新しいトランジット
2025/01/14
KELT-3 b
49
Samuel Diaz Lopez, Observatorio Tomas Lopez. AstroCamp. , 2025/01/14
SCA260 + Atik16200
. . .
新しいトランジット
2025/01/14
KELT-3 b
49
Samuel Diaz Lopez, Observatorio Tomas Lopez. AstroCamp. , 2025/01/14
SCA260 + Atik16200
. . .
新しいトランジット
2024/05/09
KELT-3 b
49
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 tot_C_cnts and J.D.-2400000.
RAW data calibrated and reduced using AstroImageJ, including information on AIRMASS and additional (optional) detrending parameters for tot_C_cnts and J.D.-2400000.
. . .
新しいトランジット
2022/04/20
KELT-3 b
49
Francesco Scaggiante, Danilo Zardin,Marco Fiaschi, Gruppo Astrofili Salese Galileo Galilei S.M di Sala (Venezia ) ITALIA
Newton 410/1710 ccd Audine KAF1600 ME
exposure 10"
exposure 10"
. . .
新しいトランジット
2021/04/01
KELT-3 b
49
Veli-Pekka Hentunen, Taurus Hill Observatory (A95), Varkaus, Finland
C-14, Paramount MEII, ST-8XME
40 sec exposures, five comparison stars, the transit was much earlier than predicted, towards the end of the transit the sky was cloudy
40 sec exposures, five comparison stars, the transit was much earlier than predicted, towards the end of the transit the sky was cloudy
. . .
新しいトランジット
2015/12/27
KELT-3 b
49
Stan Shadick, University of Saskatchewan Physics Roof Observatory, CANADA
Meade 14" LX200GPS; SBIG STL1301E
Processed with artificial star at 12x10x10 at binning 1.
Used only reference stars C1 and C2.
Pier 4.
Processed with artificial star at 12x10x10 at binning 1.
Used only reference stars C1 and C2.
Pier 4.
. . .
新しいトランジット
2015/02/19
KELT-3 b
49
Francesco Scaggiante, Danilo Zardin, Gruppo Astrofili Salese Galileo Galilei S.M di Sala (Venezia ) ITALIA
Newton 410/1710 ccd Audine KAF402ME
. . .
新しいトランジット
2013/01/04
KELT-3 b
49
Nello Ruocco, Osservatorio Astronomico \\\"Nastro Verde\\\" MPC C82
Meade LX200 f/10 with focal reducer + ST7
. . .