“School of Astronomy”
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| Paper IPM / Astronomy / 12901 |
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Flux Autocorrelation function is useful utile to explain the Lyman alpha forest. Measuring the flux autocorrelation function in the Lyman alpha forest will be done, using UVES high resolution spectrum of some quasars at 2.6<zem<3.8. We will investigate the redshift dependency of the flux autocorrelation function.
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