Pith Number
pith:MPCKTLTA
pith:2018:MPCKTLTA6VXBGJ3YPADSBEKJ4O
not attested
not anchored
not stored
refs pending
The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars
arxiv:1808.07616 v1 · 2018-08-23 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{MPCKTLTA6VXBGJ3YPADSBEKJ4O}
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 | 2026-05-18T00:06:36.867919Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
63c4a9ae60f56e1327787807209149e39c351ca69dbbbe035d4ce79ddb7bf59e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/MPCKTLTA6VXBGJ3YPADSBEKJ4O \
| 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: 63c4a9ae60f56e1327787807209149e39c351ca69dbbbe035d4ce79ddb7bf59e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a7916eecd6a720f28f5e15e603920f33b6c002d4940f0016650f49da9fc2b319",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2018-08-23T03:17:39Z",
"title_canon_sha256": "2ace47f64c3dde26c3d98723b1144a86acdff9d2cd4498b2af451fc239894165"
},
"schema_version": "1.0",
"source": {
"id": "1808.07616",
"kind": "arxiv",
"version": 1
}
}