Table of Contents
List of Figures
spiaFtsBackgroundRemoval. This task performs a background subtraction for sparse pointed observations and works with full Observation Contexts.
spiaFtsNoiseEstimatetask in HIPE.
doPlotsis set to
False) for the observation of Saturn with observation ID 1342198279.
preCube, in the Spectrum Explorer. The RA and Dec for each spectrum is shown, and individual spectra can be plotted by clicking in the second column labeled "0". Double-clicking on the "0" column title will deselect or select all spectra.
NaNspaxels within the map for the Naive projection, but no holes when a convolution is applied.
spireSynthPhotometryfor a sparse HR observation of CRL618. The input spectra, calculated synthetic photometry and photometer values provided are all included. The SPIRE photometer RSRFs are also plotted by the task for reference.
sincGaussprofiles with various widths. There is a cutoff in the wings of the function that gets closer to the central peak as the line width decreases.
Spectrum1dproduced by the Combine PACS and SPIRE spectra Useful script, for the example source CRL618. From left-to-right, the segments are SPIRE SLW, SPIRE SSW, PACS R1, PACS B2B, PACS B2A. The log-log scale highlights the good agreement between the instrument calibrations.
List of Tables