Abstract
We discuss a new method for inferring the stellar mass of a distant galaxy of known redshift based on the combination of a near-infrared luminosity and multi-band optical photometry. The typical uncertainty for field galaxies with I<22 in the redshift range 0
Cite
CITATION STYLE
APA
Brinchmann, J., & Ellis, R. S. (2000). The Mass Assembly and Star Formation Characteristics of Field Galaxies of Known Morphology. The Astrophysical Journal, 536(2), L77–L80. https://doi.org/10.1086/312738
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