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      Galaxy clusters and groups in the ALHAMBRA survey 

      Ascaso, Begoña; Benitez, N.; Fernandez-Soto, Alberto; Arnalte-Mur, P.; López-Sanjuán, Carlos; Molino, Alberto; Schoenell, W.; Jiménez-Teja, Yolanda; Merson, Alexander I.; Huertas-Company, Marc; Díaz-García, Luis A.; Martínez, Vicent J.; Cenarro, Andres Javier; Dupke, Renato A.; Márquez, I.; Masegosa, J.; Nieves-Seoane, L.; Pović, Mirjana; Varela, Jesús; Viironen, Kerttu; Aguerri, José Alfonso López; Olmo, A. del; Moles, Mariano; Perea, Jaime D.; Alfaro, Emilio J.; Aparicio-Villegas, T.; Broadhurst, Tom J.; Cabrera Caño, Jesús María; Castander, Francisco Javier J.; Cepa, Jordi P.; Cerviño, Miguel; González Delgado, R. M.; Cristóbal-Hornillos, David (Oxford University Press, 2015)
      We present a catalogue of 348 galaxy clusters and groups with 0.2 < z < 1.2 selected in the 2.78 deg2 Advanced Large, ...
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      The ALHAMBRA survey: An empirical estimation of the cosmic variance for merger fraction studies based on close pairs 

      López-Sanjuan, C.; Cenarro, A. J.; Hernández-Monteagudo, C.; Varela, Jesús; Molino, A.; Arnalte-Mur, P.; Cabrera Caño, Jesús María (EDP Sciences, 2014)
      Aims. Our goal is to estimate empirically the cosmic variance that affects merger fraction studies based on close pairs ...
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      The ALHAMBRA survey: Bayesian photometric redshifts with 23 bands for 3 deg2 

      Molino, A.; Benítez, N.; Moles, M.; Fernández Soto, A.; Cristóbal Hornillos, D.; Ascaso, Begoña; Jiménez Teja, Y.; Schoenell, W.; Arnalte-Mur, P.; Cabrera Caño, Jesús María (Oxford University Press, 2014)
      The Advance Large Homogeneous Area Medium-Band Redshift Astronomical (ALHAMBRA) survey has observed eight different regions ...
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      The alhambra survey: evolution of galaxy spectral segregation 

      Hurtado Gil, LL.; Arnalte-Mur, P.; Martinez, V. J.; Fernández Soto, A.; Stefanon, M.; Ascaso, Begoña; López-Sanjuan, C.; Márquez, I.; Povic, M.; Viironen, Kerttu; Cabrera Caño, Jesús María (IOP Publishing Ltd., 2016-02-20)
      We study the clustering of galaxies as a function of spectral type and redshift in the range 0.35 <z <1.1 using data from ...