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A PHYSICAL MODEL FOR THE 0 less than or similar to z less than or similar to 8 REDSHIFT EVOLUTION OF THE GALAXY ULTRAVIOLET LUMINOSITY AND STELLAR MASS FUNCTIONS File File

Tacchella, Sandro , Trenti, Michele , Carollo, C. Marcella

Article Issue Date2013-05 View96
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z greater than or similar to 4 File

Tacchella, Sandro , Bose, Sownak , Conroy, Charlie , Eisenstein, Daniel J. , Johnson, Benjamin D.

Article Issue Date2018-12 View57
(Re)Solving reionization with Ly alpha: how bright Ly alpha Emitters account for the z approximate to 2-8 cosmic ionizing background File File

Matthee, Jorryt , Naidu, Rohan P , Pezzulli, Gabriele , Gronke, Max , Sobral, David , Oesch, Pascal A , Hayes, Matthew , Erb, Dawn , Schaerer, Daniel , Amorín, Ricardo , et al

Article Issue Date2022-04 View78
The SINS/zC-SINF Survey of z similar to 2 Galaxy Kinematics: SINFONI Adaptive Optics-assisted Data and Kiloparsec-scale Emission-line Properties File

Schreiber, N. M. Foerster , Renzini, A. , Mancini, C. , Genzel, R. , Bouche, N. , Cresci, G. , Hicks, E. K. S. , Lilly, S. J. , Peng, Y. , Burkert, A. , et al

Article Issue Date2018-10 View80
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