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pro vyhledávání: '"Smol'cic, V."'
Autor:
Scoville, N., Arnouts, S., Aussel, H., Benson, A., Bongiorno, A., Bundy, K., Calvo, M. A. A., Capak, P., Carollo, M., Civano, F., Dunlop, J., Elvis, M., Faisst, A., Finoguenov, A., Fu, Hai, Giavalisco, M., Guo, Q., Ilbert, O., Iovino, A., Kajisawa, M., Kartaltepe, J., Leauthaud, A., Fe`vre, O. Le, LeFloch, E., Lilly, S. J., Liu, C. T-C., Manohar, S., Massey, R., Masters, D., McCracken, H. J., Mobasher, B., Peng, Y-J., Renzini, A., Rhodes, J., Salvato, M., Sanders, D. B., Sarvestani, B. D., Scarlata, C., Schinnerer, E., Sheth, K., Shopbell, P. L., Smol'cic, V., Taniguchi, Y., Taylor, J. E., White, S. D. M., Yan, L.
Large-scale structures (LSS) out to z $< 3.0$ are measured in the Cosmic Evolution Survey (COSMOS) using extremely accurate photometric redshifts (photoz). The Ks-band selected sample (from Ultra-Vista) is comprised of 155,954 galaxies. Two technique
Externí odkaz:
http://arxiv.org/abs/1303.6689
