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    /nge cle="="bold">Acceptin: t/jge >16 November ati6//p> /" contenaanrxt/aoAlt;i>t/p>f="="="="/p>is worμstSouth (ADF-S) survey. In particular, we want to estimate the active galactic nucleus (AGN) contribution to the LIRGs and ULIRGs’ infrared emission and whi’types of AGNs are related to their activity.<i>Methods. <i/>Wt/p>f="="="="/p>d 69 gala≥t/jge >μ<i/>m by the/nge cle="="sivele-math">μstSADF-S, with optical counterparts and spectral coverage from the ultraviolet to the FIR. We used two independent spectral energy distribution fitting codes: one fitting the SED from FIR to FUV (CIGALE) (we use the results from CIGALE as a reference) and gray-body + power spectrum fit for the infrared part of the spectra (CMCIRSED) in order to identify a subsample of ULIRGs and LIRGs, and to estimate their properties.<i>Results. <i/>Bt/p>f="="="="/p>he CIGALEμstr sample (we found /nge cle="="sivele-math">~t/jge >7 ULIRGs and 22 LIRGs, spanning over the redshift range 0.06 <<i>z<i/>< /nge cle="="sivele-math"><t/jge >/nge cle="="sivele-math">z/nge cle="="sivele-math"><t/jge >ters, such as stellar mass, star formation rate (SFR), and specific SFR are consistent with the ones found for other samples selected at infrared wavelengths. We have detected a significant AGN contribution to the mid-infrared luminosity for 63% of LIRGs and ULIRGs. Our LIRGs contain Type 1, Type 2, and intermediate types of AGN, where_r masmission and whurveywhere_r masmissionima2K to estimate0'hcy,50%) their iGNs are rto gintypeand grs of Ativitsuch css" thture-nd ULIRGs. ies.&ss" thture-R), t;i>re s spectra dust /js/artic theiDF–S the 90 <i>ist2/01eed at traset;i>re s founshaps a ADF-S,dust R), t <nota ADF-S,incere_s adust heas anBt/p>f="="="="/p>Concluare ala±t/jge >t3%veywhere_r AKA K to eststimate thntermediate t2whursnd speccA masmn fraf of re requr my f19 /nge cle="="sivele-math">±t/jge >t8%Bt/p>f="="=""div cle="="kve"> >/p>Keyicalds: t/jge >me="citation_key /types of tation_key /tme="citatitation_key /tme="citatiion_art//pxt/div>
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