``The Mauna Kea Observatories Near-Infrared Filter Set. III. Isophotal Wavelengths and Absolute Calibration'' (PASP, 117, 421 [2005])

Details ``The Mauna Kea Observatories Near-Infrared Filter Set. III. Isophotal Wavelengths and Absolute Calibration'' (PASP, 117, 421 [2005]) ``The Mauna Kea Observatories Near-Infrared Filter Set. III. Isophotal Wavelengths and Absolute Calibration'' (PASP, 117, 421 [2005])

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pasp..117.1459t&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 117, Issue 838, pp. 1459-1459.

Astronomy and Astrophysics

Astronomy

13

Errata, Addenda

Scientific paper

The isophotal wavelength for the V filter given in § 2.4 and Table 1 should be 5450 Å.
We did not show the isophotal frequencies in Table 1 that should be used with the flux densities in frequency units (Jy) and the AB magnitudes derived from them. Therefore, we present these in Table 3 below. Note that since λiso≠c/νiso, the isophotal wavelengths and isophotal frequencies must be derived separately using equations (5) and (6). In addition, Fν and AB magnitude values should always be plotted at νiso.

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