CMASK/IRAC2 | ffield clnffield lthrshold,hthrshold [dispflag] |
create bad pixel mask from flat field | |
MASK/IRAC2 | inframe outframe |
replace bad pixels by neighbouring good ones | |
MKFLAT/IRAC2 | lamp_on lamp_off flat_field |
create a flat field | |
SSUBTR/IRAC2 | obj_frame sky_frame out_frame |
subtract a sky image from a science image | |
FFIELD/IRAC2 | obj_frame ff_frame out_frame |
flat field an image | |
ACUTS/IRAC2 | [image] [load] [plot] [upper] |
display an image with cuts setting | |
DCOMB/IRAC2 | [select] [seqname] [accsky] [align] output [trim] [tag] |
sky subtract and combine dithered images | |
FOCUS/IRAC2 | seqnum [focout] [create] |
determine best focus from a focus sequence | |
OBSLST/IRAC2 | [start] [end] |
lists a subsection of the IRAC2B OST | |
OBSREP/IRAC2 | start end |
print out a subsection of the IRAC2B OST | |
LAST/IRAC2 | [num] |
gives brief information on recent exposures | |
QL/IRAC2 | image1 image2 [outimage] |
subtracts one IRAC2 image from another | |
RCOMB/IRAC2 | select [align] output |
combine frames created with DCOMB/IRAC2 | |
SEEING/IRAC2 | determine the seeing |
Table J.2 contains a brief summary of the IRAC2 commands and parameters. All commands are initialized by enabling the IRAC2 context with the MIDAS command SET/CONTEXT IRAC2. The CCDRED context is also made available when the IRAC2 context is initialized. Consult Chapter 3for details of the CCDRED context.
=31 =3 =1999