jase
05-02-2007, 05:48 PM
Well... it’s been sometime since I've submitted an image to the forum.
I've been spending most (if not all) of the nights fine tuning my mount, in particular periodic error (PE). My Titan out of the box had a peak-to-peak (+/-) 5.3 arcsec error in RA. Dec was around 1.5 arcsecs (not an issue). After running PEMPro for 7 worm cycles, analysing the data, building a curve and re-programming PEC, RA is now down to 1.8 arcsecs. A significant improvement to the original worm error. I originally thought that PEC and auto-guiding would work against each other. I was amazed at reduction in auto-guider corrections required after reprogramming the PEC data. I think I should be about to squeeze a little more performance out of the mount yet. Astronomical "seeing" where the observatory is located does not often get below 2 arcsecs, so for the time being the PE of 1.8 arcsecs suffice.
Some info on the attached image:
Exposure time: 80 minutes (Subs: 7 x 10min/ 2 x 5min)
Taken: 03/02/07 @ 23:30 (local) - 12:30 UTC
Optics: C11 @ ~F/5.5 (~1540mm F/L)
Mount: Losmandy Titan
Camera: STL11k :temp -20 :selfguided :bin 1x1 (1.2 arcsec per pixel)
Filters: None - Full wavelength spectrum including UV and IR
Processing: Calibration: master DF removal in MaximDL/CCD - no Flat removal. No further processing such as DDP or unsharp masks.
Notes: Battled with glare of the full moon so sky glow was relatively high. On reflection, a 2x2 bin (2.4 arcsecs per pixel) would have delivered a better image as seeing wasn’t steady. Imaging with a CCD with no filters is not desirable as they are sensitive to IR and UV noise. A narrow band filter would work better on this target but while still in the testing/fine tuning stages I didn’t bother. More 5 min subs would bring out improved detail around Eta and the gaseous cloud and globes. Stars at the edge of the field are elongated – the Lumicon GEG doesn’t handle the large format CCD very well.
Thanks for looking. :P
I've been spending most (if not all) of the nights fine tuning my mount, in particular periodic error (PE). My Titan out of the box had a peak-to-peak (+/-) 5.3 arcsec error in RA. Dec was around 1.5 arcsecs (not an issue). After running PEMPro for 7 worm cycles, analysing the data, building a curve and re-programming PEC, RA is now down to 1.8 arcsecs. A significant improvement to the original worm error. I originally thought that PEC and auto-guiding would work against each other. I was amazed at reduction in auto-guider corrections required after reprogramming the PEC data. I think I should be about to squeeze a little more performance out of the mount yet. Astronomical "seeing" where the observatory is located does not often get below 2 arcsecs, so for the time being the PE of 1.8 arcsecs suffice.
Some info on the attached image:
Exposure time: 80 minutes (Subs: 7 x 10min/ 2 x 5min)
Taken: 03/02/07 @ 23:30 (local) - 12:30 UTC
Optics: C11 @ ~F/5.5 (~1540mm F/L)
Mount: Losmandy Titan
Camera: STL11k :temp -20 :selfguided :bin 1x1 (1.2 arcsec per pixel)
Filters: None - Full wavelength spectrum including UV and IR
Processing: Calibration: master DF removal in MaximDL/CCD - no Flat removal. No further processing such as DDP or unsharp masks.
Notes: Battled with glare of the full moon so sky glow was relatively high. On reflection, a 2x2 bin (2.4 arcsecs per pixel) would have delivered a better image as seeing wasn’t steady. Imaging with a CCD with no filters is not desirable as they are sensitive to IR and UV noise. A narrow band filter would work better on this target but while still in the testing/fine tuning stages I didn’t bother. More 5 min subs would bring out improved detail around Eta and the gaseous cloud and globes. Stars at the edge of the field are elongated – the Lumicon GEG doesn’t handle the large format CCD very well.
Thanks for looking. :P