NV Cnc (食連星)

RA: 08h 16m 12.88s, DE: +26° 41' 13.70" (124.0536666567, 26.6871388886)

2026/03/09, 01:44 - 2026/03/09, 03:56 (UTC)

データ:

  • 観測者: Bill Tschumy
  • 作成: 2026/03/09, 17:30
  • 観測所: Home Observatory
    Lat: +40°, Long: -105°
  • 観測装置: Agema 130 SD; ZWO 2600MM Pro, V,B
  • 測光バンド: V
  • 基準時: Gjd
  • 光度: Mag
決定された極小
  • S: 2461108.62707 (2026/03/09, 03:02)
    HJDmin: 2461108.63085 +/- 0.00063  
    太陽中心補正: 0.00379
    注釈:
    Note:  The info on NC Cnc says that the minimum brightness for the secondary eclipse is 11.6 V.  From my reading last night, the secondary has a very shallow eclipse and the minimum is 11.15 V.
    
    I'm also curious about the small hump I observed buying the secondary minimum.  I haven't been able to show this as an artifact.  It seems real.  Not sure what would cause it.
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光度曲線
近傍の天体、比較星や確認用の恒星
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