Pith Number
pith:TFNNGC6T
pith:2019:TFNNGC6TDHK3KE33MOU2ESVPHW
not attested
not anchored
not stored
refs pending
SILVERRUSH. IX. Lya Intensity Mapping with Star-Forming Galaxies at z=5.7 and 6.6: A Possible Detection of Extended Lya Emission at $\gtrsim$100 comoving kpc around and beyond the Virial-Radius Scale of Galaxy Dark Matter Halos
arxiv:1906.00173 v2 · 2019-06-01 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{TFNNGC6TDHK3KE33MOU2ESVPHW}
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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 | 2026-07-05T03:06:09.147111Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
995ad30bd319d5b5137b63a9a24aaf3db47ab4b755f3f69b9ea6f596f2bb71e0
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/TFNNGC6TDHK3KE33MOU2ESVPHW \
| 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: 995ad30bd319d5b5137b63a9a24aaf3db47ab4b755f3f69b9ea6f596f2bb71e0
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "6ad07efeb70d0bdb56d77dfe098393c6fd3cbd8f980b85b81405dcf1f6d8ad51",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-06-01T07:46:40Z",
"title_canon_sha256": "c64d7960eb0e5b8c7b9cd1ece88a101a6c8bc4a15d790d09590ee31ebdadd384"
},
"schema_version": "1.0",
"source": {
"id": "1906.00173",
"kind": "arxiv",
"version": 2
}
}