Table 2.
Number of galaxies in our sample after each cut is made.
| z, M* | sSFR | AGN | |
|---|---|---|---|
| Mass sample detections (z < 0.4, M* > 1010.05) | 3464 | 2417 | 2353 |
| Mass sample limits (z < 0.4, M* > 1010.05) | 10 447 | 1798 | |
| Redshift sample detections (z < 1.0, M* > 1010.45) | 10 046 | 7190 | 6856 |
| Redshift sample limits (z < 1.0, M* > 1010.45) | 41 763 | 9784 | |
Notes. Each column shows the number of galaxies in our sample after each successive cut is made. The cuts are made in z, M* plane, sSFR, and to remove AGN. The two rows for each sample show the detections at 150 MHz and limits at 150 MHz. There is no number in the AGN column for the limits because AGN are excluded automatically based on their MAGPHYSχ2 flag which identifies bad fits, making it impossible to identify which of those galaxies are AGN.
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