Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at \(1 \le z \le 4\) from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry

We investigate the stellar and dust properties of massive (log\((M_*/M_\odot) \ge 10.5\)) and dusty (\(A_V \ge 1\)) galaxies at \(1 \le z \le 4\) by modeling their spectral energy distributions (SEDs) obtained from the combination of UltraVISTA DR3 photometry and \textit{Herschel} PACS-SPIRE data using MAGPHYS. Although the rest-frame U-V vs V-J (UVJ) diagram traces well the star-formation rates (SFR) and dust obscuration (A\(_V\)) out to \(z \sim 3\), \(\sim\)15-20\% of the sample surprisingly resides in the quiescent region of the UVJ diagram, while \(\sim50\)\% at \(3