Spectroscopy in the Era of LSST
Thomas Matheson (NOAO), Xiaohui Fan (Arizona), Richard Green, (Arizona), Alan McConnachie (NRC-HIA), Jeff Newman (Pittsburgh), Knut Olsen, (NOAO), Paula Szkody (Washington), and W. Michael Wood-Vasey (Pittsburgh)

TL;DR
This paper summarizes a workshop discussing the role and future needs of spectroscopy in the context of LSST, focusing on science applications across multiple astrophysical domains.
Contribution
It provides a comprehensive overview of science cases and desired capabilities for spectroscopy to support LSST-era research across various fields.
Findings
Identification of key science drivers for spectroscopy in LSST era
Framework for characterizing spectroscopic needs for different science cases
Synthesis of desired capabilities to guide future instrument development
Abstract
This report summarizes the results of the 'Spectroscopy in the Era of LSST' workshop held April 11-12, 2013 in Tucson, Arizona. At the workshop, there were breakout sessions covering four broad science topics. These were: time domain science, Galactic structure and stellar populations, galaxies and AGN, and dark energy and cosmology. We present the science cases discussed in these breakout sessions and provide a synthesis of highly desired capabilities that meet needs across all four broad topics. We also present a table that will be useful to characterize the needs of specific science cases in a format that provides a general framework for discussion of future spectroscopic capabilities.
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Taxonomy
TopicsAstronomy and Astrophysical Research
