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SDSS name | Short name | Reference | u | g | r | i | z |
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SDSS J031051.66-075500.2 | SDSS J0310 | Szkody et al. (2003) | 15.76 | 15.49 | 15.74 | 15.89 | 16.10 | 22.03 |
SDSS J074355.55+183834.8 | SDSS J0743 | Szkody et al. (2006) | 20.11 | 20.07 | 19.29 | 18.78 | 18.61 | 21.66 |
SDSS J074640.61+173412.7 | SDSS J0746 | Szkody et al. (2006) | 18.21 | 18.16 | 18.37 | 18.52 | 18.55 | 21.20 |
SDSS J075059.97+141150.1 | SDSS J0750 | Szkody et al. (2007) | 19.20 | 19.09 | 18.98 | 18.79 | 18.58 | 18.83 |
SDSS J075808.81+104345.5 | SDSS J0758 | Szkody et al. (2009) | 17.06 | 16.92 | 17.07 | 17.17 | 17.25 | 17.06 |
SDSS J090628.24+052656.9 | SDSS J0906 | Szkody et al. (2005) | 18.82 | 18.76 | 18.46 | 18.10 | 17.82 | 19.32 |
SDSS J092444.48+080150.9 | SDSS J0924 | Szkody et al. (2005) | 19.49 | 19.25 | 19.26 | 18.70 | 17.88 | 19.36 |
SDSS J115207.00+404947.8 | SDSS J1152 | Szkody et al. (2007) | 19.22 | 19.26 | 19.15 | 19.13 | 19.00 | 19.56 |
SDSS J152419.33+220920.1 | SDSS J1524 | Szkody et al. (2009) | 19.04 | 19.04 | 18.90 | 18.80 | 18.50 | 19.52 |
Notes.
is an apparent magnitude calculated by convolving the SDSS flux-calibrated spectra with the g passband function. These represent a different epoch to the SDSS ugriz magnitudes, but may be affected by ``slit losses'' due to any errors in astrometry or positioning of the fibre entrance.
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