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Near-infrared photometry of stars Results are presented of infrared photometric observations performed oncomparison stars during a monitoring of long-period variables. Theseobservations, spread over a lapse of about 5 years, are used to derivethe J, H, and K magnitudes of 54 stars in the photometric systemdescribed by Koornneef (1983). The 1950.0 coordinates, spectral types,visual magnitudes, average magnitudes, and the number of observationsare given for each object.
 
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Observation and Astrometry data
| Constellation: | つる座 |  
    | Right ascension: | 22h26m06.76s |  
    | Declination: | -44°59'53.0" |  
    | Apparent magnitude: | 7.993 |  
    
        | Distance: | 242.718 parsecs |  
        
    
    | Proper motion RA: | 2 |  
    | Proper motion Dec: | 13.7 |  
    | B-T magnitude: | 9.286 |  
    | V-T magnitude: | 8.1 |  
    
 
 
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