6. Example 3 - Nod-and-Shuffle Point Source

In this example we will reduce a GMOS longslit nod-and-shuffle observation of a quasar with the R400 grating. The observations were obtained with the GMOS-N Hamamatsu CCDs.

• 6.1. Example 3 - Datasets descriptions
• 6.2. Example 3 - Nod-and-Shuffle Point Source - Using the “reduce” command line
• 6.3. Example 3 - Nod-and-Shuffle Point Source - Using the “Reduce” class