Pith Number
pith:NPA4XQTB
pith:2019:NPA4XQTB5CDKLFFUKIP4U4J73T
not attested
not anchored
not stored
refs pending
Measuring the delay time distribution of binary neutron stars. III. Using the individual star formation histories of gravitational wave event host galaxies in the local universe
arxiv:1905.04310 v2 · 2019-05-10 · astro-ph.HE · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{NPA4XQTB5CDKLFFUKIP4U4J73T}
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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 | 2026-05-17T23:43:34.297429Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6bc1cbc261e886a594b4521fca713fdcc009c937fe1d5d0213b97f879f0e363b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/NPA4XQTB5CDKLFFUKIP4U4J73T \
| 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: 6bc1cbc261e886a594b4521fca713fdcc009c937fe1d5d0213b97f879f0e363b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "297c6810a501c49fa991a9af3f6bf76b60f903f0074530bb4292717b94f14854",
"cross_cats_sorted": [
"astro-ph.GA"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2019-05-10T18:00:01Z",
"title_canon_sha256": "632b2978864eba3c85c7e25266a940e0641d9a7ae488e1f0fcbf53783346d844"
},
"schema_version": "1.0",
"source": {
"id": "1905.04310",
"kind": "arxiv",
"version": 2
}
}