  Images of the exoplanets TOI 717.01, Qatar-8 b, and HAT-P-3 b were requested
in the w-filter from the Las Cumbres Observatory 0.4-meter telescopes. Of these
requests, images were taken of TOI 717.01 and HAT-P-3b and were reduced using
the EXOplanet Transit Interpretation Code (EXOTIC) software, as well as 6
photometric algorithms from the Our Solar Siblings pipeline. The transit
midpoint for HAT-P-3 b was found to be 2458907.6205, which is 20.2 minutes
different from its expected midpoint that night. For TOI 717.01, the transit
was not discernible, likely due to its low transit depth of 0.1%. It is
possible that one of the comparison stars in the TOI 717.01 field is variable.
