Pith Number
pith:73DHAWMT
pith:2017:73DHAWMTB3DX2CN7ONSFT35WVJ
not attested
not anchored
not stored
refs pending
Can Dust Injected by SNe Explain the NIR-MIR Excess in Young Massive Stellar Clusters?
arxiv:1705.08899 v1 · 2017-05-24 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{73DHAWMTB3DX2CN7ONSFT35WVJ}
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
· sign in to
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 | 2026-05-18T00:39:25.628226Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
fec67059930ec77d09bf736459efb6aa4c21f71e37e07929c3f28a477a93d4b6
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/73DHAWMTB3DX2CN7ONSFT35WVJ \
| 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: fec67059930ec77d09bf736459efb6aa4c21f71e37e07929c3f28a477a93d4b6
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "fbdc9bca5f2e309c640d25498eedd8daff3390f2e4827c49e83275cc16323520",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2017-05-24T18:00:02Z",
"title_canon_sha256": "6b28636ed4782ec1ee9bf9bf6de958ced0fbb25d017c88592926ec9739cf906e"
},
"schema_version": "1.0",
"source": {
"id": "1705.08899",
"kind": "arxiv",
"version": 1
}
}