Pith Number
pith:WTOZ5PGN
pith:2020:WTOZ5PGN2FM7QQEHO3FJDAM7TC
not attested
not anchored
not stored
refs pending
Mass Ratios of Merging Double Neutron Stars as Implied by the Milky Way Population
arxiv:2007.06560 v1 · 2020-07-13 · astro-ph.HE · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{WTOZ5PGN2FM7QQEHO3FJDAM7TC}
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 | 2026-07-05T01:18:14.021935Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b4dd9ebccdd159f8408776ca91819f98be39f9c94a1dcd2bb278de7a6389e432
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/WTOZ5PGN2FM7QQEHO3FJDAM7TC \
| 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: b4dd9ebccdd159f8408776ca91819f98be39f9c94a1dcd2bb278de7a6389e432
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7b7393a2501fdfa894ca32c86b2f570356bcf73f62dbe15f52683fe9b54745f5",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2020-07-13T17:59:50Z",
"title_canon_sha256": "979a78b4597d726e36e970f42de41a683840a8ce466f54944f074c98c2323f8c"
},
"schema_version": "1.0",
"source": {
"id": "2007.06560",
"kind": "arxiv",
"version": 1
}
}