Pith Number
pith:IKUQTVLC
pith:2015:IKUQTVLCKTHDXZ2EX4U7TN6KHQ
not attested
not anchored
not stored
refs pending
A model for the polarization of the high-energy radiation from accreting black holes: the case of XTE J1118+480
arxiv:1512.09015 v1 · 2015-12-30 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{IKUQTVLCKTHDXZ2EX4U7TN6KHQ}
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 | 2026-05-18T01:20:32.473022Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
42a909d56254ce3be744bf29f9b7ca3c145971bad6c44b1d88be6e9aa7a5dab7
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/IKUQTVLCKTHDXZ2EX4U7TN6KHQ \
| 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: 42a909d56254ce3be744bf29f9b7ca3c145971bad6c44b1d88be6e9aa7a5dab7
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "cb87755a566bcc79a6783ebd39a01809fcc0d986425a47cdee3579e674e1f770",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2015-12-30T17:05:28Z",
"title_canon_sha256": "bfe8769d54b61da29dc42fb5d392509d3116994600c5e95062fcb926d90142d2"
},
"schema_version": "1.0",
"source": {
"id": "1512.09015",
"kind": "arxiv",
"version": 1
}
}