Table 2.
Similar information as in Table 2 of Barentsen et al. (2014) with values for all the survey filters.
| Filter | ⟨fλ⟩ | EW | λ0 | λp | Vega magnitude |
|
|---|---|---|---|---|---|---|
| (erg cm−2 s−1) Å−1 | (Å) | (Å) | (Å) | AB | Vega system | |
| URGO | 4.24 × 10−9 | 138.8 | 3646 | 3640 | 0.742 | 0.023 |
| g | 4.98 × 10−9 | 716.7 | 4874 | 4860 | −0.088 | 0.023 |
| r | 2.44 × 10−9 | 745.3 | 6224 | 6212 | 0.153 | 0.023 |
| Hα | 1.79 × 10−9 | 57.1 | 6568 | 6568 | 0.373 | 0.045 |
| i | 1.29 × 10−9 | 708.2 | 7677 | 7664 | 0.393 | 0.023 |
Notes. Mean monochromatic flux of Vega, filter equivalent width, mean photon and pivot wavelengths as defined in Bessell & Murphy (2012) are given, along with the calculated AB and defined Vega system magnitudes for the CALSPEC Vega spectrum stis_009 (the Vega broad band magnitude is from Bohlin 2007). We note that the catalogue data for URGO are not globally calibrated and the broad band filters g, r, and i are transformed onto the Pan-STARRS photometric system.
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