Image Details
Caption: Fig. 12.
Theoretical limits of sensitivity to brown dwarfs aged 1.0 Gyr through F1042M. All curves are as described in the legend to Fig. 11. At 1 Gyr, our search is no longer sensitive to 5 MJ brown dwarfs.
© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.