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Page 16
The latter is a methods - only paper , but emphasizes that wavelets lose less information during smoothing than other methods in current use . This information - conserving aspect makes wavelet transforms a particularly promising ...
The latter is a methods - only paper , but emphasizes that wavelets lose less information during smoothing than other methods in current use . This information - conserving aspect makes wavelet transforms a particularly promising ...
Page 302
is an upper bound in Li with color starting at log e ( Li ) = 3.2 for the hottest stars and declining to less than 0.7 for the coolest . The Li dip is readily apparent starting sharply at ( B - V ) = 0.42 and merging with the more ...
is an upper bound in Li with color starting at log e ( Li ) = 3.2 for the hottest stars and declining to less than 0.7 for the coolest . The Li dip is readily apparent starting sharply at ( B - V ) = 0.42 and merging with the more ...
Page 406
These data are tabulated in Table 2 , wherein N gives the number of detections . Only stars with at least two detections , V errors less than 0.050 mag , and B - V errors less than 0.071 mag are shown in Fig . 2 and Table 2.
These data are tabulated in Table 2 , wherein N gives the number of detections . Only stars with at least two detections , V errors less than 0.050 mag , and B - V errors less than 0.071 mag are shown in Fig . 2 and Table 2.
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