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[APML] M51 & M97
Hi,
Tony's M51 was an inspiration to all imagers to go deeper than usual to extract as much
info as possible in the image field. I was intrigued to see how deep I could go in my
moderately light polluted area near Worcester MA. Limiting magnitude is 4.9 - 5.0 at my
site in the area of M51 reducing to about 3rd mag 25 degrees above the horizon in the
south. Seeing was about 6 the night I took these images with transparency about 8. I took
the images just after Tony posted his luminance image I but it took me a long time to get
my M51 image to a half decent point and post today.
M51 and M97 are both (L)LRGB's with 90:24:24:30 minute respective total exposures using
10 minute individual exposures for the L frame in 1x1 bin mode and 5 minute individual
exposures in the RGB frames in 2x2 bin mode. The L and RGB's were combined in MAXIM
using average and bicubic resampling for each set.The luminance for M51 was also slightly
DDP'ed ( custom setting of 20) and 0.8 gamma stretched before importing into PS6for
further curve work. Both images were (L)LRGB' in Photoshop using the double layering
techniques that Rob Gendler prepared on his website with considerable lassoing,
feathering, curve adjustment and star shaping ( thanks Matt!) techniques used to enhance
local features.
M51 is almost a full field image using a Finger Lakes IMG6303E CCD (2K x 3K x 9 micron
pixels) camera on my 20" homemade F/4 Newt while M97 is a subframe.
I tried the "Mike Cook" technique on both images today to reduce the "fat" stars using the
radius at 1 and adjusting the fade to somepoint between 40% and 70% but noted it also
eroded finer detail in the spiral arms and eliminated faint stars. Bloated stars are one of my
biggest challenges in imaging and I was hoping for a silver bullet fix. Are these effects
expected or did I do something wrong in the execution?
You will note some astigmatic effects in the stars images on M51 from the cooldown
problems with the 20" pyrex Galaxy primary as it chased thermal equilibrium all through
that particular night.
The new images are at:
http://www.heavensgloryobservatory.com/Color_Jpegs/m51FRGB04-6303Eweb.jpg
and
http://www.heavensgloryobservatory.com/Color_Jpegs/m97FRGB01-6303Eweb.jpg
M97 shows additional faint galaxies through the nebula in addition to the 6 stars that form 2
distinct triangles.
I had considerable problems to remove the magenta from the HII regions in M51's arms.
Any ideas how to accentuate these with more "accurate" color?
Thanks, Brian Lula
Brian Lula
Polytec PI, Inc.
(508) 832-3456
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