Annuar, A.A.AnnuarGandhi, P.P.GandhiAlexander, D. M.D. M.AlexanderRicci, C.C.Ricci2020-09-172020-09-172015-12-01https://hdl.handle.net/20.500.13025/4153The Astrophysical Journal, Volume 815, Issue 1, article id. 36, <NUMPAGES>13</NUMPAGES> pp. (2015).We present two Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the local Seyfert 2 active galactic nucleus (AGN) and an ultraluminous X-ray source (ULX) candidate in NGC 5643. Together with archival data from Chandra, XMM-Newton, and Swift-BAT, we perform a high-quality broadband spectral analysis of the AGN over two decades in energy (˜0.5-100 keV). Previous X-ray observations suggested that the AGN is obscured by a Compton-thick (CT) column of obscuring gas along our line of sight. However, the lack of high-quality ≳10 keV observations, together with the presence of a nearby X-ray luminous source, NGC 5643 X-1, have left significant uncertainties in the characterization of the nuclear spectrum. NuSTAR now enables the AGN and NGC 5643 X-1 to be separately resolved above 10 keV for the first time and allows a direct measurement of the absorbing column density toward the nucleus. The new data show that the nucleus is indeed obscured by a CT column of N<SUB>H</SUB> ≳ 5 10<SUP>24</SUP> cm<SUP>-2</SUP>. The range of 2-10 keV absorption-corrected luminosity inferred from the best-fitting models is L<SUB>2-10,int</SUB> = (0.8-1.7) 10<SUP>42</SUP> erg s<SUP>-1</SUP>, consistent with that predicted from multiwavelength intrinsic luminosity indicators. In addition, we also study the NuSTAR data for NGC 5643 X-1 and show that it exhibits evidence of a spectral cutoff at energy E ˜ 10 keV, similar to that seen in other ULXs observed by NuSTAR. Along with the evidence for significant X-ray luminosity variations in the 3-8 keV band from 2003 to 2014, our results further strengthen the ULX classification of NGC 5643 X-1.galaxies activegalaxies nucleitechniques spectroscopicX-rays galaxiesX-rays individual NGC 5643NGC 5643 X--1NuSTAR Observations of the Compton-thick Active Galactic Nucleus and Ultraluminous X-Ray Source Candidate in NGC 564310.1088/0004-637X/815/1/36http://adsabs.harvard.edu/abs/2015ApJ...815...36A2015ApJ...815...36A