starutil.glevel = starutil.NONE
starutil.ilevel = starutil.CRITICAL
# Declare the script parameters. Their positions in this list define
# their expected position on the script command line. They can also be
# specified by keyword on the command line. No validation of default
# values or values supplied on the command line is performed until the
# parameter value is first accessed within the script, at which time the
# user is prompted for a value if necessary. The parameters "MSG_FILTER",
# "ILEVEL", "GLEVEL" and "LOGFILE" are added automatically by the ParSys
# constructor.
params = []
params.append(starutil.Par0S("CONFIG1", "The first config" ))
params.append(starutil.Par0S("CONFIG2", "The second config" ))
params.append(starutil.ParChoice("WAVEBAND", ("450","850"),
"The waveband to display - 450 or 850",
"850" ))
params.append(starutil.Par0L("DEFAULTS", "Include defaults for missing "
"values?", True, True ))
params.append(starutil.Par0S("TOOL", "The file comparison tool to use",
None, True ))
params.append(starutil.Par0S("PARAM", "A single config parameter to display",
None, True ))
# Initialise the parameters to hold any values supplied on the command
# line.
parsys = ParSys( params )
# Are we displaying a single parameter?
param = parsys["PARAM"].value
# parameter value is first accessed within the script, at which time the
# user is prompted for a value if necessary. The parameters "MSG_FILTER",
# "ILEVEL", "GLEVEL" and "LOGFILE" are added automatically by the ParSys
# constructor.
params = []
params.append(
starutil.ParNDG(
"IN", "The input NDFs",
starutil.get_task_par("DATA_ARRAY",
"GLOBAL",
default=Parameter.UNSET)))
params.append(
starutil.ParChoice("INSTRUMENT",
["SCUBA-2(450)", "SCUBA-2(850)", "ACSIS", "DAS"],
"The JCMT instrument", "SCUBA-2(850)"))
params.append(
starutil.Par0L("JSA", "Are the input NDFs on the JSA "
"all-sky pixel grid?",
True,
noprompt=True))
params.append(
starutil.Par0L("RETAIN",
"Retain temporary files?",
False,
noprompt=True))
# Initialise the parameters to hold any values supplied on the command
# "ILEVEL", "GLEVEL" and "LOGFILE" are added automatically by the ParSys
# constructor.
params = []
params.append(
starutil.ParNDG(
"IN", "Template POL2 time series NDFs",
starutil.get_task_par("DATA_ARRAY",
"GLOBAL",
default=Parameter.UNSET)))
params.append(starutil.Par0S("OUT", "Output simulated POL2 data"))
params.append(
starutil.Par0L("NEWART", "Create new artificial I, Q and U maps?"))
params.append(
starutil.ParChoice("ARTFORM", ("0", "1"),
"Form of artificial I, Q and U to create",
"0",
noprompt=True))
params.append(starutil.ParNDG("ARTI", "Artificial I map", maxsize=1))
params.append(starutil.ParNDG("ARTQ", "Artificial Q map", maxsize=1))
params.append(starutil.ParNDG("ARTU", "Artificial U map", maxsize=1))
params.append(
starutil.ParNDG("INCOM",
"Non-POL2 data files to define COM",
None,
noprompt=True))
params.append(
starutil.Par0F("COMVAL1",
"Constant sky emission (pW)",
0.0,
noprompt=True))
params.append(
"circular sky region",
None,
noprompt=True))
params.append(
starutil.Par0S("CENTRE2", "Latitude at centre of required "
"circular sky region"))
params.append(
starutil.Par0F(
"RADIUS", "Radius of the required "
"circular region on the sky (arc-mins)"))
params.append(
starutil.ParChoice("SYSTEM", ["ICRS", "GALACTIC"],
"System in which centre is defined",
"ICRS",
noprompt=True))
params.append(
starutil.Par0S("REGION", "An NDF or AST Region defining "
"the require region of the sky",
None,
noprompt=True))
params.append(
starutil.Par0F("PIXSIZE",
"Output pixel size (arcsec)",
None,
maxval=1000,
minval=0.01,
noprompt=True))