BLINC / MIRAC
MIRAC-BLINC(Unavailable): has two main modes of operation; imaging at 8 – 25um and nulling interferometry at 8 – 13um with BLINC being the cooled fore-optics for the MIRAC system. It uses the f/15 adaptive beam to give a FOV of 11.5″ and a pixel scale of 0.09″/pix. A R = 100 grism mode is also available. It is a PI Instrument, contact is Phil Hinz. For instructions on how to propose to use MIRAC-BLINC please see here.
|Detector||256 x 256||further info|
|Filters||18 filters in two filter wheels||further info|
|Grism||available in wheel 1||further info|
The Mid-Infrared Array Camera and Bracewell Infrared Nulling Cryostat (MIRAC-BLINC) is an instrument developed for use with the adaptive optics system on the 6.5 m MMT. It has two main modes of operation: imaging at 8-25 microns, and nulling interferometry at 8-13 microns.
A fourth version of MIRAC (MIRAC4) saw first light in late October 2006. The camera features a 256×256 array with high quantum efficiency and low dark current. The camera is cooled using a pulse tube mechanical cooler which eliminates the need for liquid helium cooling. BLINC is a liquid nitrogen-cooled set of fore-optics for the MIRAC system.
The entrance window provides the reflection surface for the visible light to be sent to the AO wavefront sensor. The Cassegrain focus is reimaged by an off-axis ellipse within BLINC which is capable of being rotated to send the light to either the nulling interferometer or the imaging channel. The imaging channel forms an image of the secondary on a reflective cold stop which baffles out warm radiation from the telescope. The mirror at the cold stop is mounted on a rotating voice coil actuator. This allows chopping at 1-10 Hz within the cryostat.
The nulling interferometer splits the entrance pupil in half and overlaps these two beams on a 50% transmissive beamsplitter. Manual alignment of the beams can be achieved with feedthrough actuators. Pathlength changes are introduced by translating the beamsplitter mount using a stepper motor with 42 microns of motion per revolution. Small pathlength changes can be introduced by a PZT-mounted mirror in the right arm of the interferometer. Both outputs of the interferometer are sent to a NICMOS3 detector within BLINC to allow sensing of phase variations in the interferometer. One of the outputs has a short pass dichroic which sends 8-13 micron light to MIRAC.
For further information please see the MIRAC-BLINC wiki.