Ricci, C.Bauer, F. E.Treister, E.Romero-Cañizales, C.Arevalo, P.Iwasawa, KazushiPrivon, G. C.Sanders, D. B.Schawinski, K.Stern, D.Imanishi, Masatoshi2019-10-102019-10-102016-03-010004-637Xhttps://hdl.handle.net/2445/142103We report the detection of a heavily obscured active galactic nucleus (AGN) in the luminous infrared galaxy (LIRG) NGC 6286 identified in a 17.5 ks Nuclear Spectroscopic Telescope Array observation. The source is in an early merging stage and was targeted as part of our ongoing NuSTAR campaign observing local luminous and ultra-luminous infrared galaxies in different merger stages. NGC 6286 is clearly detected above 10 keV and by including the quasi-simultaneous Swift/XRT and archival XMM-Newton and Chandra data, we find that the source is heavily obscured (NH sime(0.95−1.32) × 1024 cm−2) with a column density consistent with being Compton-thick (CT, $\mathrm{log}({N}_{{\rm{H}}}/{\mathrm{cm}}^{-2})\geqslant 24$). The AGN in NGC 6286 has a low absorption-corrected luminosity (L2−10 keV ~ 3−20 × 1041 erg s−1) and contributes lesssim1% to the energetics of the system. Because of its low luminosity, previous observations carried out in the soft X-ray band (<10 keV) and in the infrared did not notice the presence of a buried AGN. NGC 6286 has multiwavelength characteristics typical of objects with the same infrared luminosity and in the same merger stage, which might imply that there is a significant population of obscured low-luminosity AGNs in LIRGs that can only be detected by sensitive hard X-ray observations.13 p.application/pdfeng(c) American Astronomical Society, 2016Galàxies activesRaigs XActive galaxiesX-raysinfo:eu-repo/semantics/article6699692019-10-10info:eu-repo/semantics/openAccess