Pith Number
pith:HAGSC2JH
pith:2013:HAGSC2JHOUZXHOXQG34XYB3A3R
not attested
not anchored
not stored
refs pending
The relation between accretion rates and the initial mass function in hydrodynamical simulations of star formation
arxiv:1312.3330 v1 · 2013-12-11 · astro-ph.GA · astro-ph.SR
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{HAGSC2JHOUZXHOXQG34XYB3A3R}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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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 | 2026-05-18T02:57:07.867685Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
380d216927753373baf036f97c0760dc40f3e8b4a197f1b259626fd228f275c8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/HAGSC2JHOUZXHOXQG34XYB3A3R \
| 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: 380d216927753373baf036f97c0760dc40f3e8b4a197f1b259626fd228f275c8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "3a4db40ae90af17a9166d88470b8cd8e2d6eae8cc1c9ac4a568f492f2788a215",
"cross_cats_sorted": [
"astro-ph.SR"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2013-12-11T21:00:15Z",
"title_canon_sha256": "8e9c7b68c7a0ead24b53a7ea219d888f27d8afed430ca09b621b1fc2c00ffc1d"
},
"schema_version": "1.0",
"source": {
"id": "1312.3330",
"kind": "arxiv",
"version": 1
}
}