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The growth of typical star forming galaxies and their super massive black holes across cosmic time since z~2

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Figure

Figure 1. Hare used in this paper (after the aplication of a stellar mass cut, seetheα luminosity distribution of the sample of Hα emitters that §2.2)and those with individually detected X-ray emission (filled histograms)
Table 1. The luminosity in the X-rays and centraldirectly detected by the C-COSMOS survey (all sources directly detectedhave luminosities higher than M˙BH for the sources 1041 erg s−1).* - These sources were taken directly from the tables of the HiZELS sur-
Figure 3are typically much lower luminosity and have lower stellar massesThere are clear detections forForthis is the smallest sample and particularly because ii) the sourcesin the z shows the results of the stacking for the four redshifts
Table 3. Number of Hα emitters classified as possible and likely AGN according to the selections mentioned in Section 3.
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