Table 2: Mean magnitude corrections to compensate for extended [OIII]$\lambda $5007 emission line envelopes (upper part of table) and scattered quasar Balmer emission (lower part of table). Also shown are the number of sources affected in each interval, excepting the objects for which individual corrections for [OIII] emission were made.
Emission line z-range filter correction # obj

[OIII]		 0.37-0.53 R 0.14 2

[OIII]

 0.37-0.53 I 0.15 1

[OIII]

 0.54-0.67 I 0.31 2

H$\alpha$		 0.40-0.51 I 0.12 4
H${\beta}$ 0.37-0.42 R 0.13 2
H${\beta}$ 0.58-0.73 I 0.13 9

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