Pith Number
pith:G7LF44B3
pith:2014:G7LF44B3UQIV4GARH74NEGHKWP
not attested
not anchored
not stored
refs pending
Combining Physical galaxy models with radio observations to constrain the SFRs of high-z dusty star forming galaxies
arxiv:1412.3458 v1 · 2014-12-10 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{G7LF44B3UQIV4GARH74NEGHKWP}
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 | 2026-05-18T02:31:36.537785Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
37d65e703ba4115e18113ff8d218eab3fef408c3f847e6e3ba5c9ebca9b830cf
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/G7LF44B3UQIV4GARH74NEGHKWP \
| 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: 37d65e703ba4115e18113ff8d218eab3fef408c3f847e6e3ba5c9ebca9b830cf
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "0c18d82611828b3529c01325f476b3325d0e38a9f0f9d731f88a30e158d80203",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2014-12-10T21:00:06Z",
"title_canon_sha256": "43135e693e51a8f5d9bdf45a2d16ae233604b78d2c19bfb7ea89e572db1d6b9e"
},
"schema_version": "1.0",
"source": {
"id": "1412.3458",
"kind": "arxiv",
"version": 1
}
}