A model for the infrared-radio correlation of main-sequence galaxies at GHz frequencies and its dependence on redshift and stellar mass

MLA

Schober, J., et al. A Model for the Infrared-Radio Correlation of Main-Sequence Galaxies at GHz Frequencies and Its Dependence on Redshift and Stellar Mass. Jan. 2022. EBSCOhost, https://doi.org/10.48550/arxiv.2210.07919.

APA

Schober, J., Sargent, M. T., Klessen, R. S., & Schleicher, D. R. G. (2022). A model for the infrared-radio correlation of main-sequence galaxies at GHz frequencies and its dependence on redshift and stellar mass. https://doi.org/10.48550/arxiv.2210.07919

Chicago

Schober, J., M. T. Sargent, R. S. Klessen, and D. R. G. Schleicher. 2022. “A Model for the Infrared-Radio Correlation of Main-Sequence Galaxies at GHz Frequencies and Its Dependence on Redshift and Stellar Mass,” January. doi:10.48550/arxiv.2210.07919.