Pith Number
pith:GQIJH3KR
pith:2020:GQIJH3KRQLSHUKJ5PNYCAD2VLE
not attested
not anchored
not stored
refs pending
Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
arxiv:2010.06605 v1 · 2020-10-13 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{GQIJH3KRQLSHUKJ5PNYCAD2VLE}
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.
Receipt and verification
| First computed | 2026-07-05T01:48:56.388617Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
341093ed5182e47a293d7b70200f55592105b72c9d265bc835d67104ba2b010a
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/GQIJH3KRQLSHUKJ5PNYCAD2VLE \
| 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: 341093ed5182e47a293d7b70200f55592105b72c9d265bc835d67104ba2b010a
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "f85debc04407c51287030c7bcc09d534876603f82550dfa094f6f416efb9d043",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2020-10-13T18:02:48Z",
"title_canon_sha256": "1c70cc8149bb9e451f845e3eecc0388c2187df5ad1676a624857e8bb23dbd199"
},
"schema_version": "1.0",
"source": {
"id": "2010.06605",
"kind": "arxiv",
"version": 1
}
}