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Nouveau transit
04/12/2024
HAT-P-4 b
56
Manfred Raetz, Privatsternwarte Herges-Hallenberg, 13/05/2024
SCT 280 / 1870 (C11 with Starizona reducer)+ CCD MII G2-1600
filter : Astrodon ExoPlanet-BB (V to IR)
filter : Astrodon ExoPlanet-BB (V to IR)
. . .
Nouvelle observation
04/12/2024
HAT-P-4
51
Manfred Raetz, Privatsternwarte Herges-Hallenberg, 13/05/2024
SCT 280 / 1870 (C11 with Starizona reducer)+ CCD MII G2-1600
filter : Astrodon ExoPlanet-BB (V to IR)
filter : Astrodon ExoPlanet-BB (V to IR)
. . .
Nouveau transit
01/05/2019
HAT-P-4 b
56
Veli-Pekka Hentunen, Taurus Hill Observatory (A95), Varkaus, Finland
C-14, Paramount MEII, ST-8XME
60 sec exposures, clouds, bright north sky
60 sec exposures, clouds, bright north sky
. . .
Nouveau transit
20/03/2016
HAT-P-4 b
56
Veli-Pekka Hentunen, Taurus Hill Observatory (A95), Varkaus, Finland
Meade 16" ACF OTA, Paramount ME, SBIG ST-8XME
601 unfiltered images, 30 sec exposures, seven comparison stars used, almost full moon
601 unfiltered images, 30 sec exposures, seven comparison stars used, almost full moon
. . .
Nouveau transit
12/02/2016
HAT-P-4 b
56
Francesco Scaggiante, Danilo Zardin, Gruppo Astrofili Salese Galileo Galilei S.M di Sala (Venezia ) ITALIA
Newton 410/1710 ccd Audine KAF1600 ME
. . .
Nouveau transit
05/11/2015
HAT-P-4 b
56
Stan Shadick, University of Saskatchewan Physics Roof Observatory, CANADA
Meade 10" LX200GPS; SBIG ST10XME CCD
Processed with artificial star at 8x5x10 at binning 2.
Used only reference stars C1-C9, C11.
Pier 3.
Processed with artificial star at 8x5x10 at binning 2.
Used only reference stars C1-C9, C11.
Pier 3.
. . .
Nouveau transit
03/04/2013
HAT-P-4 b
56
Veli-Pekka Hentunen, Taurus Hill Observatory, Varkaus, Finland
C-14 OTA, Paramount ME, SBIG ST-8XME
Corrected light curve model-fit of data. Differently calculated model-fit data was posted a few hours ago.
Corrected light curve model-fit of data. Differently calculated model-fit data was posted a few hours ago.
. . .
Nouveau transit
08/07/2012
HAT-P-4 b
56
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 12\\\" LX200; SBIG ST10XME CCD
Processed with artifical star at 8x4x10 at binning 2.
Used only reference stars C1, C2, C5, C8, C10.
Pier 5.
Processed with artifical star at 8x4x10 at binning 2.
Used only reference stars C1, C2, C5, C8, C10.
Pier 5.
. . .
Nouveau transit
11/04/2012
HAT-P-4 b
56
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 12\\\" LX200; SBIG ST10XME CCD
CBB FILTER.
Processed using artificial star at 8x4x10 at binning 2.
Used only reference stars C1, C2, C4-C7, C9-C11, C13.
Pier 5
CBB FILTER.
Processed using artificial star at 8x4x10 at binning 2.
Used only reference stars C1, C2, C4-C7, C9-C11, C13.
Pier 5
. . .
Nouveau transit
10/04/2012
HAT-P-4 b
56
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 10\\\" LX200GPS; SBIG ST10XME CCD
Processed with artificial star at 8x4x10 at binning 2.
Used only reference stars C1, C3, C5,C6,C9-C12, C14.
Pier 3.
Simultaneous observation with another dataset from pier 5 with cbb filter.
Processed with artificial star at 8x4x10 at binning 2.
Used only reference stars C1, C3, C5,C6,C9-C12, C14.
Pier 3.
Simultaneous observation with another dataset from pier 5 with cbb filter.
. . .
Nouveau transit
02/04/2010
HAT-P-4 b
56
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 12\\\\\\\" LX200; SBIG ST9ECCD
used 16 reference stars with Bruce Gary\\\'s Artificial Star Spreadsheet technique 7X1X7 ApertureXGapXAnnulus
used 16 reference stars with Bruce Gary\\\'s Artificial Star Spreadsheet technique 7X1X7 ApertureXGapXAnnulus
. . .
RL200, f/6 + ST8, guider RF80/600+G1-0300
180s exposure with autoguiding, only a first half of transit captured, superposited with observation from 30th March 2009 (4 cycles ago), where egress was captured. Per = 3.056536d was used for superpositing. No vertical shifts were applied to the data.
180s exposure with autoguiding, only a first half of transit captured, superposited with observation from 30th March 2009 (4 cycles ago), where egress was captured. Per = 3.056536d was used for superpositing. No vertical shifts were applied to the data.
. . .