Pith Number
pith:BEXCYSSX
pith:2020:BEXCYSSXF6RUZBG6J6I3HH6R4T
not attested
not anchored
not stored
refs pending
The Ultimately Large Telescope -- what kind of facility do we need to detect Population III stars?
arxiv:2007.02946 v2 · 2020-07-06 · astro-ph.GA · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{BEXCYSSXF6RUZBG6J6I3HH6R4T}
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 | 2026-07-05T01:57:52.378832Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
092e2c4a572fa34c84de4f91b39fd1e4f1f098ea4c6a559226e9bcfe9eb9f238
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/BEXCYSSXF6RUZBG6J6I3HH6R4T \
| 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: 092e2c4a572fa34c84de4f91b39fd1e4f1f098ea4c6a559226e9bcfe9eb9f238
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a0a7e303b1999cc5495fd0bcc9b169e863cb8b98cfb28b7dfe91aee9bff3775b",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2020-07-06T18:00:01Z",
"title_canon_sha256": "e2c011115cc9e7a09bbf26cff39d454d8276f688a0ed757e7150753ec3ee7fb1"
},
"schema_version": "1.0",
"source": {
"id": "2007.02946",
"kind": "arxiv",
"version": 2
}
}