Star Mass / SNR graph in Imaging > Guider

[Tom Cowland]

What

As a User, it would be helpful to see the guiding software's Star Mass and/or Signal to Noise ratio graphs overlaid on top of the main guiding graph.

Why

When imaging without a sky quality meter, the Star Mass or Signal to Noise graph provided by guiding software such as PHD gives a useful indicator of incoming clouds during a long exposure. Knowing of incoming clouds can prevent wasted time on already ruined exposures and help guard against rain. NINA already displays guide drift and corrections in the Guider panel, adding these would avoid the need to switch back and forth between NINA and PHD to check on the other readings.