Abstract
Four quasars with redshifts greater than four were detected in a
low-resolution CCD grism survey. CCD photometry and high S/N, moderate
resolution spectra are presented for these quasars and the six other
known quasars with redshifts above 4. The MB values of nine
of the objects are between -27.5 and -25, with the tenth quasar having
an MB value of -29. The emission lines and shapes of the
continua of these ten quasars are similar to those of lower-redshift
quasars. The results suggest that the C IV emission lines in
high-redshift quasars may be weaker than those in lower-redshift
quasars. The continua of all of the high-redshift quasars display strong
depressions blueward of the Ly-alpha emission line.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1507-1522 |
| Journal | Astronomical Journal |
| Volume | 98 |
| DOIs | |
| State | Published - Nov 1 1989 |
| Externally published | Yes |
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