新しいトランジット
2023/05/29
HAT-P-33 b
31
Andre Kovacs, Erika Pakštienė, Moletai Astronomical Observatory (MAO)
35/51 cm Maksutov f/3.5 (MAO) Apogee Alta U47-BB
RAW data calibrated and reduced using AstroImageJ, including information on AIRMASS and additional (optional) detrending parameters for Width_T1.
RAW data calibrated and reduced using AstroImageJ, including information on AIRMASS and additional (optional) detrending parameters for Width_T1.
. . .
新しいトランジット
2023/05/29
HAT-P-33 b
31
Andre Kovacs, Erika Pakštienė, Moletai Astronomical Observatory (MAO)
35/51 cm Maksutov f/3.5 (MAO) Apogee Alta U47-BB
RAW data calibrated and reduced using AstroImageJ, including information on AIRMASS and additional (optional) detrending parameters for X(FITS)_T1 and Y(FITS)_T1.
RAW data calibrated and reduced using AstroImageJ, including information on AIRMASS and additional (optional) detrending parameters for X(FITS)_T1 and Y(FITS)_T1.
. . .
新しいトランジット
2019/02/05
HAT-P-33 b
31
Francesco Scaggiante, Danilo Zardin, Gruppo Astrofili Salese Galileo Galilei S.M di Sala (Venezia ) ITALIA
Newton 410/1710 ccd Audine KAF1600 ME
exposure 30"
exposure 30"
. . .
新しいトランジット
2012/05/24
HAT-P-33 b
31
Tanya Dax, Ortega Telescope/Olin Observatory - Florida Institute of Technology
0.8-m Ortega with Andor CCD
. . .
新しいトランジット
2011/11/06
HAT-P-33 b
31
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 12\\\" LX200; SBIG ST10XMECCD
CBB filter
Processed with artificial star technique at 8x4x10
Used only reference stars C1, C2, C4, C6, C7
CBB filter
Processed with artificial star technique at 8x4x10
Used only reference stars C1, C2, C4, C6, C7
. . .
新しいトランジット
2011/10/31
HAT-P-33 b
31
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 10\\\" LX200GPS; SBIG ST10XMECCD
CBB filter
Processed using Bruce Gary\\\'s artificial star technique at 7x4x10.
Used only reference stars C1-C6, C8, C11, C14, C15
CBB filter
Processed using Bruce Gary\\\'s artificial star technique at 7x4x10.
Used only reference stars C1-C6, C8, C11, C14, C15
. . .