The evolution of the QSO luminosity function up to Z = 4 - The role of K-correction uncertainties

Mathematics – Logic

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Cosmology, Luminosity, Quasars, Spectrum Analysis, Galactic Evolution, Magnitude, Maximum Likelihood Estimates, Red Shift, Time Dependence

Scientific paper

Uncertainties in the spectral index of the optical spectrum of QSOs induce systematic biases in the estimate of the cosmological evolution of the luminosity function. In a framework of pure luminosity evolution, a slower intrinsic evolution of the luminosity function for z is less than 2.2 after correction for uncertainties in the adopted K-correction is obtained. The slower evolution is consistent with the apparent density decline of high-redshift QSOs (z is greater than 2.5) observed in the red band. It is found that a scenario of uniform luminosity evolution up to z equal to or about 4 is suggested. The apparent decline in the redshift distribution is explained in terms of the sliding down along the steep side of the luminosity function for increasing redshift.

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