Repatch (from linux) of OSX IRAF

1 files changed, 64 insertions, 0 deletions

diff --git a/noao/imred/src/doslit/doslit.cl b/noao/imred/src/doslit/doslit.cl
new file mode 100644
index 00000000..56458435
--- /dev/null
+++ b/noao/imred/src/doslit/doslit.cl
@@ -0,0 +1,64 @@
+# DOSLIT -- Process slit spectra from 2D to wavelength calibrated 1D.
+#
+# The task SPROC does all of the interactive work and SBATCH does the
+# background work.  This procedure is organized this way to minimize the
+# dictionary space when the background task is submitted.
+
+procedure doslit (objects)
+
+string	objects = ""		{prompt="List of object spectra"}
+
+string	arcs = ""		{prompt="List of arc spectra"}
+file	arctable		{prompt="Arc assignment table (optional)"}
+string	standards = ""		{prompt="List of standard star spectra\n"}
+
+string	readnoise = "rdnoise"	{prompt="Read out noise sigma (photons)"}
+string	gain = "gain"		{prompt="Photon gain (photons/data number)"}
+real	datamax = INDEF		{prompt="Max data value / cosmic ray threshold"}
+real	width = 5.		{prompt="Width of profiles (pixels)"}
+string	crval = "INDEF"		{prompt="Approximate wavelength"}
+string	cdelt = "INDEF"		{prompt="Approximate dispersion\n"}
+
+bool	dispcor = yes		{prompt="Dispersion correct spectra?"}
+bool	extcor = no		{prompt="Extinction correct spectra?"}
+bool	fluxcal = no		{prompt="Flux calibrate spectra?"}
+bool	resize = no		{prompt="Automatically resize apertures?"}
+bool	clean = no		{prompt="Detect and replace bad pixels?"}
+bool	splot = no		{prompt="Plot the final spectrum?"}
+bool	redo = no		{prompt="Redo operations if previously done?"}
+bool	update = no		{prompt="Update spectra if cal data changes?"}
+bool	quicklook = no		{prompt="Minimally interactive quick-look?"}
+bool	batch = no		{prompt="Extract objects in batch?"}
+bool	listonly = no		{prompt="List steps but don't process?\n"}
+
+pset	sparams = ""		{prompt="Algorithm parameters"}
+
+begin
+	file	obj, arc, std
+
+	# Expand image lists
+	obj = mktemp ("tmp$iraf") 
+	arc = mktemp ("tmp$iraf")
+	std = mktemp ("tmp$iraf")
+	sgetspec (objects, arcs, arctable, standards, obj, arc, std)
+
+	apslitproc.readnoise = readnoise
+	apslitproc.gain = gain
+	apslitproc.width = width
+	apslitproc.t_width = width
+	apslitproc.radius = width
+	apslitproc.clean = clean
+	sproc.datamax = datamax
+
+	sproc (obj, arc, arctable, std, crval, cdelt, dispcor, extcor, fluxcal,
+	    resize, clean, splot, redo, update, quicklook, batch, listonly)
+	delete (std, verify=no)
+
+	if (sproc.dobatch) {
+	    print ("-- Do remaining spectra as a batch job --")
+	    print ("sbatch&batch") | cl
+	} else {
+	    delete (obj, verify=no)
+	    delete (arc, verify=no)
+	}
+end