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      The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

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          Abstract

          The Nuclear Spectroscopic Telescope Array (NuSTAR) mission, launched on 13 June 2012, is the first focusing high-energy X-ray telescope in orbit. NuSTAR operates in the band from 3 -- 79 keV, extending the sensitivity of focusing far beyond the ~10 keV high-energy cutoff achieved by all previous X-ray satellites. The inherently low-background associated with concentrating the X-ray light enables NuSTAR to probe the hard X-ray sky with a more than one-hundred-fold improvement in sensitivity over the collimated or coded-mask instruments that have operated in this bandpass. Using its unprecedented combination of sensitivity, spatial and spectral resolution, NuSTAR will pursue five primary scientific objectives, and will also undertake a broad program of targeted observations. The observatory consists of two co-aligned grazing-incidence X-ray telescopes pointed at celestial targets by a three-axis stabilized spacecraft. Deployed into a 600 km, near-circular, 6degree inclination orbit, the Observatory has now completed commissioning, and is performing consistent with pre-launch expectations. NuSTAR is now executing its primary science mission, and with an expected orbit lifetime of ten years, we anticipate proposing a guest investigator program, to begin in Fall 2014.

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          Author and article information

          Journal
          30 January 2013
          Article
          10.1088/0004-637X/770/2/103
          1301.7307
          b1d8ed97-8426-42a7-a1da-029436c74788

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          20 pages, 12 figures, submitted to the Astrophysical Journal
          astro-ph.IM astro-ph.HE

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