Starlight Xpress MX-5C |
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This photo
shows the MX-5C attached to my LX 200 through the JMI NGF-S Motofocus.
The camera simply fits into the 2" eyepiece socket of the JMI.
This is the most straightforward installation and results in a focal/diameter
ratio of f10. So why the MX-5C and not some other imager??
Read my reasons below. Click
here to go back.
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Reason #1: Total Price and dollar per arcmin coverage. | |
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Price
was an obvious consideration. The table above summarizes the price
and key technical information as I understood them at the time I made my
purchase decision. The prices may be considerably different now.
The system price includes the LX 200, JMI Motofocus, the focal reducer and equatorial wedge. It also included any camera specific add-ons I would need to buy. For example the Pictor models uses the serial port for the camera to computer interface. To also interface the laptop to the LX 200, I needed to purchase a PCMCIA adapter to add a second serial port. The dollar per arcmin figures are based upon a f10 LX 200 with the f3.3 focal reducer. Arcmin calculations were based upon the diagonal of the CCD chip size. The Pictor 416XT is a good performer from both the Sys$ per arcmin and camera $/ per arcmin values. It did exceed my $5,000 target for the total system price, but not by too much. The two MX-5 Starlight Xpress cameras met my system price target and performed very well in both system $/arcmin and camera $/arcmin criteria. Leading me to conclude very good value for the dollar.
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Reason #2: The MX-5 series chips will cover over 98% of the objects I'll probably want to image. | |
Chart #1 |
Chart #2 |
Chart #3 |
Chart #4 |
These
charts summarize some size statistics for non-stellar objects brighter
than magnitude 14. There are about 4,000. Chart #1 shows
that 90% are galaxies or multiple galaxy systems. 6% are open clusters
and the rest are planetary nebula or globular clusters.
Chart #2 through #4 are histograms of the angular size of these objects. The "Bin" is the angular size in arc-minutes. The vertical bars are a count of the number of objects in that bin. For example, in Chart #2, 1,536 of the NSO objects counted have a angular size between 2 and 4 arc-min. And about 80% have a size less than or equal to 4 arc-min. 98% have a size less than or equal to 12 arc-min. At f3.3 the MX-5C has a diagonal field of view of about 33 arc-min. So it can easily image over 98% of the NSO brighter than magnitude 14. At f10, the MX-5C has a diagonal field of view of about 11 arc-min. Charts #3 and #4 show histograms for the size of planetary nebula and Globular clusters. These show that the MX-5C can image all planetary nebula and about 97% of the Globular clusters on LX 200 operating at f3.3. All in all I felt that this was pretty good performance. For those few objects I could not image in a single frame, I could always mosaic the images or put my Nikon film back on the camera. |
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Reason #3: I knew that Terry Platt was working on an autoguide add-on for the Starlight Xpress cameras, and figured he'd eventually get it working. This has become the STAR 2000. | |
Reason #4: I finally decided I wanted single shot color. | |