All I am quite experianced with Ha / OIII bi-color imaging and thats my normal thing as I dont typically have the time to capture three channels.
However, I recently got a 5nm Astrodon SII filter to complete my set as I fancied a go at SHO.
This is a comparision between my Ha and SII channels.
The HFR reading is comparable between the two channels at just a little over 2 pixels. However the SII stars seem much much brighter and more numerious.
I did wonder if this might be an effect of the strong Ha in the nebula partially blocking the stars? But I guess I am also a little worried that my SII channel is bloated for some reason....not that bloating explains the larger number of SII stars visible..
Ha
SII
I found this example from Sara Wager that seems to show a similar effect?
Cheers,
Adam