Harrison, F.A. and Craig, W.W. and Christensen, F.E. and Hailey, C.J. and Zhang, W.W. and Boggs, S.E. and Stern, D. and Cook, W.R. and Forster, K. and Giommi, P. and Grefenstette, B.W. and Kim, Y. and Kitaguchi, T. and Koglin, J.E. and Madsen, K.K. and Mao, P.H. and Miyasaka, H. and Mori, K. and Perri, M. and Pivovaroff, M.J. and Puccetti, S. and Rana, V.R. and Westergaard, N.J. and Willis, J. and Zoglauer, A. and An, H. and Bachetti, M. and Barrière, N.M. and Bellm, E.C. and Bhalerao, V. and Brejnholt, N.F. and Fuerst, F. and Liebe, C.C. and Markwardt, C.B. and Nynka, M. and Vogel, J.K. and Walton, D.J. and Wik, D.R. and Alexander, D.M. and Cominsky, L.R. and Hornschemeier, A.E. and Hornstrup, A. and Kaspi, V.M. and Madejski, G.M. and Matt, G. and Molendi, S. and Smith, D.M. and Tomsick, J.A. and Ajello, M. and Ballantyne, D.R. and Baloković, M. and Barret, D. and Bauer, F.E. and Blandford, R.D. and Brandt, W.N. and Brenneman, L.W. and Chiang, J. and Chakrabarty, D. and Chenevez, J. and Comastri, A. and Dufour, F. and Elvis, M. and Fabian, A.C. and Farrah, D. and Fryer, C.L. and Gotthelf, E.V. and Grindlay, J.E. and Helfand, D.J. and Krivonos, R. and Meier, D.L. and Miller, J.M. and Natalucci, L. and Ogle, P. and Ofek, E.O. and Ptak, A. and Reynolds, S.P. and Rigby, J.R. and Tagliaferri, G. and Thorsett, S.E. and Treister, E. and Urry, C.M. (2013) 'The Nuclear Spectroscopic Telescope Array (NuSTAR) high-energy X-ray mission.', Astrophysical journal., 770 (2). p. 103.
The Nuclear Spectroscopic Telescope Array (NuSTAR) mission, launched on 2012 June 13, is the first focusing high-energy X-ray telescope in orbit. NuSTAR operates in the band from 3 to 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 100-fold improvement in sensitivity over the collimated or coded mask instruments that have operated in this bandpass. Using its unprecedented combination of sensitivity and spatial and spectral resolution, NuSTAR will pursue five primary scientific objectives: (1) probe obscured active galactic nucleus (AGN) activity out to the peak epoch of galaxy assembly in the universe (at z <~ 2) by surveying selected regions of the sky; (2) study the population of hard X-ray-emitting compact objects in the Galaxy by mapping the central regions of the Milky Way; (3) study the non-thermal radiation in young supernova remnants, both the hard X-ray continuum and the emission from the radioactive element 44Ti; (4) observe blazars contemporaneously with ground-based radio, optical, and TeV telescopes, as well as with Fermi and Swift, to constrain the structure of AGN jets; and (5) observe line and continuum emission from core-collapse supernovae in the Local Group, and from nearby Type Ia events, to constrain explosion models. During its baseline two-year mission, NuSTAR 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, 6° 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 10 yr, we anticipate proposing a guest investigator program, to begin in late 2014.
|Keywords:||Space vehicles, Instruments, X-rays.|
|Full text:||(VoR) Version of Record|
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|Publisher Web site:||http://dx.doi.org/10.1088/0004-637X/770/2/103|
|Publisher statement:||© 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A.|
|Record Created:||17 Sep 2013 12:20|
|Last Modified:||05 Aug 2014 13:03|
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