Pith Number
pith:EDBHQP7F
pith:2015:EDBHQP7F3HYPSUPZAJLSWSLR23
not attested
not anchored
not stored
refs pending
What determines large scale galaxy clustering: halo mass or local density?
arxiv:1510.01692 v3 · 2015-10-06 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{EDBHQP7F3HYPSUPZAJLSWSLR23}
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
✓
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 | 2026-05-18T00:51:18.352673Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
20c2783fe5d9f0f951f902572b4971d6e8dfe21fa845a89b6e7cd4cbe1519a2b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EDBHQP7F3HYPSUPZAJLSWSLR23 \
| 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: 20c2783fe5d9f0f951f902572b4971d6e8dfe21fa845a89b6e7cd4cbe1519a2b
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "08087ce974f7a8ec3fbd0e194b973686ac199170710ade12a3ce13313c066f5a",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2015-10-06T18:35:33Z",
"title_canon_sha256": "a7bcff6f416047fa88913680db2b3a014aba1e3ab02c62d0f9123be32c2dbca1"
},
"schema_version": "1.0",
"source": {
"id": "1510.01692",
"kind": "arxiv",
"version": 3
}
}