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by Jon Talbot
In August 2007, I was loaned a Stellarvue SV102ED by the company owner, Vic Maris, in order to evaluate the astrophotographic qualities of this doublet refractor. The version I received (the SV102ED2) had the optional 2inch
Feather Touch focuser.
I had used several Stellarvue telescopes in the past, including an SV78S (Nighthawk achromat), SV 80S, and 90T (both triplet apochromats) and obtained superior results from the triplets, so I was interested in how this 4inch ED
doublet would work. Being a doublet with an ED element, I was curious about how well it would correct for chromatic aberration, inherent to some degree in most doublets. I have not imaged through any ED refractors from other
manufacturers so this is not a comparison as to how this scope compares to other 4inch doublet refractors on the market.
The scope arrived in pristine condition and the first thing I noticed about it was how light it was. I was expecting it to be much heavier. I mounted it on my Mountain Instruments MI250 and piggy backed my older Stellarvue SV78S
on top to act as a guide scope. I also attached a RoboFocus stepper motor to the Feather Touch in order to do automatic focusing.
The cameras I used to evaluate the scope were a Starlight Xpress SXVH9, a small chip (11.2mm diagonal with 6.45micron pixels) CCD camera and the much larger chip SBIG STL11000 (43.7mm diagonal with 9 micron pixels).
Using the SXVH9
I used CCD Inspector software and the SXVH9 to measure the field curvature without focal reducer or field flattener to be 9%. Stars were only slightly elongated in the extreme corners.
The images shown on the next page are enlarged crops from the corners of images of M13 and M27, both showpiece objects in the summer sky.
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