Mewlon 300 CRS, ASI6200MM Pro By product of observing HAT-P-61b. More likely to be secondary minima according to the current epoch and period estimate.
Mewlon 300 CRS, ASI6200MM Pro Suspected eclipse, low SNR, but the timescale seems to be consistent with the observation done by https://var.astro.cz/en/Observations/34084. Could not determine if this is primary or secondary minima.
SCT 280 / 1870 (C11 with Starizona reducer) CCD: MII G2-1600 filter : Astrodon ExoPlanet-BB (V to IR) Exposure time of 240 s is achieved by combining two exposures of 120 s each
Mewlon 300 CRS, ASI6200MM Pro Potentially incorrect astrometry. The real EW star seems to be the one marked in my finder chart, not the one currently presented in the system. They are very close together so this might be the reason of the confusion?
Mewlon 300 CRS, ASI6200MM Pro Does not seems like a EW. Offset in lightcurve might be caused by inperfect flat. It is also where the meridian flip is. Overall the change of brightness is smaller than 1%, which seems inconsistent with the prediction.
