Meade ACF 16", Moravian G4-9000, clear and RGB filters
Data reduction and analysis were performed using the HOPS software.

Further observations and analysis are required to confirm the nature of the system and to verify the planetary candidate.

Meade ACF 16", Moravian G4-9000, clear and RGB filters
Data reduction and analysis were performed using the HOPS software.

The resulting light curve differs significantly from what is expected for a typical exoplanet transit. In particular, the shape of the signal appears more consistent with that of an eclipsing binary star rather than a planetary transit.

Further observations and analysis are therefore required to confirm the nature of the system and to verify the planetary candidate.

Meade ACF 16", Moravian G4-9000, clear and RGB filters
Data reduction and analysis were performed using the HOPS software.

Further observations and analysis are required to confirm the nature of the system and to verify the planetary candidate.

Meade 16" + ZWO ASI2600MM Pro
Candidate exoplanet

Meade 16" + ZWO ASI2600MM Pro
Candidate exoplanet

400mm f6.8 ODK, ST10XME, J/C Filters
240 second exposure unfiltered. GPS time control, analysis and detrend in AIJ. Transit appears to have started much earlier than ephemeris, ingress missed. Transit is also much deep er than expected from ephemeris. Limited comps available.

400mm f6.8 ODK, ST10XME, J/C Filters
240 second exposure unfiltered. GPS time control, analysis and detrend in AIJ. Transit appears to have started much earlier than ephemeris, ingress missed. Transit is also much deep er than expected from ephemeris. Limited comps available.

Meade 16" + ZWO ASI2600MM Pro
TESS candidate exoplanet

Meade 16" + ZWO ASI2600MM Pro
TESS candidate exoplanet