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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
Estimating the Fuel Supply Rate on the Galactic Disk from High-velocity Cloud (HVC) Infall File

Sung, Kwang Hyun , Kwak, Kyujin

Article Issue Date2019-08 View118
GAMMA-RAY BURST AND STAR FORMATION RATES: THE PHYSICAL ORIGIN FOR THE REDSHIFT EVOLUTION OF THEIR RATIO File

Trenti, Michele , Perna, Rosalba , Tacchella, Sandro

Article Issue Date2013-08 View83
Millimeter methanol emission in the high-mass young stellar object G24.33+0.14 File

Hirota, Tomoya , Wolak, Pawel , Hunter, Todd R , Brogan, Crystal L , Bartkiewicz, Anna , Durjasz, Michal , Kobak, Agnieszka , Olech, Mateusz , Szymczak, Marian , Burns, Ross A , et al

Article Issue Date2022-10 View108
Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow File

Tacchella, Sandro , Forbes, John C. , Caplar, Neven

Article Issue Date2020-09 View61
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