Pith Number
pith:M5E4RRUS
pith:2018:M5E4RRUSNYBNVYJ6TIXVZ6QUDN
not attested
not anchored
not stored
refs pending
Chandra X-ray Observations of the Neutron Star Merger GW170817: Thermal X-Ray Emission From a Kilonova Remnant?
arxiv:1812.11320 v1 · 2018-12-29 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{M5E4RRUSNYBNVYJ6TIXVZ6QUDN}
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 | 2026-05-17T23:57:12.244878Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6749c8c6926e02dae13e9a2f5cfa141b739a089eaba450a4d42d3db09d866b61
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/M5E4RRUSNYBNVYJ6TIXVZ6QUDN \
| 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: 6749c8c6926e02dae13e9a2f5cfa141b739a089eaba450a4d42d3db09d866b61
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "346a5e4c2d606179f1ce5b26a8d6b5b8ddf5f0efec95512328b93e6652032dc0",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-12-29T09:24:44Z",
"title_canon_sha256": "8ffde7dca98910256cc6c2a8cce660852d69a66cebf20a6e9f035f193955bcd0"
},
"schema_version": "1.0",
"source": {
"id": "1812.11320",
"kind": "arxiv",
"version": 1
}
}