Pith Number
pith:M5NVTBLD
pith:2019:M5NVTBLD2Z6J7BU73TNV6VPJ45
not attested
not anchored
not stored
refs pending
Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
arxiv:1903.06183 v1 · 2019-03-14 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{M5NVTBLD2Z6J7BU73TNV6VPJ45}
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 | 2026-05-17T23:47:25.311149Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
675b598563d67c9f869fdcdb5f55e9e77a345be2301beb518a0076ae3b21e6ae
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/M5NVTBLD2Z6J7BU73TNV6VPJ45 \
| 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: 675b598563d67c9f869fdcdb5f55e9e77a345be2301beb518a0076ae3b21e6ae
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "e206960ec0823b1fbb91ed5bde3b1dd2c28145ce4f12ed58f819b3c33ab06905",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-03-14T18:00:05Z",
"title_canon_sha256": "f7d5a1b3b752499bcecfa0a29805d48ce1246911db4f4867b13c4b7fd29d1731"
},
"schema_version": "1.0",
"source": {
"id": "1903.06183",
"kind": "arxiv",
"version": 1
}
}