Table A.1
Decimal logarithm of the calibration coefficient for the five star formation tracers considered in this study for a Chabrier (2003) IMF between 0.1 M⊙ and 100 M⊙, each metallicity available in the Bruzual & Charlot (2003) stellar populations models, and for a constant SFR over 100 Myr and 1 Gyr.
| Z | Lyman continuum | FUV | NUV | U | TIR |
| log [M⊙ yr-1/(photons s-1)] | log [M⊙ yr-1/(W Hz-1)] | log [M⊙ yr-1/(W Hz-1)] | log[M⊙ yr-1/(W Hz-1)] | log [M⊙ yr-1/W] | |
|
|
|||||
| 10 Myr | |||||
| 0.0001 | −53.427 | −20.923 | −20.818 | −20.705 | −36.564 |
| 0.0004 | −53.301 | −20.927 | −20.825 | −20.680 | −36.503 |
| 0.004 | −53.252 | −20.910 | −20.829 | −20.760 | −36.500 |
| 0.008 | −53.198 | −20.922 | −20.845 | −20.760 | −36.486 |
| 0.02 | −53.093 | −20.905 | −20.856 | −20.771 | −36.448 |
| 0.05 | −52.924 | −20.901 | −20.878 | −20.755 | −36.422 |
|
|
|||||
| 50 Myr | |||||
| 0.0001 | −53.439 | −21.139 | −21.031 | −20.897 | −36.697 |
| 0.0004 | −53.310 | −21.127 | −21.030 | −20.892 | −36.646 |
| 0.004 | −53.256 | −21.098 | −21.027 | −20.948 | −36.640 |
| 0.008 | −53.201 | −21.093 | −21.034 | −20.956 | −36.622 |
| 0.02 | −53.095 | −21.053 | −21.021 | −20.944 | −36.578 |
| 0.05 | −52.925 | −21.015 | −21.014 | −20.920 | −36.535 |
|
|
|||||
| 100 Myr | |||||
| 0.0001 | −53.439 | −21.200 | −21.101 | −20.990 | −36.744 |
| 0.0004 | −53.310 | −21.177 | −21.088 | −20.976 | −36.689 |
| 0.004 | −53.256 | −21.144 | −21.081 | −21.020 | −36.682 |
| 0.008 | −53.201 | −21.134 | −21.084 | −21.026 | −36.662 |
| 0.02 | −53.095 | −21.090 | −21.066 | −21.008 | −36.615 |
| 0.05 | −52.925 | −21.042 | −21.049 | −20.980 | −36.569 |
|
|
|||||
| 500 Myr | |||||
| 0.0001 | −53.439 | −21.279 | −21.206 | −21.169 | −36.827 |
| 0.0004 | −53.310 | −21.247 | −21.185 | −21.162 | −36.781 |
| 0.004 | −53.256 | −21.202 | −21.160 | −21.175 | −36.771 |
| 0.008 | −53.201 | −21.182 | −21.152 | −21.166 | −36.744 |
| 0.02 | −53.095 | −21.127 | −21.123 | −21.132 | −36.693 |
| 0.05 | −52.926 | −21.064 | −21.087 | −21.086 | −36.643 |
|
|
|||||
| 1 Gyr | |||||
| 0.0001 | −53.439 | −21.296 | −21.238 | −21.242 | −36.860 |
| 0.0004 | −53.311 | −21.261 | −21.211 | −21.232 | −36.817 |
| 0.004 | −53.256 | −21.209 | −21.176 | −21.228 | −36.807 |
| 0.008 | −53.202 | −21.186 | −21.164 | −21.211 | −36.778 |
| 0.02 | −53.095 | −21.128 | −21.130 | −21.168 | −36.727 |
| 0.05 | −52.926 | −21.064 | −21.090 | −21.115 | −36.681 |
Notes. For reference, we have also included calibrations for a constant SFR over 10 Myr, 50 Myr, and 500 Myr. Calibrations on short timescales have been studied in detail in Otí-Floranes & Mas-Hesse (2010) for instance.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.