Date: Fri, 14 Jul 2000 15:44:59 -1000 From: Bill Vacca To: denault@jeans.ifa.hawaii.edu Cc: rayner@jeans.ifa.hawaii.edu, vacca@minerva.ifa.hawaii.edu Subject: Re: spex problems.. Hi Tony, I have a suggestion for the guider set up, that I think will accommodate the ways most observers will use SpeX. The XUI could have a Guider Modes tab, with three "sub-tabs" (if possible). The three sub-tabs would be the three different guider modes: offset, nod, and step. Each tab would bring up a panel. The Offset panel would have a Box Center entry, a Box Width entry, a Default GuideBox Button, and a Send to TCS button. The observer could either give the position and size of a box or accept the default box, which would be centered (in both x and y) on the slit. This mode would be used by people who observe extended objects and want to go to sky between exposures. They could guide on the object or on something else in the field, using the box they set up. The Nod panel would have a Box A Center entry, a Box A Width entry, a Box A Center entry, a Box A Width entry, a Default GuideBoxes Button, and a Send to TCS Button. Again, the user could either accept the default guide boxes (the positions of which depend on the slit being used), or they could define their own A and B beam guide boxes. This mode would have to be able to read the position angle of the slit and figure out the correct nod offsets for the telescope when the beam is switched. All of this would be done once the Send to TCS button is pressed. The Step panel would have a Number of Positions entry, a First Box Center entry, a Box Width entry, a Step Size entry, and a Send to TCS Button. The user would specify how many guide boxes she wants along the slit, the position of the first box, and the step size between boxes (in either arcseconds or pixels). This mode would also have to read the position angle of the slit and calculate the offsets between the various boxes. The observations would be carried out entirely in the A beam, and the telescope would be stepped between each exposure. When it gets to the end, the telescope is reset to the first position. I think this would encompass most of the ways people will observe with SpeX. This layout would allow the observer to have a lot of freedom in setting up the guide boxes, while not making it complicated for the 99% of the people who will use the standard default guide boxes. What do you think? - Bill