HAWC
| Name of Instrument: |
HAWC - High-resolution Airborne Wideband Camera |
| Instrument type: |
Far Infrared Bolometer Camera
50-240 microns |
| Principal Investigator: |
Dr. AlHarper |
| Contact: |
Jesse Wirth: wirth@oddjob.uchicago.edu |
| Institute: |
University of Chicago
Yerkes Observatory
373 West Geneva Street
Williams Bay, Wisconsin 53191 |
| Instrument Team Page: |
http://astro.uchicago.edu/hawc/ |
Scientific and Technical Abstract:
HAWC (High-resolution Airborne Wideband Camera)
is a far-infrared camera designed to cover the 40-300 µm spectral
range at the highest possible angular resolution. Its purpose is
to provide a sensitive, versatile, and reliable facility imaging
capability for SOFIA's user community during its first operational
years.
HAWC will utilize a 12x32 pixel array of bolometer
detectors constructed using the silicon pop-up detector (SPUD)
technology developed at Goddard Space Flight Center. The array
will be cooled by an adiabatic demagnetization refrigerator and
operated at a temperature of 0.2 K.
Many infrared sources are dusty. Absorption of starlight
typically heats the dust grains to temperatures of tens or hundreds
of degrees Kelvin where they radiate most of their energy in the
far infrared, at wavelengths of 40-300 µm which are inaccessible
from the ground. Imagery in this spectral range with the highest
possible spatial resolution is the natural starting point from
which to develop an understanding of source energetics and morphology.
It is also a key to understanding the physics and chemistry of
the interstellar medium.
HAWC Performance Summary Instrument
sensitivity and resolution summary is provided to permit estimating
feasibility of scientific investigations.

All sensitivity and resolution data are preliminary,
and based on anticipated performance of the observatory and the
instrument. Actual performance of the SOFIA telescope and
instrument combination will be established after flight operations
begin. Telescope performance is expected to be upgraded during
the first two years, and instrument performance may be upgraded,
or additional modes or capabilities may be added.
Performance estimates given here are based on data
supplied by the instrument team. Further details and updates may
be obtained from the instrument team via the contact information
given above.
Exposure Time Calculator Link
to SOFIA Instrument Time Estimator (SITE)
Further References:
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