MUSCAT: The Mexico-UK Sub-Millimetre Camera for AsTronomy
The Mexico-UK Sub-millimetre Camera for AsTronomy (MUSCAT) is a large-format, millimetre-wave camera consisting of 1,500 background-limited lumped-element kinetic inductance detectors (LEKIDs) scheduled for deployment on the Large Millimeter Telescope (Volc\'an Sierra Negra, Mexico) in 2018. MU...
Saved in:
Main Authors: | , , , , , , , , , , , , , , , , |
---|---|
Format: | Journal Article |
Language: | English |
Published: |
23-07-2018
|
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | The Mexico-UK Sub-millimetre Camera for AsTronomy (MUSCAT) is a large-format,
millimetre-wave camera consisting of 1,500 background-limited lumped-element
kinetic inductance detectors (LEKIDs) scheduled for deployment on the Large
Millimeter Telescope (Volc\'an Sierra Negra, Mexico) in 2018. MUSCAT is
designed for observing at 1.1 mm and will utilise the full 40' field of view of
the LMTs upgraded 50-m primary mirror. In its primary role, MUSCAT is designed
for high-resolution follow-up surveys of both galactic and extra-galactic
sub-mm sources identified by Herschel. MUSCAT is also designed to be a
technology demonstrator that will provide the first on-sky demonstrations of
novel design concepts such as horn-coupled LEKID arrays and closed continuous
cycle miniature dilution refrigeration.
Here we describe some of the key design elements of the MUSCAT instrument
such as the novel use of continuous sorption refrigerators and a miniature
dilutor for continuous 100-mK cooling of the focal plane, broadband optical
coupling to Aluminium LEKID arrays using waveguide chokes and anti-reflection
coating materials as well as with the general mechanical and optical design of
MUSCAT. We explain how MUSCAT is designed to be simple to upgrade and the
possibilities for changing the focal plane unit that allows MUSCAT to act as a
demonstrator for other novel technologies such as multi-chroic polarisation
sensitive pixels and on-chip spectrometry in the future. Finally, we will
report on the current status of MUSCAT's commissioning. |
---|---|
DOI: | 10.48550/arxiv.1807.08637 |