Pith Number
pith:W77ISQ2M
pith:2025:W77ISQ2MV5FYI6BGWBXOX2QT4U
not attested
not anchored
not stored
refs pending
Consequences of radially correlated rotation curves for galaxy mass models
arxiv:2511.23106 v2 · 2025-11-28 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{W77ISQ2MV5FYI6BGWBXOX2QT4U}
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 | 2026-05-25T02:02:10.782457Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b7fe89434caf4b847826b06eebea13e50675d4ad5b49ef29ff7e7f7824eb7cd3
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/W77ISQ2MV5FYI6BGWBXOX2QT4U \
| 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: b7fe89434caf4b847826b06eebea13e50675d4ad5b49ef29ff7e7f7824eb7cd3
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "b3186ce56d8798c26ce098473b281d3dd3ae7e6f092115d5cfd552188ff26e2d",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2025-11-28T11:49:33Z",
"title_canon_sha256": "2a5792ef3145738df1dd2cb98c31220c0728e3a257850906d57a1d2c54f87afe"
},
"schema_version": "1.0",
"source": {
"id": "2511.23106",
"kind": "arxiv",
"version": 2
}
}