A Foreground Masking Strategy for [C ii] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift.

MLA

G. Sun, et al. “A Foreground Masking Strategy for [C Ii] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift.” Astrophysical Journal, vol. 856, no. 2, Apr. 2018, p. 1. EBSCOhost, https://doi.org/10.3847/1538-4357/aab3e3.

APA

G. Sun, L. Moncelsi, M. P. Viero, M. B. Silva, J. Bock, C. M. Bradford, T.-C. Chang, Y.-T. Cheng, A. R. Cooray, A. Crites, S. Hailey-Dunsheath, B. Uzgil, J. R. Hunacek, & M. Zemcov. (2018). A Foreground Masking Strategy for [C ii] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift. Astrophysical Journal, 856(2), 1. https://doi.org/10.3847/1538-4357/aab3e3

Chicago

G. Sun, L. Moncelsi, M. P. Viero, M. B. Silva, J. Bock, C. M. Bradford, T.-C. Chang, et al. 2018. “A Foreground Masking Strategy for [C Ii] Intensity Mapping Experiments Using Galaxies Selected by Stellar Mass and Redshift.” Astrophysical Journal 856 (2): 1. doi:10.3847/1538-4357/aab3e3.