Shiraz
31-05-2013, 03:15 PM
The Baader RCC1 is designed to correct coma on fast Newts. I fitted one to an imaging system based on an f4 Newtonian (currently 200mm, but will later upgrade to a 250mm). The chip is an icx694 with 6M small pixels and a field of view of 0.89 x 0.72 degrees in the current system.
The RCC1 has a required back focus of 91.5mm, which allows a lot of ancillary gear such as filter wheels, OAG etc. to be inserted. It does not do this by any optics magic though - it relies on you to set the focal plane to be a long way out, so that the RCC1 can be set back closer to the mirror than other CCs. Since the RCC1 is 75mm long, this means that the focal plane needs to be more than about 166.5mm from the OTA surface or the RCC1 will intrude into the input light column. On my GSO Newtonian, this required cutting 55mm from the OTA tube to move the mirror up and the focal plane out. I also cut down the focuser to minimise its height and fitted a 70mm secondary to allow for the larger light cone intercept. With these mods, the centre of the field of view is fully illuminated (just). Vignetting sets in at small angles off axis (from light missing the secondary and from the smallish input aperture of the RCC1). However, the centre of the fofv is of primary interest for galaxy imaging and the vignetting is not excessive over the fairly narrow field of view of the icx694. The system is usable with APSc (tried it with a QHY8), but anything larger and vignetting would be a big problem.
The system is laser collimated through the RCC1 – it needs to be right, but it is not too difficult to get it aligned. The attached composite is from a typical short sub with stretched small crops at native resolution taken from the field centre and the four corners. There is perceptible distortion in one corner at the 1.17 arc sec sampling, but I expect that to be fixed when the camera image plane alignment is tweaked up a little bit better. The additional segment shows the lower right corner without the RCC1 – it made a huge difference.
There is no noticeable decrease in central resolution with the RCC1 in place, so the corrector is not introducing excess aberration of any sort – in good seeing, the FWHM has occasionally been well under 2 arcsec. Coatings look to have very low reflection and I have not noticed any artefacts from bright stars.
All-in-all, this appears to be an excellent CC for a fast Newtonian, particularly if used with a relatively small chip for high resolution imaging.
thanks for reading. Regards Ray
The RCC1 has a required back focus of 91.5mm, which allows a lot of ancillary gear such as filter wheels, OAG etc. to be inserted. It does not do this by any optics magic though - it relies on you to set the focal plane to be a long way out, so that the RCC1 can be set back closer to the mirror than other CCs. Since the RCC1 is 75mm long, this means that the focal plane needs to be more than about 166.5mm from the OTA surface or the RCC1 will intrude into the input light column. On my GSO Newtonian, this required cutting 55mm from the OTA tube to move the mirror up and the focal plane out. I also cut down the focuser to minimise its height and fitted a 70mm secondary to allow for the larger light cone intercept. With these mods, the centre of the field of view is fully illuminated (just). Vignetting sets in at small angles off axis (from light missing the secondary and from the smallish input aperture of the RCC1). However, the centre of the fofv is of primary interest for galaxy imaging and the vignetting is not excessive over the fairly narrow field of view of the icx694. The system is usable with APSc (tried it with a QHY8), but anything larger and vignetting would be a big problem.
The system is laser collimated through the RCC1 – it needs to be right, but it is not too difficult to get it aligned. The attached composite is from a typical short sub with stretched small crops at native resolution taken from the field centre and the four corners. There is perceptible distortion in one corner at the 1.17 arc sec sampling, but I expect that to be fixed when the camera image plane alignment is tweaked up a little bit better. The additional segment shows the lower right corner without the RCC1 – it made a huge difference.
There is no noticeable decrease in central resolution with the RCC1 in place, so the corrector is not introducing excess aberration of any sort – in good seeing, the FWHM has occasionally been well under 2 arcsec. Coatings look to have very low reflection and I have not noticed any artefacts from bright stars.
All-in-all, this appears to be an excellent CC for a fast Newtonian, particularly if used with a relatively small chip for high resolution imaging.
thanks for reading. Regards Ray