Pith Number
pith:EGZPVREY
pith:2014:EGZPVREYRWCJNVL3D5LCV6SLRS
not attested
not anchored
not stored
refs pending
Evidence for a constant IMF in early-type galaxies based on their X-ray binary populations
arxiv:1401.3405 v2 · 2014-01-15 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{EGZPVREYRWCJNVL3D5LCV6SLRS}
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 | 2026-05-18T01:45:25.434942Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
21b2fac4988d8496d57b1f562afa4b8cabcb9d2b5ed9ea6c3dcbe4428ccb60a7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EGZPVREYRWCJNVL3D5LCV6SLRS \
| 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: 21b2fac4988d8496d57b1f562afa4b8cabcb9d2b5ed9ea6c3dcbe4428ccb60a7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3edb420cc9f7be284a6c19c32ec38ebc24bb226f7a4d326a486ec743c2cb34d8",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-01-15T01:44:11Z",
"title_canon_sha256": "2d8e26f0c76d8198d9ff94b049db0c88664d7786d261b417009ebe82ac2bb426"
},
"schema_version": "1.0",
"source": {
"id": "1401.3405",
"kind": "arxiv",
"version": 2
}
}