Pith Number
pith:GPQB5U5L
pith:2013:GPQB5U5LLNLLTWS2DBASUGN5HS
not attested
not anchored
not stored
refs pending
Evidence for accretion rate change during type I X-ray bursts
arxiv:1303.4824 v2 · 2013-03-20 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GPQB5U5LLNLLTWS2DBASUGN5HS}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:51:00.455937Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
33e01ed3ab5b56b9da5a18412a19bd3cb71b251e851c6410025bfda6a4b0fe85
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GPQB5U5LLNLLTWS2DBASUGN5HS \
| 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: 33e01ed3ab5b56b9da5a18412a19bd3cb71b251e851c6410025bfda6a4b0fe85
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "30e2d21c436c4cb07d3f5a316aba0f17449150b9fcccaac912bba6977ed6ee1b",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2013-03-20T03:13:24Z",
"title_canon_sha256": "479f844df08fd10eb1082be84637cb7ae570ec5f65e3fdaa442ec222c870d36d"
},
"schema_version": "1.0",
"source": {
"id": "1303.4824",
"kind": "arxiv",
"version": 2
}
}