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Nový tranzit
16.04.2025
HAT-P-20 b
154
Maddie Abrants, Bridgewater State University Observatory, 3/8/2020
14" Celestron Edge HD
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Nové pozorování
16.04.2025
HAT-P-20
159
Maddie Abrants, Bridgewater State University Observatory, 3/8/2020
14" Celestron Edge HD
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Nový tranzit
24.01.2025
HAT-P-20 b
154
Mario Morales Aimar, Observatorio de Sencelles, Spain - MPC K14, 1/23/2025
Newtonian 250 mm f/4 - SBIG ST7XME - Atlas EQ-G mount, Astrodon V photometric filter
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Nové pozorování
24.01.2025
HAT-P-20
159
Mario Morales Aimar, Observatorio de Sencelles, Spain - MPC K14, 1/23/2025
Newtonian 250 mm f/4 - SBIG ST7XME - Atlas EQ-G mount, Astrodon V photometric filter
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Nový tranzit
29.12.2024
HAT-P-20 b
154
Nico Montigiani, Massimiliano Mannucci Associazione Astrofili Fiorentini, Osservatorio Astronomico Margherita Hack, Firenze, 12/28/2024
C14 f/8.25 + CCD SBIG ST10XME
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Nové pozorování
29.12.2024
HAT-P-20
159
Nico Montigiani, Massimiliano Mannucci Associazione Astrofili Fiorentini, Osservatorio Astronomico Margherita Hack, Firenze, 12/28/2024
C14 f/8.25 + CCD SBIG ST10XME
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Nový tranzit
22.12.2024
HAT-P-20 b
154
Brian Kendrick, North Mesa Observatory (IAU code V27), 12/20/2024
0.254m reflector F6.894
CCD Atik 383L+ (KAF-8300) MaximDL, 60sec exposures, 2x2 bin= 1.27 "/px, G filter.
CCD Atik 383L+ (KAF-8300) MaximDL, 60sec exposures, 2x2 bin= 1.27 "/px, G filter.
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Nové pozorování
22.12.2024
HAT-P-20
159
Brian Kendrick, North Mesa Observatory (IAU code V27), 12/20/2024
0.254m reflector F6.894
CCD Atik 383L+ (KAF-8300) MaximDL, 60sec exposures, 2x2 bin= 1.27 "/px, G filter.
CCD Atik 383L+ (KAF-8300) MaximDL, 60sec exposures, 2x2 bin= 1.27 "/px, G filter.
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Nový tranzit
03.12.2024
HAT-P-20 b
154
Gustavo Javier Muler Schteinman, Observatorio Nazaret J47 -ASTRONOMIA LANZAROTE -, 12/3/2024
LX 200 GPS 12" ST8XME
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Nové pozorování
03.12.2024
HAT-P-20
159
Gustavo Javier Muler Schteinman, Observatorio Nazaret J47 -ASTRONOMIA LANZAROTE -, 12/2/2024
LX 200 GPS 12" ST8XME
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C2PU/Epsilon, Cassegrain+ Focal reductor F/9, QSI 632, 84 images, 120s
Circumstances:
Those data were acquired during the practical phase of an Astronomy course delivered by the Côte d’Azur University (Diplôme Universitaire d’Astronomie Observationelle (https://www.oca.eu/fr/duao-oca#:~:text=Le%20DUAO%20(Dipl%C3%B4me%20Universitaire%20d,th%C3%A9orique%20et%20pratique%20en%20astronomie)
Data acquisition:
Date: Sunday, January 15th 2023, 1st image 18:56; 84th and last image: 21:55
Location : C2PU/Calern Observatory (IAU_010), France [long.: +6.92277, lat.: +43.75377, alt. 1260 m]
Telescope: Epsilon, Focal length 9.36m, Aperture diameter: 1.04m
Focus configuration: Cassegrain, + Focal reductor F/9
Science camera: QSI 632, temp.: -20°
Weather:
1st image: temp.: 2.6° (dome+outside), pressure: 864 mbar/hPa, wind: 4.4m/s, hum.: 62%
84th and last image: temp.: 2.3° (dome+outside), pressure: 863 mbar/hPa, wind: 5.3m/s, hum.: 44%
Observers:
Serge DURAND, Paris (serge.deuxieme@hotmail.com)
Alain ESCAFFRE (alain.escaffre@gmail.com)
Data processing:
Serge DURAND, Paris (serge.deuxieme@hotmail.com)
Note about pictures :
They were taken in a defocalised mode.
Important note : there is another star very near HAT-P-20 : UCAC3 229-88754 other name 2MASS 07273963+2420171. This star is fainter than HAT-P-20 by 1.36 mag (R).
Therefore the Real depth (in flux) is the observed one multiplied by 1.3
Circumstances:
Those data were acquired during the practical phase of an Astronomy course delivered by the Côte d’Azur University (Diplôme Universitaire d’Astronomie Observationelle (https://www.oca.eu/fr/duao-oca#:~:text=Le%20DUAO%20(Dipl%C3%B4me%20Universitaire%20d,th%C3%A9orique%20et%20pratique%20en%20astronomie)
Data acquisition:
Date: Sunday, January 15th 2023, 1st image 18:56; 84th and last image: 21:55
Location : C2PU/Calern Observatory (IAU_010), France [long.: +6.92277, lat.: +43.75377, alt. 1260 m]
Telescope: Epsilon, Focal length 9.36m, Aperture diameter: 1.04m
Focus configuration: Cassegrain, + Focal reductor F/9
Science camera: QSI 632, temp.: -20°
Weather:
1st image: temp.: 2.6° (dome+outside), pressure: 864 mbar/hPa, wind: 4.4m/s, hum.: 62%
84th and last image: temp.: 2.3° (dome+outside), pressure: 863 mbar/hPa, wind: 5.3m/s, hum.: 44%
Observers:
Serge DURAND, Paris (serge.deuxieme@hotmail.com)
Alain ESCAFFRE (alain.escaffre@gmail.com)
Data processing:
Serge DURAND, Paris (serge.deuxieme@hotmail.com)
Note about pictures :
They were taken in a defocalised mode.
Important note : there is another star very near HAT-P-20 : UCAC3 229-88754 other name 2MASS 07273963+2420171. This star is fainter than HAT-P-20 by 1.36 mag (R).
Therefore the Real depth (in flux) is the observed one multiplied by 1.3
. . .
400mm f6.8, ST10XME, AO8 guider.
240 second exposure through Rc filter. GPS time control. Partial due to clouds just prior to egress. NOTE ETD HJD conversion appears different to alternative conversion sources (E.g. https://doncarona.tamu.edu/apps/jd/) or AstroImageJ. Converted time is expected to be 459957.46491(HJD). ETD Tc(HJD) is 0.01d early.
240 second exposure through Rc filter. GPS time control. Partial due to clouds just prior to egress. NOTE ETD HJD conversion appears different to alternative conversion sources (E.g. https://doncarona.tamu.edu/apps/jd/) or AstroImageJ. Converted time is expected to be 459957.46491(HJD). ETD Tc(HJD) is 0.01d early.
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Nový tranzit
17.01.2023
HAT-P-20 b
154
Anaël Wünsche, UAI B10 Observatoire des Baronnies Provençales
Planewave 17" + ZWO ASI 6200 MM pro mono
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Nový tranzit
10.12.2020
HAT-P-20 b
154
Veli-Pekka Hentunen, Taurus Hill Observatory (A95), Varkaus, Finland
C-14, Paramount MEII, ST-8XME
60 sec exposures, three comparison stars, -5 C
60 sec exposures, three comparison stars, -5 C
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Takahashi FSQ 106 ED, QHY 183M
Observation hampered by clouds until about mid transit.
A light pollution reduction filter was used: Hoya intensifier red enhancer (didymium). Relative photometry analysis with AstroImageJ 3.4.0. Camera settings: Gain: 0, Sensor temperature: -30 °C, Exposure time: 60s
Observation hampered by clouds until about mid transit.
A light pollution reduction filter was used: Hoya intensifier red enhancer (didymium). Relative photometry analysis with AstroImageJ 3.4.0. Camera settings: Gain: 0, Sensor temperature: -30 °C, Exposure time: 60s
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Nový tranzit
04.04.2019
HAT-P-20 b
154
Veli-Pekka Hentunen, Taurus Hill Observatory (A95), Varkaus, Finland
C-14, Paramount MEII, ST-8XME
40 sec unfiltered exposures, 6 comparison stars
40 sec unfiltered exposures, 6 comparison stars
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Nový tranzit
14.02.2019
HAT-P-20 b
154
AAAV Astrofili Valdera, Oss Astr G.Galilei-Libbiano Mpc code B33
RC 500 f/6 + CCD FLI PROLINE 4710
AAAV-Ass.ne Astrofili Alta Valdera
(www.astrofilialtavaldera.it)
Observers: Alberto Villa.
Clear sky with moon
AAAV-Ass.ne Astrofili Alta Valdera
(www.astrofilialtavaldera.it)
Observers: Alberto Villa.
Clear sky with moon
. . .
Nový tranzit
14.02.2019
HAT-P-20 b
154
AAAV Astrofili Valdera, Oss Astr G.Galilei-Libbiano Mpc code B33
RC 500 f/6 + CCD FLI PROLINE 4710
AAAV-Ass.ne Astrofili Alta Valdera
(www.astrofilialtavaldera.it)
Observers: Alberto Villa.
Clear sky with Monn
AAAV-Ass.ne Astrofili Alta Valdera
(www.astrofilialtavaldera.it)
Observers: Alberto Villa.
Clear sky with Monn
. . .
Nový tranzit
01.02.2019
HAT-P-20 b
154
Francesco Scaggiante, Danilo Zardin, Gruppo Astrofili Salese Galileo Galilei S.M di Sala (Venezia ) ITALIA
Newton 410/1710 ccd Audine KAF1600 ME
esposure 35"
esposure 35"
. . .
Nový tranzit
30.03.2017
HAT-P-20 b
154
Francesco Scaggiante, Danilo Zardin, Gruppo Astrofili Salese Galileo Galilei S.M di Sala (Venezia ) ITALIA
Newton 410/1710 ccd Audine KAF1600 ME
. . .