NIR fluxes for 35 HR late-type stars (Taylor, 2009)

Details NIR fluxes for 35 HR late-type stars (Taylor, 2009) NIR fluxes for 35 HR late-type stars (Taylor, 2009)

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..61210827t&link_type=abstract

VizieR On-line Data Catalog: J/PASP/121/827. Originally published in: 2009PASP..121..827T

Physics

Stars: Late-Type, Spectrophotometry

Scientific paper

For files fg5blue.dat, k3blue.dat and k3red.dat: The data are given as magnitudes per unit frequency interval. If no measurement for a particular passband was made, the entry "-999" is given. Negative numbers represent genuine data.
For files fg5bwave.dat, k3bwave.dat, and k3rwave.dat: Wavelengths and auxiliary data for the passbands used to obtain the measurements are included. The auxiliary data include two numbers for wavelength programs (see Sect. 2.4 of the paper). If a passband is a member of only one program, the program numbers are the same. If a passband is a member of two neighboring programs, the first (second) number refers to the program used at shorter (longer) wavelengths.
For k3rwave.dat, this is done solely to enforce consistency with wavelength files for collateral data sets. Because program numbers 1-4 are used for short-wavelength data for G and K giants and Procyon, all program numbers in this data file are 5.
(7 data files).

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