TAO
Tools for Automated Observing
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Introduction
  System requirements
 
Getting Started
  Installation
  Modeling slew times
  Measuring camera
  download times
  Specifying filter
  names and numbers
  Modeling the local
  horizon
  Creating user profiles
  Initializing target
  databases
  Customizing the
  scheduler
 
Daily Operation
  Starting observatory
  control software
  Updating target
  databases
  Generating a list of
  potential targets
  Preparing a list of
  observation requests
  Requests using
  default options
  Specifying exposure
  time
  Specifying camera
  resolution
  Specifying frame
  size
  Specifying frame
  mode
  Specifying filters
  Specifying the
  number of images
  to take
  Specifying the time
  interval between
  exposures
  Specifying the
  image insertion
  method
  Specifying the
  minimum altitude
  limit
  Specifying the
  maximum |hour
  angle| limit
  Specifying the
  moon avoidance
  radius
  Specifying a
  request identifier
  Specifying an
  observing window
  Specifying mosaics
  of CCD fields
    Page 1
    Page 2
  Running the
  scheduler
  Starting scheduled
  observations
 
Image Acquisition with
the MU Script
  Customizing the
  script
  Starting MU
  Sequence of events
  during an observing
  run using MU
 
Timing Refinement
  Collecting timing
  data
  Analyzing timing
  data
  Adjusting the
  empirical timing
  correction
 
Other Tools
  Slew time
  measurement script
  Minor Planet Checker
  query script
  Regression program
 
Etc.
  Software updates
  License agreement
  Contact the author
Daily Operation



Step 4: Preparing a list of observation requests (continued)

Specifying the image insertion method

The image insertion method determines how the scheduler will determine the "best" times to carry out an observation request. The four available image insertion methods may be selected using the opt, asap, alap, and mix keywords, whose meaning has been previously discussed:

  • If none of these keywords is present, the scheduler will use the keyword which is specified in the user's profile under "Image insertion method."

  • If one of these keywords is present, it will be used instead of the default keyword:

    • The opt keyword specifies that observations should be made at the highest possible altitude. For example,

      2003 QF70; opt
      

      is a request for observations of asteroid 2003 QF70, made by the default user. The default number of exposures specified in the default user's profile is being requested, and they should be taken as close to the meridian as possible. The other options for this request are all taken from the default user's profile.

    • The asap keyword specifies observations made at the earliest possible time. For example, the request

      2003 QF70; asap
      

      is identical to the previous one, except that the observations would take place at the earliest possible time.

    • The alap keyword is analogous to asap, with observations being made at the latest possible time.

    • The mix keyword tells the scheduler to try to achieve a trade-off between maximum altitude and minimum slew time in moving between the requested target and the next target. The relative importance of slew time minimization in this trade-off is specified in the scheduler configuration file.

Specifying the minimum altitude limit

If the minimum altitude limit for the exposures belonging to a given observation request is not specified explicitly, the default minimum altitude specified in the user's profile would be used. Although this may be adequate for many requests, the user may wish to specify a non-default altitude limit. This is done using the alt keyword:

NGC4698; alt>50

This would be interpreted as a request for observations of NGC4698, made by the default user. The observations would be carried out using the default options specified in the default user's profile, except that the minimum altitude limit would be 50 deg.

Note: Regardless of the minimum altitude limit specified in an observation request, no observations will be scheduled at altitudes and azimuths which are below the horizon line specified in the scheduler configuration file. Click here for more details about modeling of horizon lines.

Specifying the maximum |hour angle| limit

If the maximum |hour angle| limit for the exposures belonging to a given observation request is not specified explicitly, the default maximum |hour angle| specified in the user's profile would be used. Although this may be adequate for many requests, the user may wish to specify a non-default hour angle limit. This is done using the HA keyword:

NGC4698; HA<60

This would be interpreted as a request for observations of NGC4698, made by the default user. The observations would be carried out using the default options specified in the default user's profile, except that the maximum |hour angle| would be 60 min (which means that observations would be carried out when the object is at some hour angle between -60 and +60 min.

Note: Regardless of the maximum |hour angle| limit specified in an observation request, no observations will be scheduled at hour angles which violate the minimum and maximum |hour angle| limits specified in the scheduler configuration file. These limits represent safety slew limits for the telescope, so they should never be violated by any observation.

Previous: Specifying filters, number of images to take, interval between exposures
Next: Specifying moon avoidance radius, request identifier, observing window



© 1999-2004 Paulo Holvorcem