Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the 
origin of the Schechter function

Peng, Ying-jie; Lilly, Simon J.; Kovač, Katarina; Bolzonella, Micol; Pozzetti, Lucia; Renzini, Alvio; Zamorani, Gianni; Ilbert, Olivier; Knobel, Christian; Iovino, Angela; Maier, Christian; Cucciati, Olga; Tasca, Lidia; Carollo, C. Marcella; Silverman, John; Kampczyk, Pawel; de Ravel, Loic; Sanders, David; Scoville, Nicholas; Contini, Thierry; Mainieri, Vincenzo; Scodeggio, Marco; Kneib, Jean-Paul; Le Fèvre, Olivier; Bardelli, Sandro; Bongiorno, Angela; Caputi, Karina; Coppa, Graziano; de la Torre, Sylvain; Franzetti, Paolo; Garilli, Bianca; Lamareille, Fabrice; Le Borgne, Jean-Francois; Le Brun, Vincent; Mignoli, Marco; Montero, Enrique Perez; Pello, Roser; Ricciardelli, Elena; Tanaka, Masayuki; Tresse, Laurence; Vergani, Daniela; Welikala, Niraj; Zucca, Elena; Oesch, Pascal; Abbas, Ummi; Barnes, Luke; Bordoloi, Rongmon; Bottini, Dario; Cappi, Alberto; Cassata, Paolo; Cimatti, Andrea; Fumana, Marco; Hasinger, Gunther; Koekemoer, Anton; Leauthaud, Alexei; Maccagni, Dario; Marinoni, Christian; McCracken, Henry; Memeo, Pierdomenico; Meneux, Baptiste; Nair, Preethi; Porciani, Cristiano; Presotto, Valentina; Scaramella, Roberto

doi:10.1088/0004-637X/721/1/193

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Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

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Bongiorno, Angela
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Tanaka, Masayuki
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Hasinger, Gunther
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Peng, Y.-j., Lilly, S. J., Kovač, K., Bolzonella, M., Pozzetti, L., Renzini, A., et al. (2010). Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function. The Astrophysical Journal, 721(1), 193-221. doi:10.1088/0004-637X/721/1/193.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0012-DFFB-9

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