Before making ACP plans, you need to set things up in the Preferences window. If you're a new Starry Night user, you should read Getting Started With Starry Night. If you plan to take dusk or dawn sky-flats, be sure to read Automatic Sky Flats. Before turning on any of the (advanced) Flat Planning options, read Flat Planning Options below.
The ACP Video web site has a series of very useful videos covering Planner.
If you are a beginner, or routinely plan for single targets, it may be helpful to turn off ACP Planner's target position and timing visualization features (later versions of Planner have this off by default). You can do this with the Disable Timing Features checkbox in Tools/Preferences. While this may help you get started, it also hides Planner's most useful capability. Don't disable timing features unless you have a hard time understanding how objects move in the sky as time progresses, and don't want Planner to help you get your images at the most favorable times.
If you use Planner with more than one observatory and/or equipment setup, you can easily switch between preferences. In Planner's File menu, there are options for saving and loading profiles. All of Planner's preferences and presets are saved in a profile. The Observatory Name field in preferences makes it easy to tell which profile you have loaded. The profiles are XML files. Normally you save them to the Profiles subfolder, but you can send these to other users. If you operate a Share Your Sky! observatory, you might want to put the profile for your observatory in the WebDocs\files subfolder of your ACP install folder so your users can download it and instantly set their Planners up for your observatory.
By default, ACP Planner assumes you are making plans for your local observatory. If you are making plans for a remote observatory in a different time zone, you can turn on a feature that causes "local" times in Planner to match those at the remote observatory. It is called "Local time at Observatory..." and includes a field for the observatory's time offset from UTC. Leaving this off will cause local times to be for your location and time zone.
This feature is really useful when you're using Starry Night in conjunction with Planner. Of course(!) the Starry Night time and zone must be set for the remote observatory so you have a view of the sky from there, right? Well, Planner will automatically grab the time zone information from the Starry Night and configure itself to show times that match those in the planetarium (local time at the observatory).
If you plan without a planetarium, you need to set the time zone offset for the observatory next to the checkbox. The value is the number of hours that local time at the observatory differs from UTC, including any daylight time in effect. West is negative. For example, US Eastern Standard Time is 5 hours earlier than UTC, so the value to enter is -5 (minus 5). If daylight savings changes at the observatory, you must manually adjust this to reflect the change!
The Observing Time Overhead section is used to estimate the total time that each of your image sets will take. Values are not critical. Try to get something close to the real times (ask the observatory operator if you are a web user). If the times are too long, the planner will show the observatory busy longer than it will actually be, reducing the available time showing in the planner. If the times are too short, imaging for the next object could be delayed because you planned it for a time when the observatory was still busy doing the previous object. When in doubt, make the times longer rather than shorter. Here are some things to be aware of:
The Filters section lists the filters that the ACP-based observatory has available. The filter names must be the same as those of the observatory! If you are the observatory operator, simply click Get From MaxIm to load MaxIm's filter set into ACP Planner. If you are a web user, look on the ACP/Share Your Sky!™ Instruments and Reference Info page for the observatory you will be using and fill in the correct filter names. If you are planning to use Planner's Flat Planning feature, list the filters in "dusk flat" order.
Virtually all robotic observatories have automatic focusing (AF) available, and these settings determine how your plans will manage AF.
If you are planning for a remote ACP observatory, fill in the remote info and click Test. If it says your info is OK, then you'll be offered to have your plans uploaded immediately after viewing them in Notepad.
After filling in this info, click Test to verify that your info is valid.
Now you're ready to start using the ACP Planner. Before doing so, though, if you're a new Starry Night user you should read Getting Started With Starry Night. Then read through the appropriate Routine Use page.
If you want to use ACP Planner to generate ACP Flat Plans (advanced users only), you must first order the filters in the list. Filters must be listed in dusk order, that is, from the least sensitive to the most sensitive. Note that Red is typically the least sensitive for flat fields (you're imaging a blue sky!). Typical order would be Red, Green, Blue, Clear for color astro-imaging, or R, G, B, V for Johnson-Cousins. Narrowband filters used for astro-imaging are typically much fainter, and thus should be listed before color or J-C filters.
There are three options in the Flat Planning section of Preferences:
-flat
appended. With it on, you'll see a second file-save window when saving your plans. In this second file-save window, you name your flat plan. Don't turn this on unless you're an expert user and need this extra level of flexibility! See Flat Plan Name and Location.