Infrared Camera

Crab Nebula We are in the process of developing an infrared camera that that is used on the Thirty Inch Telescope at the University of California at Berkeley Astronomy Department's Leuschner Observatory. This instrument is used as the central focus of a new course Astronomy 122 Infrared Astronomy. The camera is sensitive to light as long as 2.5 microns wavelength. This wavelength is long enough to make it easier to peer through the dust that fills our galaxy and to see stars that are have only recently (astronomically speaking) been born. The camera is funded by an Instructional Improvement Grant from the National Science Foundation and a generous gift from the Rockwell Corporation.

To the right is one of the first images from the Rockwell PICNIC array on the Thirty Inch telescope. It is a picture of of the Crab Nebula at H band (1.6 microns) taken by Melissa Enoch.

Description of Camera

Observing

Software

The camera control software consists of two parts: a server program running under Linux on the camera control computer and a client running on a UNIX or Win95 platform. The BAIT communication protocol is used.

Analyses of Performance


[ Leuschner Observatory | UGAstro ]

Last updated on 2000 November 21