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The AO Acquisition Tool User's Guide


  1. Introduction
  2. Starting up the acquisition tool
  3. Grabbing an acquisition image
  4. Performing the acquisition
    1. Mode 1 - Setting up a complete AO integration
    2. Mode 2 - Moving an object to a target position
    3. Mode 3 - Moving an object onto the pickoff probe
  5. Finetuning an OASIS Acquisition
  6. Example acquisition scenarios
    1. Imaging observations with INGRID/OASIS
    2. Spectroscopic observations with OASIS
  7. Further notes

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1. Introduction


This page is intended to provide a step-by-step guide to using the AO Acquisition Tool in conjunction with the NAOMI adaptive optics system. It also outlines the most efficient techniques for performing target acquisition, for a variety of observing scenarios with the INGRID and OASIS instruments.

For more detailed documentation about the tool and its calibration, as well as troubleshooting information, you should refer to the WHT Acquisition Tool User Guide.

There are two major goals when performing an AO acquisition. The first is to accurately position the science target onto the science detector (of INGRID or OASIS) at the required position. The second is to select an appropriate guide star (which may or may not be the science target), for performing the AO correction, and to send its light to the wavefront sensor of the AO system. By using the acquisition tool outlined here, one can simultaneously perform both these goals, while operating with any sky PA.

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2. Starting up the acquisition tool


Main display page GUI

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3. Grabbing an acquisition image


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4. Performing the acquisition


Pick Object GUI

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5. Finetuning an OASIS Acquisition


For OASIS observing, one will normally have used Mode 1 (Setup AO Integration) for the acquisition. In this instance, the telescope and pickoff probe will have been suitably positioned and the guide star should appear on the AO wavefront sensor (once the NCU slide is back in the science position). The support astronomer should be able to directly close the AO loop if the acquisition tool is well calibrated; if not, ask the TO to tweak the telescope position to centre the guide star spots and then close the loop.

Assuming the observer has selected the science target position to correspond to the centre of the spectroscopic FOV of OASIS (denoted by a green circle in the overlay), then in principle one can start to take science exposures. However, due to the very small FOVs available with the four spatial enlargers used by OASIS, it is recommended to finetune the positioning of the science target whether to (a) centre the target, (b) offset the target or (c) mosaic a larger field of view. This finetuning can be performed with the OASIS Acquisition features of the acquisition tool; these treat the imaging mode of OASIS as an acquisition camera to correctly position the science target in the smaller spectroscopic field of view(s). The tool performs simultaneous and synchronised moves of the telescope and pickoff probe so that the guide star will always remain on the wavefront sensor.

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6. Example acquisition scenarios


This section is intended to record efficient techniques for performing the acquisition under different scenarios of targets and science modes. It is currently under construction and will be updated with more information in the future.

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7. Further notes


This tool will only work if it is correctly calibrated with the correct data in the Grab Acquisition Image window. These values will be monitored and updated by the AO team - any problems should be reported to them. If it is necessary to recalibrate the Nominal WFS Offset Pixels (eg. if the camera has been moved or if the dichroic has caused an offset):

For more details on the acquisition tool please refer to the WHT Acquisition Tool User Guide by Craige Bevil.

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Last Updated: 15 November 2005
Samantha Rix, srix@ing.iac.es