3D Spectroscopic Instrumentation
Abstract
In this Chapter we review the challenges of, and opportunities for, 3D spectroscopy, and how these have lead to new and different approaches to sampling astronomical information. We describe and categorize existing instruments on 4m and 10m telescopes. Our primary focus is on grating-dispersed spectrographs. We discuss how to optimize dispersive elements, such as VPH gratings, to achieve adequate spectral resolution, high throughput, and efficient data packing to maximize spatial sampling for 3D spectroscopy. We review and compare the various coupling methods that make these spectrographs ``3D,'' including fibers, lenslets, slicers, and filtered multi-slits. We also describe Fabry-Perot and spatial-heterodyne interferometers, pointing out their advantages as field-widened systems relative to conventional, grating-dispersed spectrographs. We explore the parameter space all these instruments sample, highlighting regimes open for exploitation. Present instruments provide a foil for future development. We give an overview of plans for such future instruments on today's large telescopes, in space, and in the coming era of extremely large telescopes. Currently-planned instruments open new domains, but also leave significant areas of parameter space vacant, beckoning further development.
Keywords
Cite
@article{arxiv.0910.0167,
title = {3D Spectroscopic Instrumentation},
author = {Matthew A. Bershady},
journal= {arXiv preprint arXiv:0910.0167},
year = {2009}
}
Comments
53 pages, 6 tables, 17 figures; to appear in ``3D Spectroscopy in Astronomy, XVII Canary Island Winter School of Astrophysics,'' eds. E. Mediavilla, S. Arribas, M. Roth, J. Cepa-Nogue, and F. Sanchez, Cambridge University Press, 2009; high-resolution version available http://www.astro.wisc.edu/~mab/publications/ws3d05.pdf