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Re: A Comment on the Lenses (part 2)
One place to test this would be at the image end of the lens. Here the
opening diameter is a little over 2" so anything larger than a 2" diameter
filter would do the job. This would save tearing up a camera, but would
add two more surfaces to the optical path. There is room for something up
to 1/2" thick here.
Tom Droege
At 10:07 AM 11/5/02 -0700, you wrote:
>As I said, the test would "perhaps be simpler". It depends
>on how much trouble it would be to replace the camera window.
>That is in your regime, but since you bought a stock Omega
>filter, the Custom Scientific filter may be similar enough
>in size and thickness to almost be a drop-in replacement.
>This is a test that only needs to be done on one camera just
>to see if the long-wavelength tail is the problem. Adding
>internal stops in a camera lens would appear to me to be
>just as time-consuming!
> As for adding something to remove the long-wavelength response:
>this would be another piece of glass, and I doubt you have room
>in the current camera to do this. You can have someone coat the
>current filter with an interference coating, but that might be
>more expensive/difficult than just buying someone else's stock filter.
> Tom, I'm not trying to make things difficult for you! You had
>a problem and were looking for solutions. Changing the filter is
>a viable experiment that you may or may not decide to do. A theoretical
>test would be to run a ray-trace using the real bandpass of the
>filter/CCD combination and see if it shows significant image
>aberration compared with a true Ic bandpass. A person running
>something like Zemax could also check to see what effect stopping
>down the lens would have or where to put an internal baffle.
>Arne
>
>Tom Droege wrote:
>>Those not familiar with the design should know that the filter is used as
>>the camera window. Part of the camera body, the camera window, and the
>>shutter are all one unit. Changing the filter means building a new
>>camera. You all should remember that I give these things away, so I have
>>tried to keep the cost down in every way possible.
>>Is it possible to just add something to just cut off the tail of the IR
>>response? Is this even desirable?
>>Having learned a little, my present interest (for the systems that I run)
>>is to just take specific fields night after night attempting to cover the
>>whole sky. I can now see that this has absolute photometry problems. At
>>my location I could probably not solve these even if I tried. It does
>>appear that I can do field specific relative photometry with considerably
>>better precision. This will detect variable stars in two simultaneous
>>filter. We may never be able to get good calibration on the either the V
>>or the V-I photometry. Sigh! That may be life in Batavia. I am hoping
>>that a large catalog of such measurements will still be useful.
>>Tom Droege
>>At 09:07 AM 11/5/02 -0700, you wrote:
>>
>>>One option would be to order an interference Ic from Custom
>>>Scientific, and try that on your I-band camera. This has the
>>>proper bandpass and would not have any out-of-band transmission.
>>>I am not sure how well such a filter will work in an f/4 beam,
>>>but you can ask David Marcus (owner).
>>> This test would perhaps be simpler than experimenting with
>>>internal aperture/pupil stops.
>>>Arne
>>>
>>>Tom Droege wrote:
>>>
>>>>The filters are "Bessell I" from Omega Optical. I assume they are
>>>>"stock" since there were no special instructions on the order. This is
>>>>something that Michael Richmond selected after talking with the expert
>>>>at Omega Optical.
>>>>Tom Droege
>>
>