Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE

MLA

Masters, Daniel, et al. Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE. 2014. EBSCOhost, https://doi.org/10.1088/0004-637X/785/2/153.

APA

Masters, D., McCarthy, P., Siana, B., Malkan, M., Mobasher, B., Atek, H., Henry, A., Martin, C. L., Rafelski, M., Hathi, N. P., Scarlata, C., Ross, N. R., Bunker, A. J., Blanc, G. A., Bedregal, A. G., Dominguez, A., Colbert, J., Teplitz, H., & Dressler, A. (2014). Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE. https://doi.org/10.1088/0004-637X/785/2/153

Chicago

Masters, Daniel, Patrick McCarthy, Brian Siana, Matthew Malkan, Bahram Mobasher, Hakim Atek, Alaina Henry, et al. 2014. “Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE.” doi:10.1088/0004-637X/785/2/153.