Pith Number
pith:P744P3LQ
pith:2014:P744P3LQWH4ZZUR5CGKJI6EF2O
not attested
not anchored
not stored
refs pending
The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30$^{\circ}$,0$^{\circ}$)
arxiv:1403.3327 v1 · 2014-03-13 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{P744P3LQWH4ZZUR5CGKJI6EF2O}
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Record completeness
1
Bitcoin timestamp
2
Internet Archive
3
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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 | 2026-05-18T02:56:21.773832Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
7ff9c7ed70b1f99cd23d1194947885d386b3316c33f067877355ee45fc312ead
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/P744P3LQWH4ZZUR5CGKJI6EF2O \
| 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: 7ff9c7ed70b1f99cd23d1194947885d386b3316c33f067877355ee45fc312ead
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "48d7f3339904a01a3a41680891e4453fbbff02834ae49cc758f2923b2004656f",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-03-13T17:03:09Z",
"title_canon_sha256": "9ca8da9727c311d82587e07557fe16ede3fb3a6a91fd66b172b2ff699f1ef6b0"
},
"schema_version": "1.0",
"source": {
"id": "1403.3327",
"kind": "arxiv",
"version": 1
}
}