VOL 20 ISSUE 01 Space Telescope Science Institute NASA and G. Bacon, STScI. (See page 24.) NASA and G. NASA and G. Bacon, STScI. (See page 24.) NASA and G. Illustration Credit: Interview: Illustration Credit: Bill Workman & Ian Jordan An artist’s concept of a gas giant planet orbiting the cool, red dwarf star Gliese 876. Bill Workman,
[email protected], and Ian Jordan,
[email protected] An artist’s concept of a gas giant planet orbiting the cool, red dwarf star Gliese 876. Bill and Ian, you are working on the Hubble long-range (constraint) window with available telescope orbit resources. Since we don’t observing plan (LRP). Please explain the role of the LRP actually schedule the telescope, the task is—by definition—statistical in Hubble operations and the work that creating it entails. in nature. Like any good science project, the ‘fun’ part is dealing with the ILL: Well, it’s not clear we can describe what we do in less than ‘Hubble uncertainties in the system. In this case, this means predicting HST behavior BTime’, but we’ll try! and what the whole General Observer (GO) observing program will look like BILL & IAN: Primarily the Long Range Planning Group (LRPG) and the LRP for the cycle. exist to help the Institute and user community maximize the science output of the Hubble Space Telescope (HST). Observers see the LRP as a set of plan How do you know when you are done with the LRP? windows that represent times when a particular set of exposures are likely IAN: Well, the long range plan is never done! Perhaps the LRP logo should to be observed by the telescope, similar to scheduling observing runs at a be a yin-yang symbol? ground-based observatory.