New transit
7/20/2024
WASP-123 b
11
Eduardo Fernández Lajús, Romina P. Di Sisto, Complejo Astronómico El Leoncito, Argentina
0.6 m Telescope + SBIG STL 1001 CCD
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New transit
9/4/2020
WASP-123 b
11
Alfa Crucis - De Carvalho Aguiar P., Kulh D., Olim E., Rodrigues M.A., Silva S., Treü R., TUGA – Porto Feliz, Sao Paulo, Brazil
Celestron C11 Edge HD, Lens: Hyperstar F2, Sensor: ASI071MC Pro (color), Mount: iOptron CEM60
Filter: IDAS D1 QRO + "Green-channel - in a CMOS sensor". 50s exposures. Average of the 2 green-channels. Weighted ensemble photometry with 2 comp stars, apertures (4, 7, 11). More about Alfa Crucis: https://alfacrucis.org/
Filter: IDAS D1 QRO + "Green-channel - in a CMOS sensor". 50s exposures. Average of the 2 green-channels. Weighted ensemble photometry with 2 comp stars, apertures (4, 7, 11). More about Alfa Crucis: https://alfacrucis.org/
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New transit
7/16/2020
WASP-123 b
11
Alfa Crucis - Kulh D., Olim E., Rodrigues M.A., Silva S., Treü R., TUGA – Porto Feliz, Sao Paulo, Brazil
Celestron C11 Edge HD, Lens: Optec F6.2 reducer, Sensor: Atik 414ex, Mount: iOptron CEM60
Filter: ZWO - G (wavelength: 480-600nm). 7s exposures binned 2x2. Each data point is the average of 5 images.
Weighted ensemble photometry with 9 comp stars, apertures (4, 7, 11). Duration estimation has been compromised due to instrumental issues. More about Alfa Crucis: https://alfacrucis.org/
Filter: ZWO - G (wavelength: 480-600nm). 7s exposures binned 2x2. Each data point is the average of 5 images.
Weighted ensemble photometry with 9 comp stars, apertures (4, 7, 11). Duration estimation has been compromised due to instrumental issues. More about Alfa Crucis: https://alfacrucis.org/
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New transit
7/16/2020
WASP-123 b
11
Alfa Crucis - Colesanti C., Kulh D., Napoleao T., Olim E., Rodrigues M.A., Treü R., Orion Observatory - Mairinque, Sao Paulo, Brazil
12 inch Schmidt-Cassegrain (305mm, f/10), focal reducer f/3.3, Sensor: SBIG ST-7XME, Mount: Paramount MX
15s exposures binned 1x1. Each data point is the average of 4 images. Weighted ensemble photometry with 1 comp star, apertures (4, 7, 11) More about Alfa Crucis: https://alfacrucis.org/
15s exposures binned 1x1. Each data point is the average of 4 images. Weighted ensemble photometry with 1 comp star, apertures (4, 7, 11) More about Alfa Crucis: https://alfacrucis.org/
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