Pith Number
pith:XDY5TY74
pith:2006:XDY5TY74N2STYDEHYTL5SA3CMT
not attested
not anchored
not stored
refs pending
Disparate MgII Absorption Statistics towards Quasars and Gamma-Ray Bursts : A Possible Explanation
arxiv:astro-ph/0605676 v3 · 2006-05-26 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XDY5TY74N2STYDEHYTL5SA3CMT}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
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Bitcoin timestamp
2
Internet Archive
3
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4
Citations
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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 | 2026-07-04T16:58:48.104102Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b8f1d9e3fc6ea53c0c87c4d7d9036264f51f009f4615a72fc7507c5d4cc760df
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XDY5TY74N2STYDEHYTL5SA3CMT \
| 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: b8f1d9e3fc6ea53c0c87c4d7d9036264f51f009f4615a72fc7507c5d4cc760df
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "c0562db6ee3187ad7803271bfc11100dd4d17f471b937f34ee910a722b9ae965",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2006-05-26T22:02:02Z",
"title_canon_sha256": "8ce163259a6ea3334e12afaa49f056cbf3b5b5d6a26354a5ae8303e80a2e3227"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0605676",
"kind": "arxiv",
"version": 3
}
}