OASIS daily checks


Version 1.0 (last update 18th December 2005 by Jürg Rey)

These checks should be performed with a flattened DM e.g. after simplexing with AG7.

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Introduction

In the interests of brevity it has been assumed that users of this document will have a reasonable level of familiarity with the WHT observing environment. A key component of this environment is ING's ULTRADAS data acquisition system. For further information about this system please consult the Operations manual for UltraDAS.

To get light onto OASIS you need:

WHT ULTRADAS startup for OASIS

  1. Login to the observing system ICS computer (currently taurus) as: whtobs

  2. The following two windows should then appear:

  3. Prior to starting any of the observing software OASIS needs to be configured for use in the observing system. In the Observing System (pink) window enter:

    obssys, followed by option 1

  4. Review the cameras and instruments that are currently defined in the observing system. If necessary select:

    option c

    to edit the WHT configuration file (look on the CCD whiteboard to see which DAS machine is hosting the OASIS camera server and enable the appropriate entry in the configuration file.)

  5. On completion of this step the Observing System (pink) window should display the following prompt:

    SYS@taurus>

  6. Using the Combined Terminal (yellow) window select the tab page associated with the OASIS camera server. Type:

    obssys

    followed by option 1, then option 1 again. At the end of this configuration procedure you should receive a DASn prompt (where n refers to the das machine you are on).

  7. Again, in the same window type: startobssys

    to load the ULTRADAS camera software, checking that no unusual error messages are emitted. Repeat steps 5-6 for any other cameras that have been defined in the observing system configuration.

  8. At the Observing System (pink) window type:
  9. startobssys

    to start the main components of the observing system. During start-up various windows will be started. The important ones for OASIS are:

  10. When the system prompt is returned, the observing system is ready for use. To avoid screen clutter, minimise the windows that are not being used.

Take Test Image

  1. To take an image, enter at the prompt:
  2. SYS@taurus> run OASIS 2
  3. Wait until the ULTRADAS Camera mimic indicates that the detector has been read out and has been 100% processed. Make sure the images are written (with TCS header information) to the Observing Log.
  4. Immediately after every readout, the Real Time Display Tool (RTD) will detect the new image file and load it to the XIMTOOL display window. You expect to see one spot close to the CCD centre.
  5. Now take a bias to check the detector for noise:

Analyze the Test Image

  1. Login on the WHT Data Reduction Sparc (whtdr) as: whtguest
  2. Open the programs menu by clicking on the background and start an xgterm and ximtool session.
  3. In the xgterm, start an IRAF session using the command: cl
  4. Within IRAF, change to the obsdata directory where the images are being stored. This information can be found on the ULTRADAS Camera mimic. e.g.
  5. cd /obsdata/whta/20051218
    The obsdata discs currently being: whta, whtb, whtc, whtd & whte.
    It should be noted that a new 'date' directory is generated at 12:00 UTC daily

  6. To display an image, enter at the IRAF prompt: display rnnnnnn[1] 1 fill+
  7. At the IRAF prompt, type: imexam
  8. Check (using the r command) the FWHM of the run exposure and (using the m command) the bias level.
  9. Exit imexam by typing: q (the cursor must be in the image area).

Document History

Rev 1.0 Dec 18th 2005 JR; OASIS checks based on INGRID checks document.

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