Pith Number
pith:Q7P7VECO
pith:2015:Q7P7VECOK5QR4CXIIMNQN4VXRF
not attested
not anchored
not stored
refs pending
Thermal absorption as the cause of gigahertz-peaked spectra in pulsars and magnetars
arxiv:1505.07243 v1 · 2015-05-27 · astro-ph.HE
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{Q7P7VECOK5QR4CXIIMNQN4VXRF}
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 | 2026-05-18T01:35:47.551475Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
87dffa904e57611e0ae8431b06f2b78977b6f72b52eeebb8345e1ab052e57fcf
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Q7P7VECOK5QR4CXIIMNQN4VXRF \
| 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: 87dffa904e57611e0ae8431b06f2b78977b6f72b52eeebb8345e1ab052e57fcf
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "a692f786df13b32fdb43c4e8178b6fcc9197b7627eed1aaaed1ddd9c5e686751",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.HE",
"submitted_at": "2015-05-27T09:46:56Z",
"title_canon_sha256": "e185c980e0962f978f042cdc246cf7d280db9a370c52f729bb814640b4a74a69"
},
"schema_version": "1.0",
"source": {
"id": "1505.07243",
"kind": "arxiv",
"version": 1
}
}