Author(s): , , , , , , , ,
Institution(s): 1. Space Telescope Science Institute
The Near Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope will provide astronomers the ability to observe through fixed slits, the integral field unit, or in multi-object mode with the micro-shutter array, at spectral resolutions of R ∼ 100, 1000, and 2700. The combination of JWST’s sensitivity and superb resolution in the infrared and NIRSpec’s full wavelength coverage from 0.6 to 5 μm will open new parameter space for studies of galaxies and resolved stellar populations alike. We will provide a general overview of the NIRSpec instrument and the user interface development, including proposal planning and the data calibration and reduction pipeline. We will discuss the capabilities of NIRSpec for survey science, and introduce the science use cases that are being used to drive development of the NIRSpec user interfaces.