示例#1
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   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
示例#2
0
    #  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
示例#3
0
    #  "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(
示例#4
0
                       "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))