Table 3.
Cylindrical projected X-ray luminosity using the M1 mask.
| Sample | log10(Mvir) | S/N | LX [1040 erg s−1] | ||||
|---|---|---|---|---|---|---|---|
| name | halo | 80 | 300 | XRB | max PS | Rp < 80 kpc | Rp < 300 kpc |
| ALL_M10.7 | 12.2 | 5.2 | 2.3 | 1.1 |
2.8 | 2.8 ± 0.5 | 15.4 ± 6.6 |
| Fixed stellar mass selection | |||||||
| QU_M10.7 | 12.2 | 7.3 | 4.3 | 0.6 |
3.1 | 4.0 ± 0.5 | 28.7 ± 6.6 |
| SF_M10.7 | 12.2 | 3.6 | 0.9 | 1.4 |
2.6 | 1.9 ± 0.5 | 5.7 ± 6.7 |
| Quiescent galaxies | |||||||
| QU_M11.71 | 15.0 | 10.9 | 10.3 | 7.1 |
92.2 | 82.2 ± 7.6 | 440.7 ± 42.6 |
| QU_M11.58 | 14.5 | 8.5 | 7.5 | 5.3 |
78.0 | 70.0 ± 8.2 | 314.3 ± 42.1 |
| QU_M11.54 | 14.4 | 3.9 | 5.0 | 4.8 |
24.8 | 22.3 ± 5.7 | 174.1 ± 35.0 |
| QU_M11.35 | 13.8 | 8.6 | 7.0 | 3.0 |
17.1 | 14.9 ± 1.7 | 87.5 ± 12.5 |
| QU_M11.2 | 13.2 | 8.4 | 4.4 | 2.1 |
10.0 | 8.9 ± 1.1 | 40.5 ± 9.2 |
| QU_M11.04 | 12.8 | 6.3 | 4.5 | 1.5 |
3.7 | 5.0 ± 0.8 | 36.7 ± 8.2 |
| QU_M10.88 | 12.5 | 6.1 | 5.2 | 1.0 |
3.8 | 4.6 ± 0.8 | 41.5 ± 8.0 |
| QU_M10.73 | 12.3 | 5.7 | 3.1 | 0.7 |
2.9 | 3.9 ± 0.7 | 22.4 ± 7.2 |
| QU_M10.53 | 12.0 | 5.5 | 3.5 | 0.4 |
2.4 | 3.2 ± 0.6 | 22.5 ± 6.4 |
| Star-forming galaxies | |||||||
| SF_M11.25 | 13.4 | 3.3 | 1.7 | 4.0 |
10.3 | 5.7 ± 1.7 | 21.8 ± 12.7 |
| SF_M11.12 | 13.0 | 2.5 | 1.5 | 3.1 |
7.9 | 4.1 ± 1.6 | 18.8 ± 12.2 |
| SF_M11.05 | 12.8 | 2.4 | 1.7 | 2.6 |
4.8 | 3.7 ± 1.6 | 20.6 ± 11.9 |
| SF_M10.99 | 12.7 | 3.5 | 1.3 | 2.4 |
5.3 | 3.7 ± 1.0 | 12.1 ± 9.1 |
| SF_M10.9 | 12.5 | 3.2 | 1.2 | 2.0 |
3.3 | 3.1 ± 1.0 | 10.1 ± 8.7 |
| SF_M10.86 | 12.4 | 3.0 | 1.1 | 1.9 |
3.5 | 2.3 ± 0.8 | 8.5 ± 7.7 |
| SF_M10.74 | 12.3 | 2.8 | 0.6 | 1.6 |
3.3 | 2.1 ± 0.7 | 4.3 ± 7.5 |
| SF_M10.63 | 12.1 | 2.8 | 0.7 | 1.3 |
3.1 | 2.0 ± 0.7 | 5.3 ± 7.3 |
| SF_M10.52 | 12.0 | 1.8 | 0.6 | 1.2 |
0.8 | 1.2 ± 0.7 | 4.2 ± 7.0 |
| SF_M10.41 | 11.9 | 2.5 | 0.8 | 1.0 |
1.5 | 1.6 ± 0.7 | 5.8 ± 6.9 |
| SF_M10.3 | 11.8 | 1.9 | 0.5 | 0.9 |
1.8 | 1.2 ± 0.6 | 3.4 ± 6.5 |
| SF_M10.18 | 11.8 | 2.9 | −0.0 | 0.7 |
1.3 | 1.7 ± 0.6 | −0.2 ± 6.2 |
| SF_M10.03 | 11.6 | 2.1 | 0.5 | 0.6 |
1.4 | 1.1 ± 0.5 | 2.8 ± 5.9 |
| SF_M9.86 | 11.5 | −0.2 | −0.4 | 0.4 |
0.3 | −0.1 ± 0.4 | −2.3 ± 5.3 |
| SF_M9.64 | 11.4 | 1.3 | 0.3 | 0.3 |
0.3 | 0.5 ± 0.4 | 1.5 ± 4.8 |
Notes. Cylindrical projected luminosity in units of 1040 erg s−1 measured within projected distances of 80 and 300 kpc for each sample with the M1 mask. In the column S/N we report the S/N of the measurement. We consider to have a “detection” when the S/N is larger than 3, a “hint of detection” if the S/N is between 1 and 3, and an “upper limit” when the S/N is smaller than 1. These are compared with the XRB model prediction of Aird et al. (2017). “max PS” is the luminosity obtained when integrating the point-source profiles (gray lines in the figures), which constitutes an upper limit to the luminosity that can be attributed to point-source emission. log10(Mvir) is the estimated mean halo mass obtained using the stellar to halo mass relation from Moster et al. (2013). Table 4 reports the same quantities as obtained when applying the ‘M3’ mask.
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