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Table 1

Full and abbreviated names, references and SDSS apparent ugriz magnitudes of the targets.

SDSS name Short name Reference u g r i z g spec
SDSS J075059.97+141150.1 SDSS J0750 Szkody et al. (2007) 19.20 19.09 18.98 18.79 18.58 18.83
SDSS J075653.11+085831.8 SDSS J0756 Szkody et al. (2011) 16.70 16.25 16.29 16.34 16.38 17.27
SDSS J092122.84+203857.1 SDSS J0921 Szkody et al. (2009) 20.68 19.85 19.16 19.17 19.64 19.20
SDSS J092444.48+080150.9 SDSS J0924 Szkody et al. (2005) 19.49 19.25 19.26 18.70 17.88 19.36
SDSS J093537.46+161950.8 SDSS J0935 Szkody et al. (2009) 19.51 19.08 18.99 19.01 18.99 18.77
SDSS J100658.40+233724.4 SDSS J1006 Southworth et al. (2009a) 18.46 18.31 17.93 17.51 17.14 18.63
SDSS J105754.25+275947.5 SDSS J1057 Szkody et al. (2009) 19.87 19.61 19.61 19.81 19.65 19.64
CSS J112634-100210 CSS J1126 Drake et al. (2009) 18.81 18.81 18.61 18.38 18.12
SDSS J132411.57+032050.4 SDSS J1324 Szkody et al. (2004) 23.74 22.08 20.46 20.19 19.42 23.29
CSS J132536+210037 CSS J1325 Wils et al. (2010) 21.94 23.10 20.38 20.63 20.55
SDSS J133309.19+143706.9 SDSS J1333 Szkody et al. (2009) 19.11 18.48 18.15 17.94 17.90 20.95

Notes. gspec is a spectroscopic apparent magnitude calculated by convolving the SDSS flux-calibrated spectra with the g-band response function. These correspond to a different epoch to the photometric magnitudes, but may be affected by “slit losses” due to errors in astrometry or fibre positioning.

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