We present results of optical follow-up observations of candidate ultra-luminous X-ray sources (ULXs). Using Keck optical spectroscopy, 17 of the candidates from the Colbert & Ptak (2002) catalog have been identified; this is one of the largest sets of optical identifications of such objects thus far. 15 are background active galactic nuclei (AGN); 2 are foreground stars in our Galaxy. These findings are compared with background and foreground object expectations, as derived from log relations. Also, the results are briefly discussed in terms of the spiral-galaxy/ULX connection.
S. B. Cenko, J. S. Bloom, S. R. Kulkarni, Linda E. Strubbe, Adam A. Miller, N. Butler, R. Quimby, A. Gal‐Yam, E. O. Ofek, Eliot Quataert, Lars Bildsten, D. Poznanski, D. A. Perley, Adam Morgan, Alexei V Filippenko, D. A. Frail, I. Arcavi, Sagi Ben-Ami, A. Cucchiara, C. D. Fassnacht, Yoav Green, I. Hook, D. A. Howell, David Lagattuta, ,
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