| Button | Action |
|---|---|
| Open a directory navigator to select a local FITS file containing a SOFIA spectral cube downloaded from the SOFIA Science Archive. |
After opening the file, the median of cube along the spectral dimension is shown on the image panel while the spectrum plotted on the left panel is obtained by summing all the spatial pixels for each wavelength.
In the case of FIFI-LS two further cubes are read and displayed:
In the case of GREAT, one can open the Tmb cubes. In this case, only the flux panel is displayed since the exposure map is not yet saved in the GREAT products. The program assumes that the flux is conserved in Tmb and then it converts it into Jy.
It is possible to open Spectral Simple Cube generated by the Herschel pipeline and available in the Herschel Science Archive. After downloading the level 2 PACS spectroscopy products from the archive, search for the SpectralSimpleCube:
find . -name 'SpectralSimpleCube'
You will see the location of several files. For instance, in the case of the red array, simple spectral cubes are available for the following products:
Each of these directories contains a different product which is coded in the name of the directory.
| Directory | Meaning |
|---|---|
| HPS3DDR | Herschel Pacs Spectroscopy 3D Drizzled Red |
| HPS3DEQDR | Herschel Pacs Spectroscopy 3D Equidistant wavelength grid Drizzled Red |
| HPS3DPR | Herschel Pacs Spectroscopy 3D Projected Red |
The last one uses a normal projection. The other ones use drizzled projections. In particular the "Equidistant wavelength grid" is an interpolation along a wavelength grid with a constant step.
The PACS cubes have extensions for flux and exposure.
It is possible to resize the relative sizes of the image and spectral panel by clicking and dragging the splitter in between the two windows.