Pith Number
pith:5MBZGQDV
pith:2018:5MBZGQDVAYUESMP5G44AVPEPWK
not attested
not anchored
not stored
refs pending
Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
arxiv:1803.05446 v2 · 2018-03-14 · astro-ph.GA · astro-ph.CO
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{5MBZGQDVAYUESMP5G44AVPEPWK}
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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.
Receipt and verification
| First computed | 2026-05-18T00:03:49.379440Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
eb0393407506284931fd37380abc8fb2966703de6beffb1786df33ac53dfef94
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/5MBZGQDVAYUESMP5G44AVPEPWK \
| 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: eb0393407506284931fd37380abc8fb2966703de6beffb1786df33ac53dfef94
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "644623ab8d753f90d1109baabe50be15c19ae36ff0a850b9504a7e73534c1db1",
"cross_cats_sorted": [
"astro-ph.CO"
],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2018-03-14T18:00:11Z",
"title_canon_sha256": "8bfd5bc7d646816b52f46f909f5e8e1df938ffaa3fc269c03b8fdec23913ef71"
},
"schema_version": "1.0",
"source": {
"id": "1803.05446",
"kind": "arxiv",
"version": 2
}
}