Image Details
Caption: Fig. 1.
2MASS camera optics. Light enters through the ZnSe window at right. The Cassegrain focal plane lies 10 cm behind the window at a cryogenic field stop. A first lens is common to all three bands. Two dichroic mirrors immediately follow this common lens to split the light between the three bandpasses with the J‐band light reflected first and the Ks‐band light undeviated. Broadband filters near each Lyot stop primarily define the bands.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.