Pith Number
pith:HW6LWHJ6
pith:1997:HW6LWHJ63GO3LJZP43IVIBDJLF
not attested
not anchored
not stored
refs pending
Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991
arxiv:astro-ph/9705237 v2 · 1997-05-29 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HW6LWHJ63GO3LJZP43IVIBDJLF}
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.
Cited by
Receipt and verification
| First computed | 2026-07-04T16:03:02.046219Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3dbcbb1d3ed99db5a72fe6d1540469596cc1ea0269af75bbef95c3430c73f8a4
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HW6LWHJ63GO3LJZP43IVIBDJLF \
| 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: 3dbcbb1d3ed99db5a72fe6d1540469596cc1ea0269af75bbef95c3430c73f8a4
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7e7ae4bd7e566b86f7324295be09ccba4e8ecde683ef0634e175ed293a26100f",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1997-05-29T16:22:44Z",
"title_canon_sha256": "0411fc2f6b747387a9f3075d31a85ee89d4ba9ee7474b4901b24bd73abf8fc55"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9705237",
"kind": "arxiv",
"version": 2
}
}