REDSHIFTED AND BLUESHIFTED BROAD LINES IN LUMINOUS QUASARS`

摘要

We have observed a sample of 22 luminous quasars, in the range 2.0 ≈＜ z ≈＜ 2.5, at l.6 μm with the near infrared (NIR) spectrograph FSPEC on the Multiple Mirror Telescope. Our sample contains 13 radio-loud and nine radio-quiet objects. We have measured the systemic redshifts z_sys directly from the strong [O Ⅲ] λ5007 line emitted from the narrow-line region. From the same spectra, we have found that the nonresonance broad HO lines have a systematic mean redward shift of 520 ± 80 km s~(-1) with respect to systemic. Such a shift was not found in our identical analysis of the low-redshift sample of Boroson & Green. The amplitude of this redshift is comparable to half the expected gravitational redshift and transverse Doppler effects and is consistent with a correlation between redshift differences and quasar luminosity. From data in the literature, we confirm that the high-ionization rest-frame ultraviolet broad lines are blueshifted ~550-1050 km s~(-1) from systemic and that these velocity shifts systematically increase with ionization potential. Our results allow us to quantify the known bias in estimating the ionizing flux from the intergalactic medium J_v~IGM via the proximity effect. Using redshift measurements commonly determined from strong broad-line species, like Lyα or C Ⅳ λ1549, results in an overestimation of J_v~IGM by factors of ~l.9-2.3. Similarly, corresponding lower limits on the density of baryons Ω_b will be overestimated by factors of ~1.4-1.5. However, the low-ionization Mg II λ2798 broad line is within ~50 km s~(-1) of systemic and thus would