Pith Number
pith:TLIBPSF7
pith:2016:TLIBPSF73LQWAV3UWPJJLBZRRR
not attested
not anchored
not stored
refs pending
The dust-to-stellar mass ratio as a valuable tool to probe the evolution of local and distant star forming galaxies
arxiv:1610.08979 v1 · 2016-10-27 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{TLIBPSF73LQWAV3UWPJJLBZRRR}
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.
Cited by
Receipt and verification
| First computed | 2026-05-18T00:55:40.517612Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
9ad017c8bfdae1605774b3d29587318c72c39b13d52debff86d22515d08363d7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/TLIBPSF73LQWAV3UWPJJLBZRRR \
| 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: 9ad017c8bfdae1605774b3d29587318c72c39b13d52debff86d22515d08363d7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cad2773905bb0f085b51decc5482cfa35108d0e48d093187a7f864c98c643a33",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2016-10-27T20:00:01Z",
"title_canon_sha256": "f27d0bfb6e48e815047055493fb92bfc3b895f8f7b99793990a0132e637b0cd4"
},
"schema_version": "1.0",
"source": {
"id": "1610.08979",
"kind": "arxiv",
"version": 1
}
}