A 370  1z(photo) = .138; observed redshift is suprisingly large.  However,
A 370  2photometric redshift formula probably can not be extrapolated to red-
A 370  3shifts this large.
A 465  1May be foreground galaxy; z(photo) = .155.
A 480  1May be foreground galaxy; z(photo) = .132.
A 509  1Alternative redshift is z = .0836 (KUC) for one galaxy; chosen value
A 509  2agrees slightly better with z(photo) = .147.
A 514  1z = .0348 radio galaxy (N) is probably foreground; chosen value agrees
A 514  2better with z(photo) = .066.
A 680  1May be foreground galaxy; z(photo) = .172.
A 695  1May be foreground galaxy; z(photo) = .152.
A1216  1z = .0237 radio galaxy (N) is probably foreground; chosen value agrees
A1216  2better with z(photo) = .070.
A1232  1Alternative redshift is z = .1997 (HGT) for one galaxy; chosen value
A1232  2agrees better with z(photo) = .148.
A1246  1Incorrectly identified as A1245 in (N).
A1254  1This cluster is in a confused region.  Alternative redshift is z = .0439
A1254  2(HSM) for one galaxy; chosen value agrees better with z(photo) = .123,
A1254  3although both may be foreground galaxies.  The HGT galaxy is 30 arcmin
A1254  4from cluster center.  Note that the m1 given by LvdB is probably for a
A1254  5foreground galaxy, and that Abell (1982) has revised his m10 upward,
A1254  6suggesting that the cataloged cluster is more distant that the fore-
A1254  7ground groups.  z(photo) is from equation 4.
A1318  1May be foreground galaxy; z(photo) = .038.
A1337  1Alternative redshift is z = .0826 (PL) for two galaxies; chosen value
A1337  2agrees better with z(photo) = .130.
A1342  1Alternative redshift is z = .1516 (PL) for two galaxies; chosen value
A1342  2agrees better with z(photo) = .110.
A1354  1z = .0201 galaxy (N) is probably foreground; chosen value agrees
A1354  2better with z(photo) = .131.
A1356  1Alternative redshift is z = .0699 (PL) for two galaxies; chosen value
A1356  2agrees better with z(photo) = .132.
A1385  1Alternative redshift is z = .0832 (PL) for two galaxies; z(photo) = .113
A1385  2does not usefully discriminate between the two values.
A1399  1Confused with poor cluster MKW-3 by N.
A1541  1The LvdB z(photo) = .047 is low because their m1 is a foreground galaxy.
A1631  1The LvdB z(photo) = .034 is low because their m1 is probably a fore-
A1631  2ground galaxy.
A1667  1Alternative redshift z = .0951 (N) for 5 galaxies probably applies to
A1667  2the group around B264; chosen value agrees better with z(photo) = .161.
A1759  1Two cluster centers (A1759, A1760) are only 3.5 arcmin apart; probably
A1759  2only one cluster.
A1760  1Two cluster centers (A1759, A1760) are only 3.5 arcmin apart; probably
A1760  2only one cluster.
A1878  1z(photo) = .138; observed redshift is surprisingly large.  However,
A1878  2photometric redshift formula probably can not be extrapolated to
A1878  3redshifts this large.
A2001  1Alternative redshift is z = .1755 (Mea) for two galaxies; chosen value
A2001  2agrees better with z(photo) = .125.
A2084  1z(photo) = .157; observed redshift is surprisingly large.  However,
A2084  2photometric redshift formula probably can not be extrapolated to
A2084  3redshifts this large.
A2151  1Probably two clusters.  Mean redshift is given; individual redshifts
A2151  2are .0383 and .0365.
A2152  1Part of Hercules supercluster, a very confused region.  Alternative
A2152  2redshift for only two brightest galaxies is z = .0448 (HSM); chosen
A2152  3value agrees better with z(photo) = .030.
A2177  1Alternative redshift is z = .0769 (KUC) for one galaxy; chosen value
A2177  2agrees better with z(photo) = .133.
A2241  1Two clusters; smaller redshift, which agrees better with photometric
A2241  2redshift z = .056, is given.  Larger redshift is z = .1021 for three
A2241  3galaxies.
A2255  1May be two clusters (see Tarenghi and Scott 1976, Astrophys. J. 207, L9)
A2319  1Probably two clusters; the lower redshift is given.  Larger redshift is
A2319  2z = .0634 (N) for 9 galaxies.
A2355  1Alternative redshift is z = .1244 (KUC) for two galaxies; chosen value
A2355  2agrees better with z(photo) = .219.
A2440  1Alternative redshifts are z = .057 for the radio galaxy 3C 445 (C) which
A2440  2may be a foreground galaxy, and z = .1121 (HSM) based on only one line
A2440  3from one galaxy; z(photo) = .069 does not usefully discriminate between
A2440  4the two lower values.
A2638  1May be foreground galaxy; z(photo) = .184.
A2645  1Alternative redshift is z = .186 (N) for two galaxies; chosen value
A2645  2agrees better with z(photo) = .238.