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2010MNRAS.409..867D - Mon. Not. R. Astron. Soc., 409, 867-872 (2010/December-1)
Understanding the shape of the galaxy two-point correlation function at z ≃ 1 in the COSMOS field.
DE LA TORRE S., GUZZO L., KOVAC K., PORCIANI C., ABBAS U., MENEUX B., CAROLLO C.M., CONTINI T., KNEIB J.P., FEVRE O.L., LILLY S.J., MAINIERI V., RENZINI A., SANDERS D., SCODEGGIO M., SCOVILLE N., ZAMORANI G., BARDELLI S., BOLZONELLA M., BONGIORNO A., CAPUTI K., COPPA G., CUCCIATI O., DE RAVEL L., FRANZETTI P., GARILLI B., IOVINO A., KAMPCZYK P., KNOBEL C., KOEKEMOER A.M., LAMAREILLE F., LE BORGNE J.-F., LE BRUN V., MAIER C., MIGNOLI M., PELLO R., PENG Y., PEREZ-MONTERO E., RICCIARDELLI E., SILVERMAN J., TANAKA M., TASCA L., TRESSE L., VERGANI D., WELIKALA N., ZUCCA E., BOTTINI D., CAPPI A., CASSATA P., CIMATTI A., FUMANA M., ILBERT O., LEAUTHAUD A., MACCAGNI D., MARINONI C., McCRACKEN H.J., MEMEO P., NAIR P., OESCH P., POZZETTI L., PRESOTTO V. and SCARAMELLA R.
Abstract (from CDS):
Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS
Journal keyword(s): galaxies: evolution - galaxies: high-redshift - galaxies: statistics - cosmology: observations - large-scale structure of Universe
Simbad objects: 1
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