Table 1.
Cluster members of MACS 1149 considered in our mass model.
| ID | RA | Dec | F160W | Sel. criterion |
|---|---|---|---|---|
| (J2000) | (J2000) | [mag] | ||
| 1 | 177.37311 | 22.39300 | 21.17 ± 0.01 | P |
| 2 | 177.37497 | 22.40452 | 23.26 ± 0.03 | P |
| 3 | 177.37618 | 22.39166 | 22.24 ± 0.01 | P |
| 4 | 177.37640 | 22.40045 | 22.26 ± 0.02 | P |
| 5 | 177.37655 | 22.40522 | 20.41 ± 0.05 | G |
| 6 | 177.37663 | 22.40207 | 23.30 ± 0.04 | P |
| 7 | 177.37692 | 22.39462 | 21.20 ± 0.01 | P |
| 8 | 177.37766 | 22.40312 | 21.18 ± 0.07 | G |
| 9 | 177.37776 | 22.39401 | 23.75 ± 0.03 | P |
| 10 | 177.37871 | 22.39281 | 22.77 ± 0.02 | P |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
Notes. Columns give, from left to right, the IDs following Table 6 of G16, right ascension, declination, and the magnitude from the HFF F160W image with the corresponding uncertainty. In the last column, we indicate whether it was selected photometrically (P), based on the WFC3-IR-GRISM redshift (G) from GLASS (Treu et al. 2016), the MUSE observations presented in G16 (M1), or in this publication (M2). This catalog is downloadable in its entirety from the web.
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