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pith:23I3TOIZ

pith:2010:23I3TOIZ72BO5OSF6LLKBQNXHX
not attested not anchored not stored refs pending

What Does a Submillimeter Galaxy Selection Actually Select? The Dependence of Submillimeter Flux Density on Star Formation Rate and Dust Mass

Christopher C. Hayward (CfA), Desika Narayanan (Arizona), Du\v{s}an Kere\v{s} (Berkeley), Lars Hernquist (CfA), Patrik Jonsson (CfA), T. J. Cox (Carnegie)

arxiv:1101.0002 v2 · 2010-12-29 · astro-ph.CO

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2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open

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1 paper in Pith

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First computed2026-05-18T03:48:24.466287Z
Builderpith-number-builder-2026-05-17-v1
SignaturePith Ed25519 (pith-v1-2026-05) · public key
Schemapith-number/v1.0

Canonical hash

d6d1b9b919fe82eeba45f2d6a0c1b73df9bf8679afaec77cf89ad361a4ded0e6

Aliases

arxiv: 1101.0002 · arxiv_version: 1101.0002v2 · doi: 10.48550/arxiv.1101.0002 · pith_short_12: 23I3TOIZ72BO · pith_short_16: 23I3TOIZ72BO5OSF · pith_short_8: 23I3TOIZ
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/23I3TOIZ72BO5OSF6LLKBQNXHX \
  | 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: d6d1b9b919fe82eeba45f2d6a0c1b73df9bf8679afaec77cf89ad361a4ded0e6
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "a7c8440c4c1bc71139c1c9aa9972f334195ee8f311ec9174dabc2a29e369d003",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2010-12-29T21:00:02Z",
    "title_canon_sha256": "052927a81689418c7dfcd6616715acdbae08c6e7acc8fcd5be4734331f1e737c"
  },
  "schema_version": "1.0",
  "source": {
    "id": "1101.0002",
    "kind": "arxiv",
    "version": 2
  }
}