Pith Number
pith:SWKSRKRA
pith:2017:SWKSRKRACO67SDZ3RYYVEGXKYT
not attested
not anchored
not stored
refs pending
Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
arxiv:1706.08296 v1 · 2017-06-26 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{SWKSRKRACO67SDZ3RYYVEGXKYT}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more
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 | 2026-05-18T00:35:19.741727Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
959528aa2013bdf90f3b8e31521aeac4df5c5de5405c07e6b7e2d7d4d6a614e0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/SWKSRKRACO67SDZ3RYYVEGXKYT \
| 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: 959528aa2013bdf90f3b8e31521aeac4df5c5de5405c07e6b7e2d7d4d6a614e0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "9d83f7cf8d53c002333890405f56835a00dfa782cf9170dfcbda673377e9f016",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-06-26T09:15:23Z",
"title_canon_sha256": "b8b8dabd586fa46b3b39d11a20eeee43bfcf7e94327c637dd40edf1782752784"
},
"schema_version": "1.0",
"source": {
"id": "1706.08296",
"kind": "arxiv",
"version": 1
}
}