Pith Number
pith:2C26VF5T
pith:2018:2C26VF5TMZCUPHKBWEXFQ6CGS4
not attested
not anchored
not stored
refs pending
A connection between accretion states and the formation of ultra-relativistic outflows in a neutron star X-ray binary
arxiv:1812.04867 v1 · 2018-12-12 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{2C26VF5TMZCUPHKBWEXFQ6CGS4}
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 | 2026-05-17T23:58:01.279972Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d0b5ea97b36645479d41b12e5878469718ffcb706ea000f206d1d187acf39747
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/2C26VF5TMZCUPHKBWEXFQ6CGS4 \
| 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: d0b5ea97b36645479d41b12e5878469718ffcb706ea000f206d1d187acf39747
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d8af7932301c40c2caa0a15deba342b9d681682b3a516cd1b65a7e47c1841f3f",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-12-12T09:44:30Z",
"title_canon_sha256": "0caa412821fd00dc51ac35ad44fbf66445e2a8385539c8ca6068c19afbbabd45"
},
"schema_version": "1.0",
"source": {
"id": "1812.04867",
"kind": "arxiv",
"version": 1
}
}