Abstract
The isophotal wavelengths, flux densities, and AB magnitudes for Vega (alpha Lyr) are presented for the Mauna Kea Observatories near-infrared filter set. We show that the near-infrared absolute calibration for Vega determined by Cohen et al. and Megessier are consistent within the uncertainties, so that either absolute calibration may be used.
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CITATION STYLE
APA
Tokunaga, A. T., & Vacca, W. D. (2005). The Mauna Kea Observatories Near‐Infrared Filter Set. III. Isophotal Wavelengths and Absolute Calibration. Publications of the Astronomical Society of the Pacific, 117(830), 421–426. https://doi.org/10.1086/429382
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