NuSTAR observations of rotation-powered pulsars and magnetars

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Abstract

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. © 2013 International Astronomical Union.

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Kaspi, V. M., An, H., Bachetti, M., Bellm, E., Beloborodov, A. M., Boggs, S., … Zhang, W. (2012). NuSTAR observations of rotation-powered pulsars and magnetars. In Proceedings of the International Astronomical Union (Vol. 8, pp. 331–336). https://doi.org/10.1017/S1743921312024027

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