RT CMa
Kiyota1998 - Kiyota1998V (Johnson V)
V observations were kindly sent to me by Seiichiro Kiyota. The model presented here has an arbitrary mass ratio as no radial velocity data exists. It is given only as one example of many possible solutions. The data were phased according to my measurement (using the Kwee & van Woerden method) of Kiyota’s (1998) best primary eclipse using the Kwee & van Woerden method. The time I obtained was 2450403.1920(4) and I used the period from Kiyota (1998) of 1.2937348(3) to phase the data. These phases are also the ones given in the online data file.