Pith Number
pith:HNR3S4WW
pith:2021:HNR3S4WWJ7EJV77V2DQ64Z4SSK
not attested
not anchored
not stored
refs pending
The role of the halo magnetic field on accretion through High-Velocity Clouds
arxiv:2111.12733 v1 · 2021-11-24 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HNR3S4WWJ7EJV77V2DQ64Z4SSK}
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 | 2026-07-05T03:38:42.475468Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
3b63b972d64fc89afff5d0e1ee67929288f3c61871a4589f23101b70fb442df3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HNR3S4WWJ7EJV77V2DQ64Z4SSK \
| 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: 3b63b972d64fc89afff5d0e1ee67929288f3c61871a4589f23101b70fb442df3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "d8f5c994535a2b31226a847483419c430571ca23a4204cd060a07c2894869e14",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2021-11-24T19:00:09Z",
"title_canon_sha256": "12d169ed5b1a72e116c5343a6e9d483b3f01114aeb0142b7296acc76b30f17bb"
},
"schema_version": "1.0",
"source": {
"id": "2111.12733",
"kind": "arxiv",
"version": 1
}
}