Hello folks,
until now, I did not really care about the offset settings of my ASI183MM camera. I just took the images setting exposure time and gain. Then, an almost unmentionable comment from amother user made me think of using the offset parameter as well. I did some research and found out, that the offset is basically used to shift the histogram of an image a little to the right (I know, it is not really the histogram that is shifted) to get smoother transistions in really dark areas of the image due to the statistical distribution of the measured values.
So far, so good. But here comes my question. Which values should be used for different situations. I guess, that narrowband images need higher offset values, because the light is so faint, that a lot of data is really close to the left of the histogram. Using color filters may need some smaller offsets (or maybe none?), because there is (usually) more light detected from the image sensor and therefore the histogram should tend to have more data in the lighter values. Am I right here?
I also realized, that NINA (which I use to take my images) offers a "Standard range" of 0-80 for the offset parameter. I guess, those values are especially for the ASI 183MM camera. I also guess, that the values are A/D-Units. Using offset values higher than 0 then must somewhat increase the number of blown out stars in the images. Do you realize that this is a problem for you?
It would be really great to hear, what you experienced astrophotographers think about using offset values and how you decide, which values are the "right" ones.
Thanks for your help…
CS
Christian
until now, I did not really care about the offset settings of my ASI183MM camera. I just took the images setting exposure time and gain. Then, an almost unmentionable comment from amother user made me think of using the offset parameter as well. I did some research and found out, that the offset is basically used to shift the histogram of an image a little to the right (I know, it is not really the histogram that is shifted) to get smoother transistions in really dark areas of the image due to the statistical distribution of the measured values.
So far, so good. But here comes my question. Which values should be used for different situations. I guess, that narrowband images need higher offset values, because the light is so faint, that a lot of data is really close to the left of the histogram. Using color filters may need some smaller offsets (or maybe none?), because there is (usually) more light detected from the image sensor and therefore the histogram should tend to have more data in the lighter values. Am I right here?
I also realized, that NINA (which I use to take my images) offers a "Standard range" of 0-80 for the offset parameter. I guess, those values are especially for the ASI 183MM camera. I also guess, that the values are A/D-Units. Using offset values higher than 0 then must somewhat increase the number of blown out stars in the images. Do you realize that this is a problem for you?
It would be really great to hear, what you experienced astrophotographers think about using offset values and how you decide, which values are the "right" ones.
Thanks for your help…
CS
Christian