Image Details
Caption: Fig. 4.
Differential 24 μm photometry from the MIPS observations. The mean of the ensemble stars has been set to zero, as marked by the dashed line. For the cataclysmic variable, the mean level of the 24 μm flux densities (for MIPS‐1, MIPS‐3, and MIPS‐4) has been set to zero after subtraction of the ensemble flux densities.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.