Pith Number
pith:63SOVP7K
pith:2014:63SOVP7KKNH3EOQ3SOYRGNOZE3
not attested
not anchored
not stored
refs pending
Predicting Lyman-alpha and Mg II Fluxes from K and M Dwarfs Using GALEX Ultraviolet Photometry
arxiv:1410.4263 v1 · 2014-10-16 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{63SOVP7KKNH3EOQ3SOYRGNOZE3}
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 | 2026-05-18T01:41:48.017428Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f6e4eabfea534fb23a1b93b11335d926c0b61a59c53b8dd2497f85d1e0e52cfd
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/63SOVP7KKNH3EOQ3SOYRGNOZE3 \
| 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: f6e4eabfea534fb23a1b93b11335d926c0b61a59c53b8dd2497f85d1e0e52cfd
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0dd5556ef5256ae180b214af87eb57b93d80b2598bff888d26b9e9eeadc9ff72",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2014-10-16T00:27:30Z",
"title_canon_sha256": "7b06885cb79be785b3676051c30ecd9da98b7aab1221558fed599cb5e2c6787b"
},
"schema_version": "1.0",
"source": {
"id": "1410.4263",
"kind": "arxiv",
"version": 1
}
}