Abstract
Photometric and spectroscopic observations of PC 1158 + 4635, a quasar
with a redshift of 4.73, are presented. This object was discovered by
the detection of its Ly-alpha emission line in a low-resolution CCD
grism survey. The apparent magnitude of the quasar is r = 20.2; its
absolute magnitude is similar to that of 3C 273 (for q0 = 0.5). The
spectrum of PC 1158 + 4635 reveals prominent emission lines of Ly-alpha
and C IV and a sharp, approximately one magnitude drop in the continuum
level across the Ly-alpha emission line (features seen in most greater
than 4 quasars). The redshift-continuum depression relation for quasars
requires a dramatic change in the 'Lymann alpha clouds' (either in
number or intrinsic properties) at a redshift of about 3.5 or else the
presence of a new source that is responsible for the majority of the
absorption at redshifts obove four.
Original language | English (US) |
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Pages (from-to) | 1951-1958 |
Journal | Astronomical Journal |
Volume | 98 |
DOIs | |
State | Published - Dec 1 1989 |
Externally published | Yes |