Giuseppe Marino, 23. 3. 2012 I discovered that the star TYC 3020-2195-1, usually adopted as reference for HAT-P-36, is a variable with amplitude 0.015 magn. and a period of 1h (probably a delta Scuti):
www of the light curves of the transit of HAT-P-36b present in ETD were obtained using that star.
Giuseppe Marino.
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Petri Kehusmaa, 5. 1. 2013 (www)
This observation is in error and can be removed. Correct data is re-imported. Petri Kehusmaa
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object HAT-P-36 b
I discovered that the star TYC 3020-2195-1, usually adopted as reference for HAT-P-36, is a variable with amplitude 0.015 magn. and a period of 1h (probably a delta Scuti): www of the light curves of the transit of HAT-P-36b present in ETD were obtained using that star. Giuseppe Marino.
page
No records
for this object on other pages
This observation is in error and can be removed. Correct data is re-imported. Petri Kehusmaa