Pith Number
pith:RA3PZOZQ
pith:2019:RA3PZOZQ7XYUSY45Z3V5Q36X6C
not attested
not anchored
not stored
refs pending
From the Outside Looking in: What can Milky Way Analogues Tell us About the Star Formation Rate of Our Own Galaxy?
arxiv:1909.01654 v1 · 2019-09-04 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RA3PZOZQ7XYUSY45Z3V5Q36X6C}
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 | 2026-07-05T00:09:04.167591Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8836fcbb30fdf149639dceebd86fd7f0a71274a1071950d5f92c5bf22e6e129a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RA3PZOZQ7XYUSY45Z3V5Q36X6C \
| 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: 8836fcbb30fdf149639dceebd86fd7f0a71274a1071950d5f92c5bf22e6e129a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3d65ce7acc6ccc2ac066302453484a3c8dc0647dce3bf469fb834eb03a3279e5",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-09-04T09:40:55Z",
"title_canon_sha256": "57c49a2153274b7ed9fb485abc984614d02e9c0f196c216156f91f2f2c455860"
},
"schema_version": "1.0",
"source": {
"id": "1909.01654",
"kind": "arxiv",
"version": 1
}
}