Pith Number
pith:U3TCNUBG
pith:2014:U3TCNUBGSINTNYBACKQITSC6HQ
not attested
not anchored
not stored
refs pending
Trigonometric Parallaxes of High Mass Star Forming Regions: the Structure and Kinematics of the Milky Way
arxiv:1401.5377 v3 · 2014-01-21 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{U3TCNUBGSINTNYBACKQITSC6HQ}
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
· sign in to
claim
4
Citations
5
Replications
✓
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 | 2026-05-18T02:57:07.496229Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a6e626d026921b36e02012a089c85e3c06d46684caef13282692377f8880de3e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/U3TCNUBGSINTNYBACKQITSC6HQ \
| 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: a6e626d026921b36e02012a089c85e3c06d46684caef13282692377f8880de3e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8f692ac93df117f01138f51cbcae6b32263db42f410b00c241b8384606d3dee5",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-01-21T16:37:01Z",
"title_canon_sha256": "03f8f6f60dcb7d34e1dcbdcc33237b38c0a10196484565a840b1dd579d1389fa"
},
"schema_version": "1.0",
"source": {
"id": "1401.5377",
"kind": "arxiv",
"version": 3
}
}