Pith Number
pith:IKMFPYWP
pith:2014:IKMFPYWPLBKESZUSSDFXQ7VNFQ
not attested
not anchored
not stored
refs pending
Dust origin in late-type dwarf galaxies: ISM growth vs. type II supernovae
arxiv:1401.1675 v2 · 2014-01-08 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IKMFPYWPLBKESZUSSDFXQ7VNFQ}
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 | 2026-05-18T01:45:32.854350Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
429857e2cf585449669290cb787ead2c0d9eba5a5ae8769e42c65eeb56674597
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IKMFPYWPLBKESZUSSDFXQ7VNFQ \
| 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: 429857e2cf585449669290cb787ead2c0d9eba5a5ae8769e42c65eeb56674597
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cbc078134de076dcbfcc8f3971ee49f356f7712143681c6a361c513c95e4569c",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-01-08T12:05:14Z",
"title_canon_sha256": "004979a0a7d606c515981b0fcfd38ea1563624a43ff2ae605f087592d3607f8a"
},
"schema_version": "1.0",
"source": {
"id": "1401.1675",
"kind": "arxiv",
"version": 2
}
}