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Imaging with the Madawaska Highlands Obs.


THE MHO: AN IMAGING SUPERSTAR

The Madawaska Highlands Observatory is a Canadian effort. The focus is on designing and building a state-of-the-art imaging platform. All of our efforts have gone into optimizing every aspect of the imaging equation. This includes choosing the best southerly site in Canada, one with an exceptionably dark sky and good seeing, on the highest possible elevation.

An state-of-the-art dome design is used to optimize the local seeing. The dome constructed of carbon fibre sandwich core is ultra light but very strong and rigid. It is elevated 3 metres above ground level to minimize ground turbulence. The dome shape is a 3/4 sphere to optimize air flow and the slit is a top roll-over to lessen the air drag on the dome.

The telescope uses several innovative designs and advanced materials to produce the best possible image quality. This includes the use of an open back cellular mirror. This topology produces a very low mass mirror that can be vented from the back. This will ensure that the mirror has the best possible local seeing for minimizing the boundary layer above the optical surface. The key is to maintain the mirror at ambient temperature. The optical tube assembly (OTA) is made of carbon fibre sandwich core (CFSC) a material that is lighter aluminum yet very rigid. In addition the CFSC has exceptionally low thermal coefficient similar to that of the Borofloat mirror. Extensive baffling is used throughout the optical design to maximize contrast.

The camera uses the largest monolithic CCD in the world with over 110 million pixels. The chip is almost 4" across and has exceptional specifications, such as very high quantum efficiency, high transfer rate, negligible dark noise, low read noise, etc.

The amazingly large 5 degree² field of view is fully corrected with triplet lens. The u', g', r', i', z' and Hα filters will be used because they have a high bandpass and for standardization.

To top off the list of highlights is the use of active optics. With a fixed primary, the device moves the prime focus imaging train and is able to continuously achieve accurate collimation throughout the entire sky. The hexapod is able to tip/tilt, move laterally, rotate and focus. It has repeatable accuracy of 1 micron with an X,Y range of some +/-2" and Z range of +/-1"!

The telescope uses a high performance one tyne equatorial fork mount that employs 40" friction drive wheels in both RA and DEC. This will yield exceptional pointing accuracy and high precision tracking.

The Madawaska Highlands Observatory is slated to produce some truly spectacular imaging that will surely rival images produced by even the Polamar 48" Schmidt camera. Quite possibly it will be the best imaging telescope in the world open to nonprofessionals.

For example the Madawaska Highlands Observatory could do a tricolor image of the Andromeda galaxy, M31 to the 25th magnitude in about 3 hours! M31 is some 4 degrees wide so two images of M31 are required yielding a field of 4.4º x 2.22º. Since the dark noise is negligible no dark frames are required.

KEY IMAGING SPECIFICATIONS

  • 5 deg² Field of View.
  • 1.0" FWHM expected seeing.
  • 10580 x 10560 pixels image size.
  • 0.76"/pixel image scale.
  • 80,000 e- full well depth.
  • 370-1000 nm useful spectral range
  • u', g', r', i', z' + L +wL filters.
  • 4u/6u centre/edge spot 80% 4-lens fully corrected image
  • 16 seconds full image download @1 MHz
  • 1.6 seconds download @10 MHz
  • 4 e- read noise @1 MHz
  • 18e- read noise @10 MHz
  • 94% quantum efficiency
  • 16-bit Quantization
  • Back illuminated thinned UV enhanced coatings
  • -100ºC Cryo-Tiger Cooling
  • 1e-/pix/hr dark noise
  • 21.82 mag/arcsec2 sky brightness
  • One arm fork equatorial mount with zenith tracking
  • 25th magnitude stars in 2000 seconds, s/n=3, r'


Next: 5 degrees² FOV



2010 - The Madawaska Highlands Observatory, Ottawa, Canada.