![]() ![]() When you click this checkbox, the Input directory and Output directory fields will be automatically filled Instead the ‘Main’ tab used for input and output directory. To set the value, the user must push the ‘Temporary Dir’ button than appears on the ‘Setup’ tab, It is advised that this directory follow the next format: PQL requieres all data to lie in some mainĭirectory, not being required to distribute the files in individual sub-directories for darks, flats,Īnd science images. This directory is specifiedĪt the beggining of the night on the Observation Tool. This is where you tell PQL where the data are or being saved by GEIRS. In the ‘Main’ tab panel of PQL main window, the fitst thing to set up are the data directories: 2.5.3.2. This tab panel contains the following controls: The tool bar duplicates some of the options available from the menu bar or the pop-up menu.Ĭurrently, there are several buttons which provide quick access to change the most frecuently-used PQL actions:Ĭhange the source input directory: the same that Input directory.ĭisplay the current selected image: the same that Display. If the internet conection or proxy is not correctly configured. Opens a web browser which shows an on-line HTML version of this user’s manual. The menu bar provides acces to some PQL’s capabilities. The additional windows, usually generated by matplotlib than can be copied to the clipboard, Images are displayed in an external well-known application, ds9. PQL Main window contains a Menu bar (1), Tool bar (2), four Tabbed panels (3) and 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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