Pith Number
pith:K6N5F35Q
pith:2017:K6N5F35QKAW2Q6FXUDQMVILIRH
not attested
not anchored
not stored
refs pending
Time Dependent Models of Magnetospheric Accretion onto Young Stars
arxiv:1703.05652 v1 · 2017-03-16 · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{K6N5F35QKAW2Q6FXUDQMVILIRH}
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 | 2026-05-18T00:47:00.592350Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
579bd2efb0502da878b7a0e0caa16889eebb665f1c755ae5b56584e4bf7ac503
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/K6N5F35QKAW2Q6FXUDQMVILIRH \
| 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: 579bd2efb0502da878b7a0e0caa16889eebb665f1c755ae5b56584e4bf7ac503
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2570b8dac1ccf19e4e36e5bfa38330961c2a79c507cb3e6350a796bd29f2edff",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.SR",
"submitted_at": "2017-03-16T14:56:18Z",
"title_canon_sha256": "59485263ba6739b69a21784fb3416717bbe0db08919f9faacb094ec8f889de5b"
},
"schema_version": "1.0",
"source": {
"id": "1703.05652",
"kind": "arxiv",
"version": 1
}
}