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![]() ![]() The image to the left is an average of 8 x 20 second dark exposures. Note the gradient from top to bottom. The image on the right is 1 of 70 images exposed for 20 seconds. ![]() This image on the left is the flat field. It is an average of 40 x 70ms exposures. I take the flats in daylight inside a white room with no windows. The flat has had a dark frame subtracted that was an average of 8 x 70ms dark images. The image on the right is the image above right with the dark frame subtracted and the flat field divided. Note the grainy background noise. ![]() ![]() These images are from a set of 27 images with the object of interest moved slightly - this way we will get a larger field of view. Again the image on the right has been, dark framed and flat fielded. Note the grainy background. ![]() ![]() This image on the right is an average of 70 frames that have already been calibrated - note the field rotation. It appears all washed out - but there is detail in there. With a mild amount of curves and levels applied in photoshop the core of the cluster reveals its detail. ![]() ![]() Now with extra curves and levels in photoshop the fainter stars are visible but the core is burned out. The image on the right was the above right image and the left image layered in photoshop. The burned out core in the top layer was feathered and deleted to reveal the detail from the layer beneath. The dark areas were gaussian blurred and the bright areas unsharp masked. Now the images are 'stitched' together by carefully matching levels and curves and feathering the join. A final set of curves is applied to increase contrast. ![]() ![]() I then tried a new technique that I had read on one of the yahoo groups. I duplicated the layer and oversharpened until there were black halos round the stars, I then blended the layer using 'lighten'. The final image is sharp, contrasty, and fairly noise free. | ||