Pith Number
pith:VW3UU2IW
pith:2014:VW3UU2IWK3LLB47UJQOI2NVNGV
not attested
not anchored
not stored
refs pending
Dynamics of Dusty Radiation Pressure Driven Shells and Clouds: Fast Outflows from Galaxies, Star Clusters, Massive Stars, and AGN
arxiv:1406.5206 v2 · 2014-06-19 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{VW3UU2IWK3LLB47UJQOI2NVNGV}
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
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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 | 2026-05-18T01:42:52.775701Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
adb74a691656d6b0f3f44c1c8d36ad3540d5472abb985c80d40706a7b4474380
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VW3UU2IWK3LLB47UJQOI2NVNGV \
| 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: adb74a691656d6b0f3f44c1c8d36ad3540d5472abb985c80d40706a7b4474380
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2df3f03d8d0199bbc8bc057aeb8b78466aaf2bc9063a56c7a2627d01897f5abe",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-06-19T20:30:04Z",
"title_canon_sha256": "9ec6fbf087fb342d13d2880b91bcaae861cd4d56147331ab9579940c2ba3f6e6"
},
"schema_version": "1.0",
"source": {
"id": "1406.5206",
"kind": "arxiv",
"version": 2
}
}