
Hi
- my name is Maurice Gavin [mgavin at ntlworld.com]
and
I’m a retired architect. My dual interests in photography
and astronomy goes back to my teens in 1947. In 1950 I joined
the BAA and made my first real telescope by rubbing together two 6-inch
glass disks in traditional ATM style. Much later 8-inch, 12-inch
and finally 17.5-inch Newtonian telescopes were built with purchased
optics and housed under a 10-ft dome. In 1980 I bought
a Celestron C-8 and this and a massive 9-inch f/4 Wray lens were mounted
on the big Newtonian.
I enjoyed taking photos and developing the results but by the late ‘80s
increasing light pollution rendering long exposure photography impossible.
In 1990 Astronomy Now invited me to review the SBIG ST-4 CCD camera.
I was hooked. Beyond their remarkable sensitivity, CCDs allow the images
to be viewed immediately which is great for those [like me] who like to
experiment with all manner of lenses and gadgets before the camera and
get instant feedback. Initially I used a SX colour CCD for
quick snaps but now use a Fuji
1400z and Minolta
D7 digital cameras for Internet uploads which is great fun.
In
1994 I succumbed to an automated 12-inch Meade LX200 SCT and built the
smaller Meade dome shown abutting the main observatory. My
productivity rocketed - working from the computer room between the two
domes. With my long-standing interest in spectroscopy CCDs are the
perfect detector - mostly SX MX9 and MX5c cameras.
First LRGB? In Nov 1996 whilst reviewing
SBIG 255+CFW, I hit on the idea of combining luminance + RGB to create
maybe the first LRGB image [M57 posted on the popular Compuserve Astroforum
at the time - shown adjacent] which I termed "a hybrid merge mono + RGB
image".
Astronomy is nothing unless you can discuss it with fellow amateurs. I belong to my local Ewell AS, UK CCD Users Group, Webb Society, SAGAS, The Astronomer [TA] and the British Astronomical Association [BAA] serving as president of the latter in 1996-7. I regularly contribute articles to Astronomy Now and Sky & Telescope - including May 2000 issue on the SBIG spectrometer. Summer 2000 the larger dome was cleared of telescopes and a new WPO spectrograph shown above for coupling to the SX CCD cameras was developed for the LX200. The larger dome was stripped for conversion to a workshop and the former 17.5-inch Newtonian was converted to a Big Dobsonian.
text & images copyright - Maurice Gavin 1996-2003