VII) IMAGES = 1				!Make images? 0 = no; 1 = yes
	!---------------------------------------------------------------
	! If images and polarization maps are wanted, set IMAGES = 1.
	! When this option is enabled, HDUST will produce images for the
	! same set of observers as defined in the preceding section 
	! (VI.B).  Enter the number of images to be made, the 
	! size (field of view) of the image, and the resolution (number
	! of pixels).  Each image will be a square of the given size, 
	! projected on the plane of the sky and centered at the origin 
	! of the Cartesian coordinate system.
	!---------------------------------------------------------------
	N_images = 2			!number of images
	IMAGE SIZES:			!for each image, give its field of view
		R_1 = -1. Rstar		!(half size) in units of length 
							!If R_1 < 0, the code will set it to
							!   ABS(R_1)*Envelope Radius
		R_2 = -0.125 Rstar	!
	N_xy = 128				!image resolution (number of pixels)
	!---------------------------------------------------------------
	! Provide the wavelength binning for the images, using the same
	! scheme as described above in section (IV.A.2.c)
	!---------------------------------------------------------------
	N_bands = 1
	Bands = 'N BAND'

	A) IMAGE BANDS
	!---------------------------------------------------------------
	! Define the wavelength bands for the images, using the same
	! scheme as described above in section (IV.A.2.d)
	!---------------------------------------------------------------

        N BAND = CONTINUUM
        Nbins = 10
        Bin Spacing = 1
        Lower Lambda = 8.05 um
        Upper Lambda = 12.95 um

	B)  IMAGE FILE CONTENTS = 1			!0(short) or 1(full) = 1
		!-------------------------------------------------------------------
		! Choose between short output (*.maps: flux only) and full output 
		! (*.map: transmitted, scattered and emitted flux; Q, U and V stokes
		! parameters).
		!-------------------------------------------------------------------
