6. Example 3 - L-band Longslit Point Source (10 l/mm grating)

In this example, we will reduce the GNIRS L-band longslit observation of a Be-star.

This observation uses the 10 l/mm grating, the long-red camera, a 0.1 arcsec slit, and is centered at 3.7 m. The dither pattern is a standard ABBA sequence.

• 6.1. Example 3 - Datasets description
• 6.2. Example 3 - L-band Longslit Point Source - Using the “reduce” command line
• 6.3. Example 3 - L-band Longslit Point Source - Using the “Reduce” class API