Autocorrelation functions for quasar absorption spectra

Details Autocorrelation functions for quasar absorption spectra Autocorrelation functions for quasar absorption spectra

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62...19v&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Jan.-Feb. 1985, p. 19-28) Soviet Astronomy (ISSN 0038-5301), vol. 29, Jan.-Feb. 1985, p. 12-

Astronomy and Astrophysics

Astronomy

1

Absorption Spectra, Astronomical Spectroscopy, Quasars, Red Shift, Autocorrelation, Wavelengths

Scientific paper

A method developed for counting line doublets in QSO spectra, autocorrelation function (ACF) analysis, has been used to single out absorption-line redshifts in quasar spectra without a reference system. The method was applied to spectroscopic data for four objects having absorption-line redshifts of less than two. These objects include: Q1226 + 105; 4C 24.61; Q0824 + 110; and Q0453 - 423. The predicted correlation peaks for lines having similar characteristics are given in a table.

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