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The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities

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Academic year: 2021

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Fig. 1. Redshift distribution of total GMASS sample at z ≥ 1 with either spectroscopic or photometric redshift (grey); GMASS sample at z spec ≥ 1 with reliable spectroscopic redshift (green); preliminary sample of 327 SF+mixed galaxies (salmon); final samp
Fig. 2. From top to bottom: a) average spectrum of 33 quiescent galaxies in the GMASS sample; b) average spectrum of mixed galaxies in the [OII] sample, at 1 &lt; z &lt; 1.6; c) average spectrum of not-mixed SFGs in the [OII] sample, at 1 &lt; z &lt; 1.6
Fig. 4. Continuum indices distribution over the [OII] sample: MgUV, C(29 − 33), D4000
Table 1. Summary table of the general properties (spectral classes, X-ray and IR detections) of the GMASS spectroscopic sample at z spec ≥ 1.
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