Hello everyone,
I have a question about FWHM measured values through sensors Vs actual FWHM values measured in subs
I’m currently evaluating sites & options regarding establishing a remote observatory - the route I decided on pursuing was to look into the market for established setup to buy to potentially save on used equipment & shipping costs…this approach has the advantage of testing said skies and setup prior to any commitments. The idea for me to go remote is to access better data - i love traveling with my telescope and dont intend on stopping but the main idea is for me to access sub 1.5” fwhm data on the regular. In the desert its mostly 2.5-3.5” however we get lucky sometimes with chile calibre nights (lowest i got was 1.1” average on edge 14 - so i got addicted to it 😅)
Upon testing few setups available on the market (one CDK 17” in HCRO, one RC 16 on another location in new mexico) sub FWHM values were sort of high for the expectations. In nights were sensors detect “1-1.5 fwhm, sub data goes as far as 2.5-3.5 (verfied that data is in focus with high altitude and good tracking) measured through SubframSelector on pix with inputting the correct resolution in bin 1×1
So I was wondering if this is normal or if there are other limiting factors within the setups I have experimented with. Would love to hear from people with telescopes in sites that publish FWHM readings through sensors such as HCRO or El sauce
Thanks,