Spectroscopic CCD surveys for quasars at large redshift. IV. Evolution of the luminosity function from quasars detected by their Lyman-alpha emission

Maarten Schmidt, Donald P. Schneider, James E. Gunn

Research output: Contribution to journalArticle

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Abstract

We use 90 quasars detected by their Lyα emission to well-defined flux limits in the Palomar Transit Grism Survey to derive the luminosity function of quasars in the redshift range 2.75-4.75. Application of the V/Vmax test yields 〈Ve/Va〉=0.377±0.026, corresponding to a nonuniform distribution in comoving coordinates, such that the space density decreases with redshift. The luminosity function appears to be well represented by a power law with a slope corresponding to a factor of 5.6 per magnitude. We discuss and define the relationship between the line luminosity function and the continuum luminosity function of quasars. The space density for MB<-26 decreases by a factor of 2.7 per unit redshift beyond z=2.7. Based on this result and earlier published work on quasar luminosity functions at lower redshifts, it appears that there is a maximum in the comoving space density of quasars with MB<-26 between redshifts 1.7 and 2.7.

Original languageEnglish (US)
Pages (from-to)68-77
Number of pages10
JournalAstronomical Journal
Volume110
Issue number1
StatePublished - Jul 1995

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quasars
charge coupled devices
luminosity
space density
transit
power law
slopes
continuums

All Science Journal Classification (ASJC) codes

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

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title = "Spectroscopic CCD surveys for quasars at large redshift. IV. Evolution of the luminosity function from quasars detected by their Lyman-alpha emission",
abstract = "We use 90 quasars detected by their Lyα emission to well-defined flux limits in the Palomar Transit Grism Survey to derive the luminosity function of quasars in the redshift range 2.75-4.75. Application of the V/Vmax test yields 〈Ve/Va〉=0.377±0.026, corresponding to a nonuniform distribution in comoving coordinates, such that the space density decreases with redshift. The luminosity function appears to be well represented by a power law with a slope corresponding to a factor of 5.6 per magnitude. We discuss and define the relationship between the line luminosity function and the continuum luminosity function of quasars. The space density for MB<-26 decreases by a factor of 2.7 per unit redshift beyond z=2.7. Based on this result and earlier published work on quasar luminosity functions at lower redshifts, it appears that there is a maximum in the comoving space density of quasars with MB<-26 between redshifts 1.7 and 2.7.",
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Spectroscopic CCD surveys for quasars at large redshift. IV. Evolution of the luminosity function from quasars detected by their Lyman-alpha emission. / Schmidt, Maarten; Schneider, Donald P.; Gunn, James E.

In: Astronomical Journal, Vol. 110, No. 1, 07.1995, p. 68-77.

Research output: Contribution to journalArticle

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AU - Schneider, Donald P.

AU - Gunn, James E.

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