Except for an additional overhead for guide star acquisition and tracking set-up, there are no overheads exclusive to moving targets. On this page we provide examples of general overheads that apply to specific moving target observations.
Guide star acquisition and tracking
Main article: JWST Guide Stars
Guide star acquisition and initiation of tracking for moving targets will incur a 90-second overhead. An additional 30 seconds will be applied for each dither. These overheads are unavoidable for all moving target observations.
Time critical observations
Any observations specified to occur within a window of 1 hour or less are considered time critical and will incur a 1-hour (3600-second) overhead. Examples for Solar System targets include, but are not limited to, observing:
It is recommended that efforts be taken to avoid making your observations time critical, but in some cases the scientific program may require it. Below are some tips on how to avoid the 1 hour overhead.
Be careful when selecting specifying a phase constraint or a central meridian longitude constraint. For example, Jupiter's rotation period is 10 hours, so providing a phase constraint between 0.0 and 0.11 (a range of ~40 degrees of longitude) will not incur the 1 hour overhead, but a phase constraint between 0.0 and 0.09 (a range of ~32 degrees of longitude) will incur the overhead. Careful consideration of science requirements can avoid this overhead.
If complete longitudinal coverage is desired for a quickly rotating body, remaining on the object during an entire rotational period is recommended. For example, full rotational coverage of Jupiter can be obtained in ~10 consecutive hours of observations and avoids the 1 hour overhead because specific phases are not required.
Observations of faster-moving objects (asteroids, NEAs, nearby comets, etc.) at specific phase angles are more likely to incur the 1-hour overhead than observations of slower-moving objects (Centaurs, KBOs, the giant planets, etc.).
Target of opportunity (ToO) observations
There are two different categories for ToO observations: disruptive and non-disruptive. A non-disruptive ToO program activation is one that occurs 14 or more days prior to the planned observation. A disruptive ToO activation is one that occurs less than 14 days prior to the planned observation. Disruptive ToO activations that occur within 3 days of the planned observation will incur a 0.5-hour (1800-second) overhead. There are no overheads for ToO activations that occur 3 or more days before the planned observation; however, only a small number of disruptive ToO programs will be executed each cycle.
Making use of smart accounting
Main article: JWST APT Smart Accounting
Smart accounting is available for planning moving target observations as of APT 25.1.1. This process reduces the slew time charged to visits to the same target in the same same observation folder. Without smart accounting, the slew time for each visit is set at 30 minutes (1800 seconds) by default. In reality, consecutive visits to the same target do not require 30-minutes of time to slew to the target because the observatory is already pointed at the target. Using smart accounting, the slew time overhead charged to the program can be significantly reduced. For example, an observation of Titan with the NIRSpec IFU followed right afterwards by an observation of Titan with the MIRI MRS would be charged 30 minutes for the initial slew to Titan for the NIRSpec observations and a significantly shorter time (<5 minutes) for switching instruments to MIRI, target acquisition, and re-acquiring a guide star.
To run smart accounting in APT, follow the instructions on the JWST APT Smart Accounting page.
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