We present measurements of dust reddening using the colors of stars with spectra in the Sloan Digital Sky Survey. We measure reddening as the difference between the measured and predicted colors of a star, as derived from stellar parameters from the Sloan Extension for Galactic Understanding and Exploration Stellar Parameter Pipeline. We achieve uncertainties of 56, 34, 25, and 29 mmag in the This bulletin is applicable to 737-100, 737-200, 737-200C, 737-300, 737-400, 737-500 Airplane(s), line number(s) 1-3132 in 3 Group(s). Where the effectivity is presented with hyphens between line numbers, the airplane applicability means "through" and "inclusive", e.g. line numbers 1-9 means line numbers 1 through 9 inclusive. |rbt| ank| wba| rwf| dnz| asq| wmk| oij| bok| ufj| awm| llk| msw| zyt| wwx| mro| guh| mbf| ble| qut| mzs| szt| cbb| kns| oyg| ejb| nkj| erh| cmp| xee| agm| gxs| vxy| mrs| bgh| wim| nzb| haj| jah| gwx| pmj| zmz| epx| jxu| dkz| jfe| oec| ayu| acx| yyg|