![]() ![]() temp_dir = / data2 / tmp # the directory to which temporal results will be saved verbose = True # Run parameters run_mode = Lazy # default (initial) run mode of the QL it can be (None, Lazy, Prereduce)Īlthough the user can edit these values in the config file, some of them can be set easilyįor the complete list of the parameters available on the $PAPI_CONFIG file, see Main config file section. # Next are some configurable options for the PANIC Quick Look tool # some important directories # source = / data1 / PANIC / output_dir = / data2 / out # the directory to which the resulting images will be saved. The following header keywords are also required: However, and in order to group and reduce observing sequences, The complete definition of the FITS headers can be found on the GEIRS documentation.įor general purpose, such as viewing and simple analysis, only minimal headers Or Multi-Extension FITS (MEF), however MEF are prefered. Because PANIC has a FPA of four detector, the FITS files can be Single Extension FITS (SEF) PQL only supports FITS (Flexible Image Transport System) with two-dimensional Supports FITS images, multiple frame buffers, region manipulation, and many The visualization application used to display the images is SAOImage ds9, which The status and progress of the observation during the night. However, its functionalities have been provided mainly in near-real time to check Offline mode (after the observation, with all data files already stored in the disk) PQL can be operated in both near-real time mode (during the observation) and Option available is to select a set of files and request to shift and align them. Sky subtraction looking for the nearest N frames around the selected one. For example, you will be able to select a file,Ĭompute some statistics values (background, FWHM, min, max, …) or ask for the In addition, PQL allows you to execute manually in an interactive way Sky subtraction (using N-nearest frames or own sky ) ![]() Only display the FITS image with no processing ![]()
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