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Table 3:

The stars from the SDSS survey observed during this programme, excluding the pulsators listed in Table 4.
Name g' Class \ensuremath {T_{\rm {eff}}} \ensuremath{\log g} \ensuremath{\log y}
  mag   kK dex dex
PB 59161 15.3 sdB 30.1 5.7 -2.3
PG 0812+4822 15.0 sdB 25.0 5.4 -3.0
PG 0826+4802 15.8 sdB 26.1 5.5 -3.1
PG 1100-0082 16.3 sdB+ 29.2 5.5 -2.6$^{\dag }$
PG 1136-0031,2 14.2 sdB 31.6 5.6 -2.7
PG 1249+0281,2,3 15.4 sdB 30.6 5.6 -3.0
J12596-00394 16.8 sdOB+ 34.4 5.6 -2.2$^{\dag }$
PG 1315+0131,2 16.6 sdB 26.6 5.3 -2.3
J13320+67334 17.0 sdOB 36.1 6.0 -1.1
J13516+02341 17.1 sdB+ 34.7 5.3 -3.0$^{\dag }$
PG 1403+0191,2 15.6 sdB 27.7 5.5 -1.9
J14086+65311 17.4 sdB 30.4 5.6 -3.0
J14236+01491 17.1 sdB 29.5 5.7 -2.3
PG 1422+0352 16.2 sdOB 35.1 5.8 -1.5
J15107+04094 16.9 sdOB 34.7 5.7 -1.6
J15131+01141 17.1 sdB 28.0 5.6 -3.0
EGGR 4911,5 16.8 sdB 30.6 5.6 -3.0
SBSS 1544+5681 16.8 sdB 27.2 5.2 -2.0
J15481-00491 16.4 sdB+ 32.7 5.6 -3.0$^{\dag }$
J15513+0649 15.9 sdOB+ 34.3 5.0 -2.1$^{\dag }$
J15564+01131 16.0 sdB 30.7 5.7 -3.1
J16026-00121 17.5 sdB 34.0 5.8 -2.1
J16165-00381 16.7 sdOB 36.0 5.7 -1.8
J16331+00321 16.9 sdB 31.7 5.8 -3.3
J16347-00531 16.9 sdB 29.1 5.5 -2.7
J16420+44031 16.7 sdB 28.8 5.2 -2.8
J16443+45231 17.1 sdB 33.1 5.8 -2.0
PG 1653+6331,2 15.9 sdOB 36.1 5.9 -1.5
J17144+61471 16.6 sdB+ 33.4 5.6 -3.4$^{\dag }$
SBSS 1715+5561,6 16.9 sdB 30.3 5.4 -3.2
J17165+57514 18.0 sdOB 34.9 5.8 -0.8
J20440-05111 17.3 sdB 29.9 5.4 -3.2
J20457-05431 17.8 sdB 34.9 5.4 -1.7
J20573-06261 16.5 sdB 28.0 5.1 -2.5
J21531-07191 16.9 sdB 32.0 5.9 -2.0

Notes. The columns are as in Table 2, except that Sloan g' magnitudes are provided provided as indicator of the signal level. A plus sign after the class marks the presence of a cool companion from features in the spectrum, the slope of the spectrum or z-band excess. The notes indicate:
(1) Correctly identified as sdB stars in Eisenstein et al. (2006).
(2) Classified as hot subdwarf stars in Green et al. (1986).
(3) Object misnamed in the PG catalog; should be PG 1249-027.
(4) Listed as sdO stars in Eisenstein et al. (2006).
(5) Misclassified as a white dwarf in McCook & Sion (1987).
(6) Identified as an sdB star in Stepanian et al. (2001).
$^{(\dag )}$ Parameters for composites are less certain than for singles.


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