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We have studied the nuclear region of the previously detected dual AGN systemin the galaxy pair IRAS 05589+2828 and 2MASX J06021107+2828382 through newoptical spectroscopy observations, along with radio and X-ray archival data.Our multiwavelength data strongly suggest that the Sy1 \iras\,(z=0.0330$\pm$0.0002) conforms to a dual AGN system with the Sy2 \twomas\,(z=0.0334$\pm$0.0001) with a projected separation obtained from the radio dataof 20.08\arcsec\, ($\sim$13.3\,kpc). Analysis of the optical spectra reveals afaint narrow extended emission from H$\alpha$ and [OIII] amidst the two AGN,supporting evidence for an ongoing merger. \iras\, is a double component narrowemission line AGN, with complex broad Balmer emission line profiles thatclearly show a strong red-peaklet with a velocity shift of$\sim$3500\,km\,s$^{-1}$. The black hole mass estimates of \iras\, and\twomas\, are log\,M$\rm_{BH}$\,=\,8.59\,$\pm$\,0.14 (M$_\odot$) andlog\,M$\rm_{BH}$\,=\,8.21$\pm$0.2 (M$_\odot$), respectively. In the X-raybands, \iras\, is compatible with a Type 1 object, showing both spectral andflux variability. \chandra\, data of 2MASX\,J06021107+2828382 allowed us tomeasure a high hardness ratio in this source, providing evidence for a Type 2AGN. The 22 GHz image obtained with the {\it Karl G. Jansky Very Large Array}has revealed that both AGN are compact radio objects with spectral indices-0.26$\pm$0.03 and -0.70$\pm$0.11, confirming for the first time its dual AGNnature in the radio bands.

Unravelling the nature of the dual AGN in the galaxy pair system IRAS 05589+2828 and 2MASX J06021107+2828382