Pith Number
pith:QVN35JYD
pith:2022:QVN35JYDEVXCSIZZKHMGHWWIB5
not attested
not anchored
not stored
refs pending
Incorporating baryon-driven contraction of dark matter halos in rotation curve fits
arxiv:2208.04326 v1 · 2022-08-08 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{QVN35JYDEVXCSIZZKHMGHWWIB5}
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.
Cited by
Receipt and verification
| First computed | 2026-07-05T04:59:29.822570Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
855bbea703256e29233951d863dac80f4e3d57bf6beac930ef551858e921cb73
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/QVN35JYDEVXCSIZZKHMGHWWIB5 \
| 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: 855bbea703256e29233951d863dac80f4e3d57bf6beac930ef551858e921cb73
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "216bc38bcdc935f24ed2c915efc63b4bf734d18dfdb8887c3859f21ef6b02e5c",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2022-08-08T18:00:00Z",
"title_canon_sha256": "688dc0c0ba980bc7e1d76e148b966855cb884c0b7a45fb254dc2fc752d83edfb"
},
"schema_version": "1.0",
"source": {
"id": "2208.04326",
"kind": "arxiv",
"version": 1
}
}