% @(#)sky_roma.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:17:46 \se SECTION./ROMAFOT \es\co SKY/ROMAFOT 07-AUG-1989 RHW \oc\su SKY/ROMAFOT frame [sky_tab] [area] [nrx,nry] [min,max] determines intensity histogram and sky background in selected areas \us\pu Purpose: Determines intensity histogram and sky background in selected areas \up\sy Syntax: SKY/ROMAFOT frame [sky_tab] [area] [nrx,nry] [min,max] \ys\pa frame = input image frame \ap\pa sky_tab = name of the output table which will contain the values for the sky background; default is the frame name extended with the three characters `SKY'. \ap\pa area = area over which the background should be calculated. Input can given using the standard MIDAS notation. Default is the whole frame. \ap\pa nrx,nry = number of subdivisions in X and Y to create the grid of rectangular cells where the trial value of the sky background is determined. Default is 5,8 \ap\pa min,max = minimum and maximum between which a histogram of the frame pixel values is calculated (see Note) Default values are the cut values in the descriptor (LHCUTS(1) and LHCUTS(2)). If these values are identical the minimum and maximum in the frame are taken. \ap\no Note: First, a histogram of the pixel values between min and max is created, and the maximum in the histogram distribution is determined. A second window is then taken with a width of 10% of the min,max range and centered around the pixel value that corresponds with the peak in the histogram distribution. The background is determined taking all values into account that lie within this window.\\ The maximum number of cells is limited to 256. \on\exs Examples: \ex SKY/ROMAFOT GCLUSTER ? [100,300:400,500] ? 500,2000 Determine the sky background in 5 by 8 cells in the area enclosed by the pixels corners (100,300) and (400,500). The output table will be named GCLUSTERSKY. Only values between 500 and 2000 should be taken into account in determining the background level. \xe \sxe