BBC Sky at Night Magazine

SPIDER VANE

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FEBRUARY The robust design eliminates the need for constant collimatio­n, holding the secondary mirror steady in all positions. As one of the trickiest aspects of using fast Newtonians, we didn’t miss fiddling about with screwdrive­rs dangled over expensive mirrors in the dark.

we came out of these visual tests with high expectatio­ns for the telescope when used for astrophoto­graphy, and we were not disappoint­ed.

Using a DSLR and Bahtinov mask, we found focus to be sharp across the whole field. The corrector maintains good colour across the red, green and blue wavelength­s, meaning that when used with a DSLR or colour CCD, you won’t have the issue of bloated blue stars. In fact the images produced from the R200SS and Corrector PH in combinatio­n were very good indeed, with sharp, nicely shaped stars even at the edges of the frame.

Fast scopes have a tiny depth of focus, and therefore require precise focusing. The dual-speed rack and pinion focuser supplied, whilst not silky smooth, felt firm and dependable, and more than capable of allowing the miniscule movements necessary. As the outside temperatur­e dropped, the focus required tweaking, but that, remarkably for an f/3.8 Newtonian, was all the adjustment needed to achieve great quality images, even after several weeks of use.

Perhaps the ultimate compliment for a reflecting telescope would be that is as easy to use as a refractor. With the R200SS and Corrector PH combinatio­n, Vixen is very close indeed to that standard and has made it easier than ever to take high quality astro images in a short time.

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 ??  ?? Part of IC 1805 – a total of three hours and 20 minutes with a monochrome CCD
Part of IC 1805 – a total of three hours and 20 minutes with a monochrome CCD
 ??  ?? M45 – 45 minutes with a colour CCD
M45 – 45 minutes with a colour CCD

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