Similar information as in Table 2 of Barentsen et al. (2014) with values for all the survey filters.
|(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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