ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass

MLA

Bouwens, Rychard, et al. ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected Z=2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass. 2016. EBSCOhost, https://doi.org/10.3847/1538-4357/833/1/72.

APA

Bouwens, R., Aravena, M., Decarli, R., Walter, F., da Cunha, E., Labbe, I., Bauer, F., Bertoldi, F., Carilli, C., Chapman, S., Daddi, E., Hodge, J., Ivison, R., Karim, A., Fevre, O. L., Magnelli, B., Ota, K., Riechers, D., Smail, I., … Wilkins, S. (2016). ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass. https://doi.org/10.3847/1538-4357/833/1/72

Chicago

Bouwens, Rychard, Manuel Aravena, Roberto Decarli, Fabian Walter, Elisabete da Cunha, Ivo Labbe, Franz Bauer, et al. 2016. “ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected Z=2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass.” doi:10.3847/1538-4357/833/1/72.