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NuSTAR observations of rotation-powered pulsars and magnetars

Published online by Cambridge University Press:  20 March 2013

V. M. Kaspi ,
H. An ,
M. Bachetti ,
E. Bellm ,
A. M. Beloborodov ,
S. Boggs ,
D. Chakrabarty ,
F. Christensen ,
B. Craig  and
F. Dufour
...Show all authors
V. M. Kaspi
Affiliation:
Department of Physics, McGill University, Montreal, Canada email: vkaspi@physics.mcgill.ca
H. An
Affiliation:
Department of Physics, McGill University, Montreal, Canada email: vkaspi@physics.mcgill.ca
M. Bachetti
Affiliation:
IRAP/Toulouse, France
E. Bellm
Affiliation:
California Institute of Technology, USA
A. M. Beloborodov
Affiliation:
Columbia University, USA
S. Boggs
Affiliation:
University of California, Berkeley, USA
D. Chakrabarty
Affiliation:
Massachusetts Institute of Technology, USA
F. Christensen
Affiliation:
Denmark Technical University, Denmark
B. Craig
Affiliation:
University of California, Berkeley, USA Lawrence Livermore National Laboratories, USA
F. Dufour
Affiliation:
Department of Physics, McGill University, Montreal, Canada email: vkaspi@physics.mcgill.ca
F. Harrison
Affiliation:
California Institute of Technology, USA
E. V. Gotthelf
Affiliation:
Columbia University, USA
T. Kitaguchi
Affiliation:
RIKEN, Japan
C. Kouveliotou
Affiliation:
NASA/Marshall Space Flight Center, USA
K. Mori
Affiliation:
Columbia University, USA
M. Pivovaroff
Affiliation:
Lawrence Livermore National Laboratories, USA
D. Stern
Affiliation:
California Institute of Technology, USA Jet Propulsion Laboratory, USA
J. K. Vogel
Affiliation:
Lawrence Livermore National Laboratories, USA
W. Zhang
Affiliation:
NASA/Goddard Space Flight Center, USA
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Abstract

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NASA's NuSTAR observatory is the first focusing hard X-ray telescope. Launched in June 2012, NuSTAR is sensitive in the 3–79 keV range with unprecedented ~17″ FWHM angular resolution above 12 keV, a result of its multilayer-coated optics and 10-m focal length. With its large effective area (900 cm2 at 10 keV), NuSTAR has point-source sensitivity ~100 times better than previous hard X-ray telescopes. Here we describe NuSTAR and its planned work on rotation-powered pulsars and magnetars during its nominal 2-yr baseline mission that has just commenced.

Keywords

stars: neutronpulsars: generalX-rays: generalX-rays: binariestelescopes
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 331 - 336
Copyright
Copyright © International Astronomical Union 2013

References

Abdo, A. A., et al. 2010, ApJ, 720, 272Google Scholar
Archibald, A. M., et al. 2009, Science, 324, 1411Google Scholar
Archibald, A. M., et al. 2010, ApJ, 722, 88CrossRefGoogle Scholar
Baring, M. G. & Harding, A. K. 2007, ApJSS, 308, 109Google Scholar
Beloborodov, A. M. 2012, ApJ, in press, arXiv:1201.0664Google Scholar
Beloborodov, A. M. & Thompson, C. 2007, ApJ, 657, 967Google Scholar
Bogdanov, S., et al. 2011, ApJ, 742, 97Google Scholar
Burderi, L., et al. 2003, A&A, 404, L43Google Scholar
Enoto, R., et al. 2011, ApJ, 63, 387Google Scholar
Harrison, F. A., et al. 2010, SPIE, 7732, 77320SGoogle Scholar
Heyl, J. & Hernquist, L. 2005, ApJ, 618, 463CrossRefGoogle Scholar
Kargaltsev, O. Y., Pavlov, G. G., Zavlin, V. E., Romani, R. W. 2005 ApJ, 625, 307CrossRefGoogle Scholar
Kaspi, V. M. & Boydstun, K. 2010, ApJ, 710, L115Google Scholar
Kuiper, L., Hermsen, W., den Hartog, P. R., & Collmar, W. 2006, ApJ, 645, 556Google Scholar
Terada, Y., et al. 2008, PASJ, 60, 387Google Scholar