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Question: Use of existing noise maps #1284
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@rainerschoedel The star finders in |
Thank you!
… On 9. Feb 2022, at 17:15 Uhr, Larry Bradley ***@***.***> wrote:
@rainerschoedel <https://github.com/rainerschoedel> The star finders in photutils have a threshold parameter, which defines the image value above which sources are detected. Typically, the threshold is defined relative to a background-only noise map, e.g., 3-sigma above the background. That will give you a threshold image, but most of the star finders require threshold to be a scalar float. So you will need to take a mean/median of your threshold image to get a threshold value. The find_peaks function (https://photutils.readthedocs.io/en/latest/api/photutils.detection.find_peaks.html#photutils.detection.find_peaks <https://photutils.readthedocs.io/en/latest/api/photutils.detection.find_peaks.html#photutils.detection.find_peaks>) is the only one where you can input a threshold image.
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I am currently learning photutils to benchmark it against StarFinder in Adaptive Optics images.
If I have already a noise map that provides me with the empirically estimated noise for each pixel of an image, is there an easy way to use it? Thanks.
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