54ae9d22a5da04de20198bb58df86
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f3f5bbf6463a313121f7ddae7690df70d9c9489f7c06a7835cda750b155677d5",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-06-21T18:00:11Z",
"title_canon_sha256": "0bd5d747fdf7c94767d41b4ab226bae3c23ce4e677c52bc57cde2f3ee3586ca4"
},
"schema_version": "1.0",
"source": {
"id": "1706.07061",
"kind": "arxiv",
"version": 1
}
}