Science Operations

Starting the software

Login to a mountain workstation

The MODS instruments must be run from the workstations on the mountain, obs1 and obs2.  If you are observing from the Tucson remote room, open an x2go session from one of the rm507 workstations to login to obs1 or obs2, using your partner account (az, inaf, lbtb, osurc; note lower case) and using a MATE session.
  • on the mountain: login to obs1 or obs2 using your partner account credentials.
    • Select “MATE” (not Gnome or any other) as the type of session.
  • in the Tucson remote room:
    • login to a rm507 workstation as observer (ask LBTO support staff for the password)
    • from the Applications menu in the bottom left corner, select x2go.
    • enter your partner account credentials.
    • You are now essentially working on the mountain obsN machine.

To copy your scripts to the mountain workstation:

From a terminal window on computer on which your scripts are located and from a directory just above the directory in which your scripts are located (here called myscripts), type:
scp -r myscripts/ <partner>@obs1.mountain.lbto.org:~/

This command will copy the entire directory, myscripts, to obs1 and put it under the directory /home/partner where partner is one of the partner account names (az, inaf, lbtb or osurc).

Check the status of MODS

Open a terminal window and type:
mods1 status (for MODS1); and
mods2 status (for MODS2)

Everything listed but the modsUI (User Interface GUI) should be open and owned by mods. If not, notify the TO, ISA, or ISp and ask them to restart the service. Once all but the GUI are open and owned by mods, proceed.

Start the MODS User Interface

In the terminal window type:

mods1 start gui

to open the MODS Control Panel for MODS1, or type:

mods2 start gui

to open the equivalent panel for MODS2.

Setup the…

 

 

FITS Image File Names

  1. On the right side of the Setup Screen, click Get Date to update the UT date in the image filenames. Make sure it is the correct UT date for the night; if it is before 1700 MST (00 UT), you should manually increment the number to reflect the UT date for the night. Click “Apply”.
  2. Check the filenames (i.e. mods1b.20130915.0001.fits) to ensure the index numbers are as expected. If you or someone else has taken files earlier during the same UT day, you may have to manually adjust the index number to reflect this. The Refresh button would do this, unless someone has clicked “Apply” already. As a rule, avoid the Refresh button.

Observer/Project Information

While many scripts will set the Partner Name, PropID and PI Name (in blue below) automatically, it is important to enter default values for data taken “by hand” or for scripts in which it is not specified:

  1. Observer Names (can be separated by commas and spaces). This goes into headers as the value for the keyword, OBSERVER.
  2. Enter the Partner Name: OSURC, AZ, INAF, LBTB, LBTO. The name entered here goes into the headers as PARTNER and determines how the data will be archived. (Multiple partners can be listed, separated by commas but no spaces.)
  3. Enter PropID
  4. Enter PI Name,
  5. Support (SUPPORT),
  6. Telescope Operator (TELOPS) and a
  7. Comment describing the run.

Once all the necessary updates have been made, click Apply, then Save. The Partner, PropID and PI Name will be overridden later by the parameters in the “Archive” blocks of subsequent MODS observing scripts.

The MODS User Interface is now running and setup. To learn how to start or end the night and to run scripts during the night, go to the Observing Procedure page. To learn more about the MODS GUI, specifically how to use it manually, go to the MODS User Interface page.

Launch modsDisp (mods2Disp)

In a terminal window, type modsDisp. This will launch two ds9 windows, one for the blue channel of MODS1 (MODS1Blue) and the other for the red channel (MODS1Red). Each image, as it arrives in the /newdata directory, will be displayed in the appropriate ds9 window. Leave the terminal window visible, as you can copy the filenames to paste into the modsAlign command line when you come to aligning the target in the slit, or alignment stars in the boxes on a MOS mask.
Type mods2Disp to launch this display tool for MODS2 images.

Preparing for the night

To prepare for the night, it is necessary to wake up MODS and to put MODS into observing mode.

Wake up MODS

Type modsWake [bino|1|2] to wake up both MODS (bino), MODS1 only (1) or MODS2 only (2).

“Waking up” a MODS involves turning on the IR laser, setting it to the correct power level and enabling it. The CCD settings are also reset and any internal devices that should be on during observing are turned on, while what should be off is turned off.

Take test images

Type modsSimSnap [bino|1|2] or modsSieveSnap [bino|1|2] to take a set of test images. “SimSnap” will take a pair of blue and red channel images through the Sieve Mask and then remove it from the focal plane to take a second set which is useful to check for and monitor debris on the optics. “SieveSnap” takes only the set of images through the Sieve Mask.

Put MODS into observing mode & “Home” the AGw stage

  1. Click the “Observing” button near the top left of the MODS User Interface. The text on this and other buttons will be orange while mechanisms are moving. Once they have finished moving,
  2. Click the “Home” button to the right of the AGw stage X, Y, focus and Filter positions to “Home” the guider stage.

Open ancillary monitoring tools

GCSGUI

In a terminal window, type GCSGUI left & to open the SX Guide Control System GUI and GCSGUI right & to open the same for DX.
These GUIs display the guide and wavefront sensing (WFS) camera images, along with measures of the guide star FWHM, the WFS wavefront error (should be <400nm for good collimation), and the average FWHM of the WFS Shack spots.

LBTplot

In a terminal window, type LBTplot to open the LBTplot tool. The buttons are context driven, and for MODS observing, the most useful ones are SXguide and DXguide, as they plot the guide star FWHM and flux as a function of time.