ANDICAM photometry of V1118 Ori from the before the current outburst through 06 May 2006

The photometry shown above is differential, with respect to a number of stars in the field. I have yet to calibrate the field. We have JHK data at the same times, but it is yet to be reduced.

SMARTS was closed 12/23-1/09, hence a lack of data during that interval.

The star has faded back to its pre-outburst magnitude, measured February-April 2004.

V1118 Ori is now behind the Sun.