SMARTS observations
of
V1118 Ori

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

Commentary

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.