Pith Number
pith:PYGSCLR2
pith:2017:PYGSCLR2722OL7GSHVBG3SQBCO
not attested
not anchored
not stored
refs pending
The Shape of the Cosmic X-ray Background: Nuclear Starburst Discs and the Redshift Evolution of AGN Obscuration
arxiv:1711.05268 v2 · 2017-11-14 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{PYGSCLR2722OL7GSHVBG3SQBCO}
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 | 2026-05-18T00:22:27.448415Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
7e0d212e3afeb4e5fcd23d426dca0113aaff55eb6a61b6d97e09e9d7d341c3d2
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/PYGSCLR2722OL7GSHVBG3SQBCO \
| 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: 7e0d212e3afeb4e5fcd23d426dca0113aaff55eb6a61b6d97e09e9d7d341c3d2
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "fa18de6ad8adbecc991b6e6ac1aa3d70dffb5282a697b290481377a0268006bc",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2017-11-14T19:00:01Z",
"title_canon_sha256": "837a99cb61dbf789cb267d4ecc0436bb9bca533b2c2cfc542603027f9263264e"
},
"schema_version": "1.0",
"source": {
"id": "1711.05268",
"kind": "arxiv",
"version": 2
}
}