The Lockman--SpReSO project. Main properties of infrared selected star-forming galaxies
arXiv:2404.13629 · doi:10.1051/0004-6361/202449238
Abstract
Methods.We applied distinct selection criteria to attain an SFG sample with minimal AGN contamination. Multiple approaches were used to estimate the intrinsic extinction, SFR and gas-phase metallicity for the SFGs. In conjunction with findings in the literature, we examined the correlation between SFRs and stellar masses (), as well as the metallicity evolution depending on . Finally, the 3D relationship between , SFR and metallicity, is also studied.} Results. From the initial spectroscopic sample of 409 FIR-selected objects from the Lockman--SpReSO catalogue, 69 (17\%) AGNs have been identified and excluded, which is nearly double the percentage found in local studies, leaving a sample of 340 SFGs. The analysis of the --SFR relationship revealed that Lockman--SpReSO IR-selected SFGs show signs of evolution at redshifts , shifting above the main sequence, with a mean value of dex. They are located within the starburst galaxy region since 78\% of the galaxies fall into this category. In addition, no evident flattening was found in the relation to specific SFR with redshift for . In line with the --metallicity relation (MZR) outcomes published in previous studies for optically selected SFGs, however, during the analysis of the MZR, it was found that IR-selected SFGs exhibit lower metallicities than those anticipated on the basis of their and redshift. During the investigation of the 3D --SFR--metallicity relation (FP), it was established that the research sample is consistent with relations in the existing literature, with an average scatter of dex. However, a re-calibration of the FP when using the SFR obtained from the IR luminosity is required and, in this case, no attenuation in the correlation for is observed.
arXiv comment21 pages, 17 figures, accepted in A&A
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