Pith Number
pith:6GV5Q3ZP
pith:2019:6GV5Q3ZPSSLHX6J7MDO2K6JZKW
not attested
not anchored
not stored
refs pending
Near-infrared [Fe II] and H$_{2}$ Emission-line Study of Galactic Supernova Remnants in the First Quadrant
arxiv:1902.03847 v1 · 2019-02-11 · astro-ph.GA
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{6GV5Q3ZPSSLHX6J7MDO2K6JZKW}
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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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 | 2026-05-17T23:52:36.003731Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
f1abd86f2f94967bf93f60dda5793955a36ca6373bc5e7cdc811efc9b41ac5d8
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/6GV5Q3ZPSSLHX6J7MDO2K6JZKW \
| 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: f1abd86f2f94967bf93f60dda5793955a36ca6373bc5e7cdc811efc9b41ac5d8
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "9e047b8a0d92d2eb013eb8cc5a763cd529111e0da866ad6a069480913846c8d3",
"cross_cats_sorted": [],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "astro-ph.GA",
"submitted_at": "2019-02-11T12:50:49Z",
"title_canon_sha256": "37da7c5052419b621223635c1aa4b86c8e4c631e185f86865d881c05fc7addf8"
},
"schema_version": "1.0",
"source": {
"id": "1902.03847",
"kind": "arxiv",
"version": 1
}
}