Entering Observing Requests
Specifying Solar System Objects
Setting Up Dawn Calibration Frames
Setting Up Automatic Flat Fields
Familiarization Using the Simulator
Live Observing With Scheduler
Locating and Viewing Log Files
Before using the ACP Scheduler, it's really important that you set it up with the timing characteristics of your particular observatory. If you haven't done this, open the Configuration window (Scheduler menu) and look for the ACP Sequencer section. Change the timing values to match your observatory. Click on an item to display details in the area below the list.
Next, you need to create some requests in the scheduler's database. It is suggested that you first look over the Concepts page. The Schedule Browser (not to be confused with a web browser!) is the graphical tool supplied with Scheduler that lets you browse and enter observing requests.
If you are an astro-imager it is strongly suggested that you use the web browser interface to Scheduler, and submit your requests via the Submit Astro-Imaging Request form!
ACP Planner can export plans as RTML, so if your observing needs are met by Planner you already have a graphical tool for generating RTML input to Scheduler. If you have special needs, the way to generate RTML is with planner scripts. Please see Planner Scripts and look at the scripts in the Planner Scripts folder under Scheduler' installation folder. Assistance with adjusting these scripts for your needs is available from DC-3 Dreams.
Please note that the desktop Schedule Browser is not intended as a mass data entry tool. It is intended that most observing requests will be entered via the Internet/Web Submission Forms or via imported Remote Telescope Markup Language (RTML) which can be produced via a variety of means, including the free ACP Planner.
Start the Schedule Browser now.
In order to use the name, number, or designation for a minor planet or comet, the MPCORB and MPCCOMET databases must be initialized with the latest info from the Minor Planet center. See ACP Help on how to do this. These ASCOM-supplied components are installed by ACP, but it is up to you to download the databases for minor planets and comets from the Minor Planet Center then run the database construction tools supplied. You only have to do this every few months.
Using the desktop Schedule Browser or via RTML, it is possible to specify solar system objects by their orbital elements. This allows the system to calculate the ephemeris (the current coordinates) of the body at the time of the exposure, eliminating the need to force such observations to be at a fixed time. There are two ways that you can provide Scheduler with orbital elements:
In addition to the above, you may specify a rough ephemeris with 4 lines of timed coordinates spaced about 2 hours apart. This is accessible via the Ephemeris button in the desktop Schedule Browser. The format for each line is given in the Ephemeris window. It matches the MPC's "NEO Ephemeris" format, but you can make this info up easily with any planetarium which will give J2000 positions vs time. The time must be UTC of course!
Before turning on the Dawn Calibration Frames option in the Scheduler, you must be familiar with ACP's observing plan syntax and have the SchedulerCalFrames.txt in place. For more information see Dawn Calibration Frames.
Before turning on the Dawn Flat and/or Dusk Flat options in the Scheduler, you must be familiar with ACP's automatic flat system and have SchedulerDawnFlats and SchedulerDuskFlats flat plans in place. For more information see Automatic Flat Frames.
At this point you are ready to run the Scheduler and have your image taken at the appropriate time.
Before making a real run, it is strongly suggested that you become familiar with the Scheduler by running with the Simulator. Check out that page!
Your observations will be taken when constraints are met and when time is available for them.
The scheduler engine logs its activities separately from the ACP activity accompanying each Observation. The scheduler log can be viewed via the scheduler's Scheduler menu, View Log File. The logs are named with a date/time style and are saved by default in My Documents\ACP Astronomy\Scheduler Engine Logs. You can change this via Scheduler settings, Dispatcher section (1), Log Directory. This is useful for making scheduler logs visible via the web (for example).
Each job that Scheduler sends to ACP results in a "run log", and these are kept separately. By default, these logs can be found in one of two places. If the Scheduler submitted the Observation to ACP on behalf of the local observatory operator (the Plan was entered via the desktop Schedule browser or RTML import), the ACP Logs will be in My Documents\ACP Astronomy\Logs\Scheduler. If the Observation is the result of a request submitted via a web form from a remote user, the logs will be put into that user's web-visible My Documents\Logs\Scheduler.
It is possible to do most anything you want with the ACP logs generated for Observations given to ACP by Scheduler. For more information see Custom Image/Log Folder and File Naming.