We present griz observations for the clusters M92, M13 and NGC 6791 and gr photometry for M71, Be 29 and NGC 7789. In addition we present new membership identifications for all these clusters, which have been observed spectroscopically as calibrators for the Sloan Digital Sky Survey (SDSS)/SEGUE survey; this paper focuses in particular on the red giant branch stars in the clusters. In a number of cases, these giants were too bright to be observed in the normal SDSS survey operations, and we describe the procedure used to obtain spectra for these stars. For M71, we also present a new variable reddening map and a new fiducial for the gr giant branch. For NGC 7789, we derived a transformation from T_eff_ to g-r for giants of near solar abundance, using IRFM T_eff_ measures of stars with good ugriz and 2MASS photometry and SEGUE spectra. The result of our analysis is a robust list of known cluster members with correctly dereddened and (if needed) transformed gr photometry for crucial calibration efforts for SDSS and SEGUE.

Cone search capability for table J/AJ/151/7/table7 (NGC 7789 Members Observed by SEGUE)

Cone search capability for table J/AJ/151/7/table4 (M13 Members Observed by SEGUE)

Cone search capability for table J/AJ/151/7/table6 (M71 Members Observed by SEGUE)

Cone search capability for table J/AJ/151/7/table1 (Cluster Properties)

Cone search capability for table J/AJ/151/7/table3 (M92 Members Observed by SEGUE)

Cone search capability for table J/AJ/151/7/table8 (NGC 6791 Members Observed by SEGUE)

Cone search capability for table J/AJ/151/7/table9 (Berkeley 29 Members Observed by SEGUE)