Pith Number

pith:L474BHNW

pith:2009:L474BHNWHSMA2UOGK5YHOSVGPE

not attested not anchored not stored refs pending

The Lick AGN Monitoring Project: Broad-Line Region Radii and Black Hole Masses from Reverberation Mapping of Hbeta

10), (10) Dept. of Physics, (11) Institute of Astronomy, 12), (12) Dept. of Astronomy, (13) Jet Propulsion Laboratory, 14), (14) Physics Dept., 15) ((1) Dept. of Physics, (15) Research Center for the Early Universe, (2) Dept. of Physics, 3, 3), (3) Las Cumbres Observatory Global Telescope, 4), (4) Institute of Geophysics, 5), (5) Dept. of Physics, (6) Dept. of Astronomy, (7) Lick Observatory, (8) Princeton University Observatory, 9), (9) School of Physics, Aaron J. Barth (1), Alexei V. Filippenko (6), Astronomy, Carol E. Thornton (1), Daniel Stern (13), Elinor L. Gates (7), Frank J. D. Serduke (6), Gabriela Canalizo (4, Jeffrey M. Silverman (6), Jenny E. Greene (8), Jonelle L. Walsh (1), Jong-Hak Woo (2, Kyle D. Hiner (4, Marton G. Hidas (2, Matthew A. Malkan (10), Misty C. Bentz (1), Mohan Ganeshalingam (6), Nairn Baliber (2, Nicholas Lee (6), Nicola Bennert (2, Planetary Physics, Rachel A. Street (2, School of Science, Takeo Minezaki (11), Thea N. Steele (6), Tommaso Treu (2), Tsinghua Center for Astrophysics, Tsinghua University, UC Berkeley, UC Irvine, UCLA, UC Riverside, UC Santa Barbara, University of Sydney, University of Tokyo, University of Tokyo), Weidong Li (6), Xiaofeng Wang (6, Yu Sakata (11, Yuzuru Yoshii (11

arxiv:0908.0003 v1 · 2009-07-31 · astro-ph.CO

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{L474BHNWHSMA2UOGK5YHOSVGPE}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ 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

2 papers in Pith

Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion

Receipt and verification

First computed	2026-05-18T02:12:45.602579Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

5f3fc09db63c980d51c65770774aa67927f5f473e155ed57890cb47ca4f64b8b

Aliases

arxiv: 0908.0003 · arxiv_version: 0908.0003v1 · doi: 10.48550/arxiv.0908.0003 · pith_short_12: L474BHNWHSMA · pith_short_16: L474BHNWHSMA2UOG · pith_short_8: L474BHNW

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/L474BHNWHSMA2UOGK5YHOSVGPE \
  | 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: 5f3fc09db63c980d51c65770774aa67927f5f473e155ed57890cb47ca4f64b8b

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "3ffd4111e2b278330f266d096f11fd2ced30504c65624671bc26e571adefedbc",
    "cross_cats_sorted": [],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2009-07-31T20:04:26Z",
    "title_canon_sha256": "f141b5c6fe2f7b83e675bb0f134884c961568165ca0b2ccf55496dd8b68cb7eb"
  },
  "schema_version": "1.0",
  "source": {
    "id": "0908.0003",
    "kind": "arxiv",
    "version": 1
  }
}