The VIMOS Public Extragalactic Redshift Survey (VIPERS) ⋆ Luminosity and stellar mass dependence of galaxy clustering at 0.5< z< 1.1

@article{Marulli2013TheVP,
  title={The VIMOS Public Extragalactic Redshift Survey (VIPERS) ⋆ Luminosity and stellar mass dependence of galaxy clustering at 0.5< z< 1.1},
  author={F. Marulli and M. Bolzonella and E. Branchini and I. Davidzon and S. L. Torre and B. Granett and L. Guzzo and A. Iovino and L. Moscardini and A. Pollo and U. Abbas and C. Adami and S. Arnouts and J. Bel and D. Bottini and A. Cappi and J. Coupon and O. Cucciati and G. Lucia and A. Fritz and P. Franzetti and M. Fumana and B. Garilli and O. Ilbert and J. Krywult and V. Brun and O. F{\`e}vre and D. Maccagni and K. Małek and H. Mccracken and L. Paioro and M. Polletta and H. Schlagenhaufer and M. Scodeggio and L. Tasca and R. Tojeiro and D. Vergani and A. Zanichelli and A. Burden and C. D. Porto and A. Marchetti and C. Marinoni and Y. Mellier and R. Nichol and J. Peacock and W. Percival and S. Phleps and M. Wolk and G. Zamorani},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={557},
  pages={1-15}
}
Aims. We investigate the dependence of galaxy clustering on luminosity and stellar mass in the redshift range 0.5 < z < 1.1, using the first ~ 55 000 redshifts from the VIMOS Public Extragalactic Redshift Survey (VIPERS). Methods. We measured the redshift-space two-point correlation functions (2PCF), ξ(s) and ξ(rp,π) , and the projected correlation function, wp(rp), in samples covering different ranges of B-band absolute magnitudes and stellar masses. We considered both threshold and binned… Expand
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The VIMOS Public Extragalactic Redshift Survey (VIPERS) - Hierarchical scaling and biasing
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