With a couple of clear nights in a row managed to collect data in HA and NII of the lower bit of the LMC. This was done with a near full Moon!
Exposures for both HA and NII were 10x8 minutes and 10x16 minutes.
I used these two exposure levels to make a HDR or tone mapped image of each from stretched stacks. This stops the bright bits blowing out but still shows the really dim stuff down to the noise.
This is an average of both HA and NII data and is what you would get with a 5nm or wider HA filter 4MB
http://d1355990.i49.quadrahosting.co...HA+NII_AV_.jpg
This is an inverted version 4MB
http://d1355990.i49.quadrahosting.co..._AV_INVERT.jpg
Here the the HA data is the red channel and NII the green 7MB
http://d1355990.i49.quadrahosting.co..._HAR_NIIG_.jpg
Here the NII data is the red channel and HA green
http://d1355990.i49.quadrahosting.co..._NIIR_HAG_.jpg
It is obvious that HA and NII have different distributions. It would be interesting to add OIII to the absent blue channel. NII could become the new SII for the Hubble palette where the SII signal is very faint and not extensive.
This system is very fast and once I master it even better deeper images will be captured.
System details.
Astrograph is an Officina Stellare RH200 which has a focal length of 600mm and is F3, yes F3! Clear aperture is 200mm.
FLI Atlas Focuser.
FLI ten position filter wheel CFW-3-10 with 50mm square filters.
Astrodon E series LRGB and HA, NII, SII and OIII 3nm NB filters. Also a continuum filter 5nm.
Camera is a FLI PL16803 which has a sensor size 36.8 X 36.8 mm.
The FoV of this system is 3.5 X 3.5 degrees.
Mount is a Software Bisque PMX.
Guidescope is a 100ED with a Lodestar.
Bert