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Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering

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 نشر من قبل Daniel Farrow Dr
 تاريخ النشر 2015
  مجال البحث فيزياء
والبحث باللغة English
 تأليف D. J. Farrow




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We measure the projected 2-point correlation function of galaxies in the 180 deg$^2$ equatorial regions of the GAMA II survey, for four different redshift slices between z = 0.0 and z=0.5. To do this we further develop the Cole (2011) method of producing suitable random catalogues for the calculation of correlation functions. We find that more r-band luminous, more massive and redder galaxies are more clustered. We also find that red galaxies have stronger clustering on scales less than ~3 $h^{-1}$ Mpc. We compare to two differe



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