Pith Number
pith:UVSFNQSP
pith:2006:UVSFNQSPNDZA63GUHTV3XC6FQF
not attested
not anchored
not stored
refs pending
Extreme gas kinematics in the z=2.2 powerful radio galaxy MRC1138-262: Evidence for efficient AGN feedback in the early Universe?
arxiv:astro-ph/0606530 v1 · 2006-06-21 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{UVSFNQSPNDZA63GUHTV3XC6FQF}
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.
Cited by
Receipt and verification
| First computed | 2026-07-04T15:19:05.934088Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a56456c24f68f20f6cd43cebbb8bc581781e1b27f764539ea7208ebe25a6030c
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UVSFNQSPNDZA63GUHTV3XC6FQF \
| 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: a56456c24f68f20f6cd43cebbb8bc581781e1b27f764539ea7208ebe25a6030c
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e6744639f18e8ef6bee0a4e7350d00e3e112990f52d505e555b3f79ad5d67702",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2006-06-21T17:48:04Z",
"title_canon_sha256": "0ebb1a6bf40d97a52f32555ab86a0ffbbeb6b5fd8ba4d3f561ee4f76c03451fe"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0606530",
"kind": "arxiv",
"version": 1
}
}