Table 1.
Parameters used in the scaling laws (Eq. 1) to estimate the stellar mass of the galaxies.
| z | a | b | Intrinsic | Reference |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| 3 | ![]() |
![]() |
0.30 dex | Lee et al. (2012) |
| 4 | ![]() |
![]() |
0.53 dex | Song et al. (2016) |
| 5 | ![]() |
![]() |
0.42 dex | Song et al. (2016) |
| 6 | ![]() |
![]() |
0.30 dex | Stefanon et al. (2021) |
| 7 | ![]() |
![]() |
0.30 dex | Stefanon et al. (2021) |
| 8 | ![]() |
![]() |
0.30 dex | Stefanon et al. (2021) |
| 9 | ![]() |
![]() |
0.30 dex | Stefanon et al. (2021) |
| 10a | ![]() |
![]() |
0.30 dex | Stefanon et al. (2021) |
Notes. (1) Redshift range z, (2) slope of the correlation a, (3) intercept coefficient b, (4) intrinsic scatter, and (5) reference for the values adopted here. As there is no published correlation for redshift 11, we used the same as for z = 10 in Stefanon et al. (2021).
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