MIRI LRS Mosaics
Mosaics for low-resolution spectroscopy mode
Mosaics for an LRS observation can be implemented in the Astronomer's Proposal Tool (APT) using the JWST APT MIRI Low Resolution Spectroscopy template. These mosaics provide coverage of larger fields of view (FOV) that extend beyond a single pointing. Mosaics are only supported for observations with the LRS slit; the LRS slitless mode is dedicated to single-pointing time-series observations.
A pointing pattern can be defined in the Mosaic Properties tab in the observations form. Here, the pattern is defined in rows, columns, and percentage overlap between the pointings. Note that a similar strategy can be achieved by selecting the MAPPING option for the Dither strategy, and specifying the pattern steps in spatial and spectral directions, in arcseconds. The two can also be combined to execute a dither pattern at each mosaic pointing location, if specific spatial sampling of the target is required.
For mosaics, the number of rows sets the number of steps in the dispersion (cross-slit) direction, while the number of columns sets the number of steps in the cross-dispersion direction (the spatial direction, or along the slit). If the user wishes to observe the position pointed to by the target coordinates in the center of the slit, they should set an odd number of rows.
Users are strongly encouraged to always check the defined pattern using the APT Aladin visualization functionality, which shows the slit footprints superimposed on the target.
The user should also consider using the MIRI Medium-Resolution Spectrometer (MRS), which provides integral field spectroscopy (IFU) at higher spectral resolution than the LRS (from ~5 to 28.5 µm, albeit without continuous spectral coverage).
Bold italics style indicates words that are also parameters or buttons in software tools (like the APT and ETC). Similarly, a bold style represents menu items and panels.