Pith Number
pith:RXYRV4GV
pith:2023:RXYRV4GVGVUFKSF6AH4J7FRI2M
not attested
not anchored
not stored
refs pending
The advantage of Bolometric Interferometry for controlling Galactic foreground contamination in CMB primordial B-modes measurements
arxiv:2311.01814 v1 · 2023-11-03 · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{RXYRV4GVGVUFKSF6AH4J7FRI2M}
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
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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 | 2026-07-05T07:08:45.549198Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8df11af0d535685548be01f89f9628d33facf6add8d2568b3462ac05c3fea53e
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RXYRV4GVGVUFKSF6AH4J7FRI2M \
| 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: 8df11af0d535685548be01f89f9628d33facf6add8d2568b3462ac05c3fea53e
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "7106ef199b77e9b101cf436530eb85ad813b54fef25f9368411422bc447006eb",
"cross_cats_sorted": [],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2023-11-03T09:47:24Z",
"title_canon_sha256": "32e9120d556d9d5abcb774348eef422b78125cfe2364e8ea987ea3ff41d98abb"
},
"schema_version": "1.0",
"source": {
"id": "2311.01814",
"kind": "arxiv",
"version": 1
}
}