MODMAP MODMAP creates a map file (FITS image) from a model file by convolution with a Gaussian beam. The map file may be copied to FITS-format tape for transport to other institutions, passed into AIPS, or displayed using programs MAPPLOT and MAPDISP. Example: $ MODMAP MODFILE = "double.mod" MAPFILE = "test.map" LRTB = -10, 10, 10, -10 XYINT = 0.2 BEAM = 1.5 FREQ = 5000 SOURCE = "Double Model" DATE-OBS = "02/12/84" / $ Parameters: Parameter names (except DATE-OBS) may be abbreviated to uniqueness. End the list of parameters with a slash (/) or end-of-file (control-Z). MODFILE = "filename" : name of the input model file (must be specified). MAPFILE = "filename" : name for the output FITS-format map file (must be specified). BITPIX = n : specifies the BITPIX parameter for the FITS-format map file which controls whether pixels are stored as 16-bit or 32-bit integers. Possible values are 16 and 32; the default is 16. BITPIX=16 allows a "dynamic range" of about 32000:1. BITPIX=32 allows a much greater dynamic range but uses more disk space. LRTB = x1, x2, y1, y2 : specifies the location of the edges of the map in milliarcseconds relative to the origin (0,0) of the model. Note that x1 < x2, y1 > y2. XYINT = x : specifies the cellsize (sampling) of the map in milliarcsec. Choose XYINT to adequately sample the beam. The number of pixels in the output map will be (x2-x1)/xyint + 1 in the x direction and (y1-y2)/xyint + 1 in the y direction. ROTATE = angle : specifies an angle through which to rotate the model before creating the map. Use of this option is not MODMAP Page 2 recommended. BEAM = bmaj, bmin, bpa : specifies the parameters of the convolving Gaussian beam. bmaj and bmin are the FWHM of the major and minor axes, respectively, in mas, and bpa is the position angle on the sky of the major axis in degrees. If bmin and bpa are omitted, a circular beam of FWHM bmaj is used. FREQUENCY = f : specifies the observing frequency in MHz to be recorded in the FITS image header. SOURCE = "Name" : specifies an object name to be recorded in the FITS image header (FITS parameter "OBJECT"). NUMBER = n : if NUMBER is specified, only the first n model components will be used in calculating the map. TELESCOP = "text" : use this parameter to supply a value for the "TELESCOP" (name of telescope) parameter in the FITS image header. Any character string up to 16 characters can be used, but some FITS readers may truncate the string to 8 characters. For VLBI experiments, the usual convention is to use the one-letter abbreviations of the antennas, e.g., TELESCOP="BKGYO". (If you do not provide this parameter, no TELESCOP entry will be made in the FITS header.) DATE-OBS = "text" : use this parameter to supply a value for the "DATE-OBS" (date of observation) parameter in the FITS image header. The normal FITS convention for dates should be used (dd/mm/yy), e.g., DATE-OBS="21/04/86"; but MODMAP does not enforce this convention and allows you to supply any string of up to 16 characters. (If you do not provide this parameter, no DATE-OBS entry will be made in the FITS header.) Limitations: Maximum number of model components = 10000. Maximum number of map pixels = 262144 (e.g. 512x512, 1024x256). Only Gaussian and delta-function model components are allowed. Program History: Version 1.0: 1983 Aug 29 - new program (TJP). Version 1.1: 1984 Jan 20 - use new FITS routines; remove FORMAT="MODPLOT" option (TJP). Version 1.2: 1986 Oct 31 - add TELESCOP and DATE-OBS parameters (Tasso Tzioumis).