Celestial hemisphere:  Northern  ·  Constellation: Ursa Major (UMa)  ·  Contains:  M 101  ·  NGC 5447  ·  NGC 5449  ·  NGC 5450  ·  NGC 5451  ·  NGC 5453  ·  NGC 5455  ·  NGC 5457  ·  NGC 5461  ·  NGC 5462  ·  NGC 5471  ·  NGC 5477  ·  Pinwheel galaxy
M 101 B 1x1 1-hour unguided, Jason Fields
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M 101 B 1x1 1-hour unguided

M 101 B 1x1 1-hour unguided, Jason Fields
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M 101 B 1x1 1-hour unguided

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Description

This image shows what one can do with even a single long exposure.

This is a 1-hour (3600-sec) unguided image of M 101, to start to compare the effectiveness of different imaging strategies. The image has only had hot pixels and saturation blooms removed, no calibration applied. Obviously, histogram stretching has been applied. Seeing was a bit choppy and it appears the autofocuser did a reasonably job of keeping up with the 10°C temperature drop during the image; however, focus is soft and I may need to think more seriously about FocusLock.

There is a school of thought that says get above the read noise floor and coadd; this approach certainly has many benefits.

There is another school of thought that says "expose to the right", meaning, take a long exposure to get all the photons as one can and push the raw image histogram to the right. A key benefit here is getting the really faint extensions of an object (measured in tens of e-/hour) and the read noise penalty only once.

I tend to be a proponent of the former; however, there is the minor problem that any image processing method of combining (adding, subtracting, dividing, averaging, etc.) images introduces its own noise and uncertainty. Medians are nosier than means, but reject outliers better, etc. Noise always adds.

Also, this image is unguided; meaning, no guider inputs were provided to the mount. I ran the tip-tilt device at 1 Hz and every time I took at look at it, deflection was 1/5 of a pixel or less.

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M 101 B 1x1 1-hour unguided, Jason Fields