Closed 18ganesha closed 1 year ago
Looking at the TESS light curve, we can see that the stellar flux varies by 0.2% and the flux decreases by 0.7% when the planet is in-transit. Using this information, we can calculate the size of a hotspot required to increase the flux by 0.2%.
Looking at the TESS light curve, we can see that the stellar flux varies by 0.2% and the flux decreases by 0.7% when the planet is in-transit. Using this information, we can calculate the size of a hotspot required to increase the flux by 0.2%.