EPJ Web of Conferences (Jan 2014)

The NuSTAR ULX program

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

DOI
https://doi.org/10.1051/epjconf/20136406010
Journal volume & issue
Vol. 64
p. 06010

Abstract

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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.