SMARTS observations
of
V1647 Ori

ANDICAM photometry
ANDICAM optical photometry of V1647 Ori from 10 February 2004 through 2/20/06

Commentary

The photometry shown above is differential, with respect one star in the field (the others are known variables). True magnitudes are calibrated using that star (For details see Walter et al 2004 AJ 128, 1872).

The simultaneous JHK data will be plotted later.

V1647 Ori is no longer detected at BVR with this 1.3m telescope.