XMM Users' Handbook


next up previous contents
Next: XMM support instruments Up: OM specific proposal submission Previous: OM star tracking windows

   
Choice of non-default OM science windows

For OM observations more than one science window may be defined. However, it is not possible to select the entire OM FOV for science observations. There are several boundary conditions that limit the user's choice and which must be taken in account properly if a non-default instrument configuration is to be used. Note that the use of non-default OM instrument configurations is discouraged by the SOC for AO-1.


  
Figure 72: When the boundaries of OM science windows are defined in detector pixel coordinates, the relative location of the windows with respect to each other does not change. However, different areas on the sky are imaged under different position angles.
\begin{figure}
\begin{center}
\leavevmode
\epsfig{width=0.8\hsize, file=figs/omroll.eps}
\end{center} \end{figure}


  
Figure 73: Defining the locations of OM science windows in sky coordinates one makes sure that (approximately) the same area of the sky is imaged under different position angles. Now, however, the OM science windows can change their relative locations. Windows 3 and 5 (which used to be in the upper left corner of window 3, see Fig. 72) are now partially overlapping, which is not allowed and window 4 is now partly outside the OM FOV (which is also not allowed).
\begin{figure}
\begin{center}
\leavevmode
\epsfig{width=0.8\hsize, file=figs/omnewwin.eps}
\end{center} \end{figure}

For a more detailed explanation see the technical note on Constraints on the OM Window Configuration and Definition of the OM Default Configurations (§ 8).


next up previous contents
Next: XMM support instruments Up: OM specific proposal submission Previous: OM star tracking windows
European Space Agency - XMM Science Operations Centre