TABLE I
Emission line data for quasars. For 0537-286, set (a), in the second line, below each
wavelength, the first figure represents line to continuum ratio, and the second
deltalambda1/2 (in Å). Similarly, for set (b), the first represents Wlambda (in Å),
and the second FWHM (in Å).
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Quasar V Set 1 2 3 4 5 Source
(mag) (Å) (Å) (Å) (Å) (Å)
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0420-388 16.92 4250 5013 5100 5800 Osmer and Smith (1977)
0140-306 18.5 ~5020 6370 Smith et al. (1981)
0244-3017 19.3 ~5000 Wolstencroft et al. (1983)
0537-286 20 (a) 4238 5000 (5090) 5760 (6302) Wright et al. (1978, 1979)
0.9,(60) 1.7,(110) 1.0,(70) (1.0)
(b) 5016 5770 6371 Wilkes (1986)
176 15,58 163,258
1244+1129 18.4(J band) ~5058 Foltz et al. (1987)
1320-106 19.5 ~5000 Kunth et al. (1981)
2228.2-4033 19.6 (a) ~5046 Osmer (1979, 1980)
(b) ~5022 Vaucher et al. (1982)
Next Section: Emission Lines, Identification