Pith Number
pith:YQRLMDSU
pith:2024:YQRLMDSUN5JPUUMZONEIJ2NKSN
not attested
not anchored
not stored
refs pending
The Interplay between the IMF and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities
arxiv:2405.00813 v1 · 2024-05-01 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{YQRLMDSUN5JPUUMZONEIJ2NKSN}
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 | 2026-07-05T08:14:26.544029Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
c422b60e546f52fa5199734884e9aa93463aa27ad02395a1d342c9376de44c4f
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/YQRLMDSUN5JPUUMZONEIJ2NKSN \
| 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: c422b60e546f52fa5199734884e9aa93463aa27ad02395a1d342c9376de44c4f
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "8cbdf389445a22c7259e11b0266bd4fd0c0a9b4cfdb113964c47dd04a78a96c0",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2024-05-01T18:53:38Z",
"title_canon_sha256": "b12cf382c2453887a47b9cfa7bf35cc67a9a1cc40ddcd58a3f6a4ee305c919c5"
},
"schema_version": "1.0",
"source": {
"id": "2405.00813",
"kind": "arxiv",
"version": 1
}
}