Hi Adam,I know you like to know things make sense in your understanding of PI processes and scripts, and go to lengths to do that in your video instruction. It is one of the reasons I really like, and beginning to understand what I am doing.
Now I am working to compare weights showing in NWeight Image Integration vs weights showing in Noise Evaluation Image Integration of my own 100 images of M101 color camera data. Data is from my very urban site with tons of varying light pollution over several nights of imaging.
I watched your Horizons NSG A Second Example video comparison video as a starting point, looking at the Process Console outputs.
Attached is an Excel file of the Process Console outputs and weights. I have cooled CMOS color camera data.
My problem is there are too many places to find weight data and I don't understand which data is comparable....
NSG Script data Integration:
1. FITS header keyword - NWeight of the NSG created files. One NWeight for all 3 channels.
2. Weight calculated is showing in the process console after Image Integration of the NSG images with no Normalization. All 3 channels have same weight for an image, and are different than NWeight. But why is there any weight because it should be using NWeight?
The above item 1 & 2 weights are different.
Non NSG integration of same data set (registered, not the NSG data).
1. Weight calculated is showing in the process console after Image Integration of the Non - NSG images with with Normalization. This is the same place you used in the example in your comparison video.
2. There are 3 channels of data, and the weight in each channels is different, as expected.
Can you explain how I can continue my comparison with so many different generated weights? I want to show NWeight is better than noise evaluation.
Why would one NWeight be used for all 3 channels.
The data leads me around in circles without logical conclusion, especially after watching your using it in your Horizons NSG Second Example.
At the bottom of each Process Console listing you can see the Image Integration settings.
Thanks for your advice and review.
Roger
Comments
The NWEIGHT is calculated from channel 0. Hence, for a color image, the weight is entirely based on the red channel. As far as I am aware, ImageIntegration is only able to use a single weight per image. I had to choose between using a single channel, or devise some strategy to combine them. I chose the red channel partly for convenience (same code for both mono and color), and partly because red is a particularly important color in astrophotography. Since the weights are relative, it does not really matter which color has the most noise. The choice only really matters if the color noise varies from one color to another in a non linear way."
NSG v1.1 fixed a problem with the NWEIGHT calculation. The noise ratio
needed to be squared. Alas, it would therefore not be reliable to use results
obtained from pre NSG v1.1 to find relationships between NWEIGHT and subframe
selector parameters.
Trying to find relationships between NWEIGHT and subframe selector
parameters is going to be fraught with difficulties because the subframe
parameters are affected by too many variables.
Using subframe selector parameters to determine image weights can be
tricky. For example, the number of detected stars depends not just on transmission
and light pollution, but also on how sharp the star profiles are - due to
seeing, guiding and focus shift. The median level tells you nothing about transmission (how much of the useful signal was absorbed by the atmosphere / clouds).
NWEIGHT should depend on the transmission (how many useful photons
reached your sensor) and how much noise was introduced by light pollution / sky
glow / the sensor. It is a relative measurement, only relevant to files from
the same NSG run. It also depends on the PixInsights MRS noise calculation which, if used correctly, I believe to be quite good, although it is unlikely to be perfect.