We provide magnitude and color transformations between two near-infrared photometric systems, 2MASS and SIRIUS, the latter currently implemented with the three-channel SIRIUS camera on 1.4 m Infrared Survey Facility telescope at the South African Astronomical Observatory. The transformation equations are derived using a carefully selected sample of 32 770 stars in the Large and Small Magellanic Clouds that have high quality observations available in both photometric systems. The derived transformations are valid in the color range -0.1 15' —0-05 < (H -Ks)sirius < 0-7 and -0.1 < (J - Ks)sirius < 1.7Vilniaus universitetasVilniaus universiteto Teorinės fizikos ir astronomijos institutasVytauto Didžiojo universitetasŠvietimo akademij
International audienceWe present imaging data and photometry for the COSMOS survey in 15 photometric...
We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and...
In order to maximize sensitivity, optical space surveillance sensors use detectors that have good se...
We present colour transformations from Two Micron All Sky Survey (2MASS) photometric system to Johns...
Near-infrared photometry of 599 stars is used to calculate transformations from the South African A...
We present colour transformations for the conversion of the W1 and W2 magnitudes of the Wide-field I...
We discuss optical and infrared photometric properties of stars matched in the Two Micron All Sky Su...
We present color transformations for the conversion of the 2MASS photometric system to the Johnson-C...
We present a new luminosity-colour relation based on trigonometric parallaxes for thin-disc main-seq...
A challenge in absolute calibration is to relate very bright stars with physical flux measurements t...
Using reliable trigonometric measurements, we find that the absolute magnitude of cataclysmic variab...
<p>The Tycho and Tycho-2 catalogs and the SuperWASP survey report photometry for millions of stars o...
Sirius, the seventh-nearest stellar system, is a visual binary containing the metallic-line A1. V st...
Photometric data on the Kron-Cousins photometric system have been obtained for 118 new late K to mid...
We present colour transformations for the conversion of Wide-Field Survey Explorer W1, W2, and W3 ma...
International audienceWe present imaging data and photometry for the COSMOS survey in 15 photometric...
We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and...
In order to maximize sensitivity, optical space surveillance sensors use detectors that have good se...
We present colour transformations from Two Micron All Sky Survey (2MASS) photometric system to Johns...
Near-infrared photometry of 599 stars is used to calculate transformations from the South African A...
We present colour transformations for the conversion of the W1 and W2 magnitudes of the Wide-field I...
We discuss optical and infrared photometric properties of stars matched in the Two Micron All Sky Su...
We present color transformations for the conversion of the 2MASS photometric system to the Johnson-C...
We present a new luminosity-colour relation based on trigonometric parallaxes for thin-disc main-seq...
A challenge in absolute calibration is to relate very bright stars with physical flux measurements t...
Using reliable trigonometric measurements, we find that the absolute magnitude of cataclysmic variab...
<p>The Tycho and Tycho-2 catalogs and the SuperWASP survey report photometry for millions of stars o...
Sirius, the seventh-nearest stellar system, is a visual binary containing the metallic-line A1. V st...
Photometric data on the Kron-Cousins photometric system have been obtained for 118 new late K to mid...
We present colour transformations for the conversion of Wide-Field Survey Explorer W1, W2, and W3 ma...
International audienceWe present imaging data and photometry for the COSMOS survey in 15 photometric...
We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and...
In order to maximize sensitivity, optical space surveillance sensors use detectors that have good se...