Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
BOXAVE | Box-average a 1 or 2 dimensional array. |
CONVOLVE | Convolution of an image with a Point Spread Function (PSF) |
CORREL_IMAGES | Compute the 2-D cross-correlation function of two images |
CORREL_OPTIMIZE | Find the optimal (x,y) pixel offset of image_B relative to image_A |
CORRMAT_ANALYZE | Find the optimal (x,y) offset to maximize correlation of 2 images |
CR_REJECT | General, iterative cosmic ray rejection using two or more input images. |
DIST_CIRCLE | Form a square array where each value is its distance to a given center. |
DIST_ELLIPSE | Create a mask array useful for elliptical aperture photemetry |
FILTER_IMAGE | Identical to MEDIAN or SMOOTH but handle edges and allow iterations. |
FREBIN | Shrink or expand the size of an array an arbitary amount using interpolation |
IMLIST | Display pixel values on an image surrounding a specified X,Y center. |
MAX_ENTROPY | Deconvolution of data by Maximum Entropy analysis, given the PSF |
MAX_LIKELIHOOD | Maximum likelihood deconvolution of an image or a spectrum. |
MEDARR | Compute the median at each pixel across a set of 2-d images |
POSITIVITY | Map an image uniquely and smoothly into all positive values. |
PSF_GAUSSIAN | Create a 1-d, 2-d, or 3-d Gaussian with specified FWHM, center |
RINTER | Cubic interpolation of an image at a set of reference points. |
SIGMA_FILTER | Replace pixels more than a specified pixels deviant from its neighbors |
EXTRAP | This procedure fills in the ends of a one-dimensional array from interior portions using polynomial extrapolation. |
XMEDSKY | Subtract sky from an image as a 1-D function of X |
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