Pith Number
pith:IDXDGXGS
pith:2022:IDXDGXGSIJNP3YQZQ5L4P66WMS
not attested
not anchored
not stored
refs pending
Can radial motions in the stellar halo constrain the rate of change of mass in the Galaxy?
arxiv:2207.11739 v1 · 2022-07-24 · astro-ph.GA · astro-ph.CO · hep-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IDXDGXGSIJNP3YQZQ5L4P66WMS}
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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 | 2026-07-05T05:55:10.351871Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
40ee335cd2425afde2198757c7fbd664a7d82a4d17ddb4f8674ad624759b73db
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IDXDGXGSIJNP3YQZQ5L4P66WMS \
| 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: 40ee335cd2425afde2198757c7fbd664a7d82a4d17ddb4f8674ad624759b73db
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dc73fdda049eb7556a36b5d1ac0cdb6f4fc0fe15e91d1742093fb8b686cd94b4",
"cross_cats_sorted": [
"astro-ph.CO",
"hep-ph"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2022-07-24T13:33:01Z",
"title_canon_sha256": "7a6435621b5e54f5ce4d6017751a07f1000a2e70d998a4ae687c073b8254444a"
},
"schema_version": "1.0",
"source": {
"id": "2207.11739",
"kind": "arxiv",
"version": 1
}
}