The Near Infrared Spectrograph (NIRSpec) on board of the James Webb Space Telescope (JWST) will be equipped with an Integral Field Unit (IFU) which will allow the two-dimensional spectral characterization of astronomical objects with unprecedented depths, especially in the 2-5 micron wavelength range. In particular, NIRSpec-IFU observations of high-z galaxy populations will permit the capture of their often complex two-dimensional physical and kinematical structure, a pre-requisite for carrying out a number of studies. These types of observations will also help to understand possible observational biases of large 1D (i.e. slit) surveys to be carried out in multi-object mode. Here we describe the main characteristics of the NIRSpec-IFU, as well as its expected sensitivity and performance for observations of high-z galaxy populations. © 2007 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
Arribas, S., Ferruit, P., Jakobsen, P., Boeker, T., Bunker, A., Charlot, S., … Valenti, J. (2007). The integral field unit of the near infrared spectrograph for JWST. In ESO Astrophysics Symposia (Vol. 2007, pp. 21–26). https://doi.org/10.1007/978-3-540-73491-8_3
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