Pith Number
pith:ZXUTBODP
pith:1999:ZXUTBODP3BLO2UTAWSW5ZGKQPL
not attested
not anchored
not stored
refs pending
Simulations of Damped Lyman-Alpha and Lyman Limit Absorbers in Different Cosmologies: Implications for Structure Formation at High Redshift
arxiv:astro-ph/9911343 v2 · 1999-11-18 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{ZXUTBODP3BLO2UTAWSW5ZGKQPL}
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 | 2026-05-18T01:07:15.239358Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
cde930b86fd856ed5260b4addc99507ad1f57317a02f44b36e3c8762153f961e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/ZXUTBODP3BLO2UTAWSW5ZGKQPL \
| 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: cde930b86fd856ed5260b4addc99507ad1f57317a02f44b36e3c8762153f961e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3a83058611a2e11972883b1f8ed814501ced61fb8439be4926843380f9874cd3",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1999-11-18T00:04:12Z",
"title_canon_sha256": "1479a73a4fefea1d7189460677d6e310e7f1e459c4f342dd58201acb2d3174e5"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9911343",
"kind": "arxiv",
"version": 2
}
}