NIR Counterparts to Ulxs (III): Completing the Photometric Survey and Selected Spectroscopic Results
MNRAS 497, 917–932 (2020) doi:10.1093/mnras/staa1920 Advance Access publication 2020 July 7 NIR counterparts to ULXs (III): completing the photometric survey and selected spectroscopic results K. M. Lopez´ ,1,2† M. Heida ,3,4 P. G. Jonker,1,2† M. A. P. Torres,1,5,6 T. P. Roberts,7 D. J. Walton ,8 D.-S. Moon9 and F. A. Harrison4 Downloaded from https://academic.oup.com/mnras/article/497/1/917/5868255 by California Institute of Technology user on 22 October 2020 1SRON Netherlands Institute for Space Research, NL-3584 CA Utrecht, the Netherlands 2Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands 3European Southern Observatory, Karl-Schwarzschild-Straße 2, D-85748 Garching bei Munchen,¨ Germany 4Space Radiation Laboratory, California Institute of Technology, Pasadena, CA 91125, USA 5Instituto de Astrof´ısica de Canarias, E-38200 La Laguna, Tenerife, Spain 6Departamento de Astrof´ısica, Universidad de La Laguna, Astrof´ısico Francisco Sanchez´ S/N, E-38206 La Laguna, Tenerife, Spain 7Centre for Extragalactic Astronomy, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK 8Institute of Astronomy, Cambridge University, Madingley Road, Cambridge CB3 0HA, UK 9Department of Astronomy and Astrophysics, University of Toronto, Toronto, ON M5S 3H4, Canada Accepted 2020 May 31. Received 2020 May 27; in original form 2019 October 29 ABSTRACT We present results from the remaining sources in our search for near-infrared (NIR) candidate counterparts to ultraluminous X-ray sources (ULXs) within 10 Mpc. We observed 23 ULXs in 15 galaxies and detected NIR candidate counterparts to 6 of them.
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