Pith Number
pith:OMTW4NGI
pith:2003:OMTW4NGIZEYLRBRIHRENYTV5UB
not attested
not anchored
not stored
refs pending
Kinematic Masses of Super Star Clusters in M82 from High-Resolution Near-Infrared Spectroscopy
arxiv:astro-ph/0306373 v1 · 2003-06-18 · astro-ph
Add to your LaTeX paper
\usepackage{pith}
\pithnumber{OMTW4NGIZEYLRBRIHRENYTV5UB}
Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge
Record completeness
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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.
Cited by
Receipt and verification
| First computed | 2026-07-04T16:52:00.676020Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
73276e34c8c930b886283c48dc4ebda06f40c6a47741c2c11c7c8b21fadbf023
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OMTW4NGIZEYLRBRIHRENYTV5UB \
| 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: 73276e34c8c930b886283c48dc4ebda06f40c6a47741c2c11c7c8b21fadbf023
Canonical record JSON
{
"metadata": {
"abstract_canon_sha256": "2dcd582574654f6856e001aaae0be832ea1b2285025eeb2f22618d3c8925e7e8",
"cross_cats_sorted": [],
"license": "",
"primary_cat": "astro-ph",
"submitted_at": "2003-06-18T20:00:17Z",
"title_canon_sha256": "c4eda186f4f6679d0875e17f28eeac0d0ab8232a911ab5e05b13de6beb6f6304"
},
"schema_version": "1.0",
"source": {
"id": "astro-ph/0306373",
"kind": "arxiv",
"version": 1
}
}