Pith Number
pith:EKJWJHIT
pith:1996:EKJWJHITS2EKVYXXB2FW3I65RZ
not attested
not anchored
not stored
refs pending
Self-similarity and scaling behavior of IR emission from radiatively heated dust: I. Theory
arxiv:astro-ph/9612164 v1 · 1996-12-17 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{EKJWJHITS2EKVYXXB2FW3I65RZ}
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
· 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.
Cited by
Receipt and verification
| First computed | 2026-05-18T01:40:18.598953Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2293649d139688aae2f70e8b6da3dd8e639b010701df97606d4c9ecde070a12e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/EKJWJHITS2EKVYXXB2FW3I65RZ \
| 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: 2293649d139688aae2f70e8b6da3dd8e639b010701df97606d4c9ecde070a12e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "dbac203dd865e891c4b83e7bc05bbb112c34372fbf5a729156f0ef087e5155b4",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "1996-12-17T16:45:22Z",
"title_canon_sha256": "2bb56403770f88498c30542755d4ccc4fdfb95fe07417a046c05faaa90f21a4d"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/9612164",
"kind": "arxiv",
"version": 1
}
}