Three calibrator fields have been found to contain secondary standards that are eclipsing binaries. These stars were not rejected because of high dispersions since they mostly remain at a constant magnitude with occasional jumps during eclipses. Light curves for the two stars follow. Included are sequential scan plots (magnitude vs # in scan sequence), light curves (magnitude vs. Julian Day), and for one, the phased time plot (magnitude vs. Julian Day modulo the variable period).
J ~ 11.27; J-K ~ 0.3; delta J ~ 0.2
J ~ 13.58; J-K ~ 0.53; delta J ~ 0.3
J ~ 12.43; J-K ~ 2.6; delta J ~ 0.7
RA, Dec (J2000): 246.86061 -24.43157
J ~ 13.00; J-K ~ 1.15; delta J ~ 0.2