Pith Number
pith:KASLYHR5
pith:2015:KASLYHR5TOF6KCEJPP5NVJISB3
not attested
not anchored
not stored
refs pending
Are the globular clusters with significant internal [Fe/H] spreads all former dwarf galaxy nuclei?
arxiv:1510.00873 v1 · 2015-10-03 · astro-ph.GA · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{KASLYHR5TOF6KCEJPP5NVJISB3}
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 | 2026-05-18T01:05:45.905083Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5024bc1e3d9b8be508897bfadaa5120ee1a4409010c90357424d9a3d366b061e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KASLYHR5TOF6KCEJPP5NVJISB3 \
| 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: 5024bc1e3d9b8be508897bfadaa5120ee1a4409010c90357424d9a3d366b061e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "fcd8c9180f071a2d65164fa4384e5af7b71135336caa41c5c48e6b182dca1149",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2015-10-03T21:43:07Z",
"title_canon_sha256": "a205e5c5e64ef002f5743bc3bf9bead3144d5cc0ac6beab09a9dfb8d369eb027"
},
"schema_version": "1.0",
"source": {
"id": "1510.00873",
"kind": "arxiv",
"version": 1
}
}