To start EFS, you can either launch it from a script or from the IDL prompt. If you launch it from a script, from the shell prompt, type run_efs to run the normal EFS, connected to a server. To run EFS with a simulated server, type run_efs -s.
To run EFS from the IDL prompt, first you have to set the device to
handle 24 bit colors. Do this by typing device,
true_color=24 at the IDL prompt. If running it connected to the
server, first you have to compile the KIDL routines. Do this by typing
.r kidl at the prompt. Then type in nirspec_efs,
sim="nirspec" to start the EFS. To run EFS with a simulated server,
it is not necessary to compile the KIDL routines. Start the EFS by typing
nirspec_efs, sim="nirspecsim".
This
window displays the simulated echellogram for the given setup. The box
is called a Set-Up Box. It defines approximately the limits of the detector.
By using the box, you can tell which parts of the echellogram will fall
on the detector, and which parts will be chopped off. By clicking and dragging
the mouse in the window, you can move the box around, which automatically
changes the Echelle and Cross Disperser angles correspondingly. In this
way, mechanisms in NIRSPEC will be moved so that the matching parts of
the echellogram fall on the detector.
These boxes display the X (horizontal) and Y (vertical) pixel of the
detector the cursor is currently on. Pixels begin with (1,1) in the lower
left corner of the Set-Up Box.
This box gives the wavelength in the echellogram that the cursor is
currently on.
Menu Options
This section describes the routines and functions that can be called
by clicking on an option the main menu bar, above the draw window. The
menu bar is divided into four main sections, File,
Telescope, Overlays,
and Help.
This option opens a script to be edited or executed by the EFS. It uses a dialog box that allows the changing of directories, filters, and filenames directly by typing it into the box, or by clicking on the appropriate filename or directory in the scroll window. This same dialog is used for opening files throughout EFS, including saving files as well.
Use this option to save the current settings of the EFS to a file. Every settings, such as filter, echelle and cross dispersor angles, and integration time are saved into a script file, that can be opened at a later time for editing or execution.
This option removes any lines plotted on the echellogram.
Hit this button to open a previously written line list.
Enter the wavelength for the new line here.
Hit this button to add the line to the list.
Enter a comment for the new line here.
To plot the lines redshifted by a specific Z, enter the Z here.
Hit this button to remove the currently selected line from the list.
Hit this button to completely clear the list.
Hit this button to switch between the various color systems. RGB is
the default.
Red / Green / Blue
Slide the sliders to the various positions until the desired color is obtained.
OK
Enter the filename you wish to save the list as.
Hit this button to save the list. It brings up a dialog to browse for a file to save to .
Hit this button to plot the lines in the list and close the dialog.
Hit this button to plot the lines in the list, but leave the dialog open.
Hitting this option plots the OH lines on the echellogram. Hitting it again removes them.
Hitting this option plots the Neon lines on the echellogram. Hitting it again removes them.
Hitting this option plots the Argon lines on the echellogram. Hitting it again removes them.
Hitting this option plots the Krypton lines on the echellogram. Hitting it again removes them.
This help dialog shows the various Hotkeys used by the EFS. Hit OK to dismiss the dialog.
This menu selects the type of calibration mode to use. First option,
Setup Only, only moves the mechanisms in the instrument, but does not take
an exposure. The second option, Object Only, allows the exposure of an
object by the camera. Multiple setups are supported by use of the setup
boxes. The Object+Lamps option is the same as the Object Only mode, except
that at the end of the script, the use of arc lamps for calibration is
included. The fourth option, Object+Star is and option that will take two
exposures. The first is of the object. Then, you are prompted to move the
telescope to the calibration star, and the star exposure begins. The Full
Sequence is a Object+Star+Lamps sequence.
This menu selects the nod pattern to be used. A Stare is no nodding,
a Nod two through four splits the slit makes two through fours nods in
the slit. A Nod Chop makes a nod in the amount specified by the Set Nod
Parameters option in the Telescope section of the main menu.
This menu selects the number of nods to perform.
This menu selects the spectral mode between High Resolution, Low Resolution,
and Imaging. Consult the NIRSPEC manual for more about the spectral modes.
Change this dropdown menu to select the size of the slit to be used
for the current setup.
Select the filter to be used for the current setup from this list.
Select the type of blocking to be used from None, Thin, or Thick.
Hit this button to see a transmission plot of the currently selected
filter.
Switch this toggle to turn on and off the overplotting of a bad pixel
mask over the detector box. This is useful in determining which part of
the echellogram may be affected by bad pixels.
This box displays the current echelle angle. It can be changed either
by moving the box, or by entering a value into this field.
This box displays the current cross dispersor angle. It can be changed
either by moving the box, or by entering a value into this field.
Hit this button to create a new setup box.
Hit this button to go to the previous setup box.
Hit this button to go to the next setup box.
Hit this button to delete the currently selected setup box.
Enter the integration time of the object exposure in this box. It is disabled for Setup Only mode.
Enter the integration time of the calibration star exposure in this box. It is enabled for Object+Star and Full Sequence modes.
Hit this button to send the script to the NIRSPEC server to be executed.