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Ca II H and K Filter Photometry on the UVBY System. II. The Catalog of Observations
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1995AJ....109.2828T&db_key=AST
| Ca II H and K filter photometry on the UVBY system. I - The standard system
A fifth filter (fwhm = 90 A) centered on Ca II H and K has beendeveloped for use with the standard uvby system. The filter, called Ca,is designed primarily for applications to metal-poor dwarfs and redgiants, regions where the uvby metallicity index, m(l), loses somesensitivity. An index, hk, is defined by replacing v in m(l) by Ca. Theeffects of interstellar extinction on the index are modeled anddemonstrated to be modest and relatively insensitive to spectral type.Observations of V, (b-y), and hk for 163 primary standards are detailedand transformed to the standard V and (b-y) system. A qualitativeanalysis using only the primary standards indicates that hk is moresensitive than m(l) over the regions of interest by about a factor of 3.
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Observation and Astrometry data
| Constellation: | Wassermann |
| Right ascension: | 21h07m21.87s |
| Declination: | -00°45'54.5" |
| Apparent magnitude: | 6.586 |
| Distance: | 172.117 parsecs |
| Proper motion RA: | 1.3 |
| Proper motion Dec: | 19.8 |
| B-T magnitude: | 7.976 |
| V-T magnitude: | 6.701 |
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