The NuSTAR ULX program

William W. Zhang, Daniel Stern, William W. Craig, Michael Parker, Guido Risaliti, Steven E. Boggs, Charles J. Hailey, Brian W. Grefenstette, Karl Forster, Finn Erland Christensen, Jon M. Miller, Fiona A. Harrison, Felix Fürst, Natalie A. Webb, Ann E. Hornschemeier, Didier Barret, Andrew C. Fabian, Vikram R. Rana, Kristin K. Madsen, Andrew PtakMatteo Bachetti, Dominic J. Walton

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    Abstract

    We present the results of the first large program of broadband ULX observations with NuSTAR, XMM-Newton and Suzaku, yielding high-quality spectra and timing measurements from 0.3-30 keV in 6 ULXs, providing powerful information for understanding the accretion modes and nature of the central BHs. In particular, we find that all ULXs in our sample have a clear cutoff above 10 keV. This cutoff is less pronounced than expected by Comptonization from a cold, thick corona. We confirm the presence of a soft excess at low energies in the brightest ULXs, with temperatures below ~ 0.5 keV. We make an estimates on the masses of several ULXs based on spectral variability and model fitting. © 2014 Owned by the authors.
    Original languageEnglish
    Article number06010
    JournalE P J Web of Conferences
    Volume64
    Number of pages4
    ISSN2100-014X
    DOIs
    Publication statusPublished - 2014

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