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Re: ATM amateur infrared imaging?
- To: atm@shore.net
- Subject: Re: ATM amateur infrared imaging?
- From: Frank Henriquez <frank@ucla.edu>
- Date: Wed, 13 Jun 2001 13:31:54 -0700
- In-Reply-To: <E15AG0D-0001C0-00@aquarium.shore.net>
- References: <E15AG0D-0001C0-00@aquarium.shore.net>
- Reply-To: Frank Henriquez <frank@ucla.edu>
- Sender: owner-atm@shore.net
Stan,
IR imaging at 2 microns is probably out of the reach of all but the
most well-heeled and technically proficient "amateurs".
The NICMOS III IR array used in the 2MASS survey is around $50K. The
NICMOS array (and for that matter, all IR arrays) has to be
cryogenically cooled, typically with liquid nitrogen, or a closed
cycle cooler. While LN2 is very cheap, you'll need a cryostat with a
calcium floride, or other IR transparent window, a K or K' filter,
and a diffusion pump to get a good vacuum. The NICMOS array is
particularly sensitive to water, and we had to bake ours for up to a
day to drive all the water out of the array.
Next, you'll have to design the drive electronics and A/D conversion
circuits, and write the data acquisition software. Luckily, the
NICMOS III array is easy to drive (it's a CMOS device).
Assuming that you have an excellent machine shop and a diffusion pump
handy, you're looking at maybe $60K - $75K (or higher) so the dewar,
detector and electronics.
If you want to do near IR imaging, the easiest way to do it is with a
CCD camera and an I filter (from the UBVRI set) or a similar IR pass
filter.
I used this setup on a 24" telescope to make a color image of M42,
using the VRI filters. The results were impressive, since the I image
could see through much of the dust at the heart of M42, revealing the
rest of the cluster.
Frank
--
Frank Henriquez Programmer/Analyst Jules Stein Eye Institute, UCLA
frank@ucla.edu http://www.bol.ucla.edu/~frank/index.htm