Pith Number

pith:VWEGD6VL

pith:2009:VWEGD6VLHKLA3LJUEIDIWRYIMI

not attested not anchored not stored refs pending

The MAXI Mission on the ISS: Science and Instruments for Monitoring All Sky X-Ray Images

2), (2) Cosmic Radiation Laboratory, (3) Department of Earth, (4) Department of Physics, (5) Department of Physics, (6) Department of Physics, (7) Department of Astronomy, (8) Earth Observation Research Center, (9) ISAS, Aoyama Gakuin University, Atsumasa Yoshida (5), Emi Miyata (3), Haruyoshi Katayama (8), Hiroshi Tomida (1), Hiroshi Tsunemi (3), Hirotaka Chujo (2), Hitoshi Negoro (6), ISAS, JAXA, JAXA), Jun Kataoka (4), Kazuo Hiroi (7), Kazutaka Yamaoka (5), Kazuyoshi Kawasaki (1), Ken Ebisawa (9) ((1) ISS Science Project Office, Kyoto University, Masaki Ishikawa (1), Masaru Matsuoka (1), Mathematics, Mikio Morii (4), Mitsuhiro Kohama (1, Motoki Nakajima (6), Motoko Suzuki (1), Mutsumi Sugizaki (2), Naoki Isobe (2), Nihon University, Nobuyuki Kawai (4), Osaka University, Osamu Yamazaki (5), RIKEN, Ryoji Ishiwata (6), Satoshi Eguchi (7), Satoshi Nakahira (5), Shiro Ueno (1), Sho Miyoshi (6), Space Science, Tatehiro Mihara (2), Tetsuya You (5), Tokyo Institute of Technology, Yasuki Adachi (1), Yoshihiro Ueda (7), Yujin Nakagawa (2)

arxiv:0906.0631 v1 · 2009-06-03 · astro-ph.IM · astro-ph.HE

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Add to your LaTeX paper

\usepackage{pith}
\pithnumber{VWEGD6VLHKLA3LJUEIDIWRYIMI}

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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

7 papers in Pith

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

Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass

Tracing the outburst decay of soft X-ray transients Aql X-1 and 4U 1608-52 with XSPECT

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207

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

Receipt and verification

First computed	2026-05-18T02:13:29.470685Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

ad8861faab3a960dad3422068b47086216522222315c47c54fcccdc775d49721

Aliases

arxiv: 0906.0631 · arxiv_version: 0906.0631v1 · doi: 10.48550/arxiv.0906.0631 · pith_short_12: VWEGD6VLHKLA · pith_short_16: VWEGD6VLHKLA3LJU · pith_short_8: VWEGD6VL

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/VWEGD6VLHKLA3LJUEIDIWRYIMI \
  | 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: ad8861faab3a960dad3422068b47086216522222315c47c54fcccdc775d49721

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "d0b979e481a253a091951be825e7809be45966c60ba6961bcfdcfaa9afa6e8ea",
    "cross_cats_sorted": [
      "astro-ph.HE"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "primary_cat": "astro-ph.IM",
    "submitted_at": "2009-06-03T02:48:01Z",
    "title_canon_sha256": "1a2304d648e785d677fab891b6537da1d755247070b7b233c67b9feef2440992"
  },
  "schema_version": "1.0",
  "source": {
    "id": "0906.0631",
    "kind": "arxiv",
    "version": 1
  }
}