Sub-nm resolution cavity enhanced micro-spectrometer. Bernardo B. C. Kyotoku, Long Chen, and Michal Lipson. Author Information. Author Affiliations. Bernardo B. C. Kyotoku, 1, 2 Long Chen, 1 and Michal Lipson 1. 1 School of Electrical and Computer Engineering, Cornell University, Ithaca, N. Y. 14850 USA. 2 Departamento de Física, Universidade …
Sub-nm resolution cavity enhanced micro-spectrometer Bernardo B. C. Kyotoku 1,2, Long Chen 1 and Michal Lipson 1 1School of Electrical and Computer Engineering, Cornell University, Ithaca, N.Y. 14850, The chip size is 8 mm x 8 mm. High channel density and spectral resolution are achieved using high aspect ratio 0.6 mum x 1.5 mum waveguide apertures to inject the light into the input combiner …
1/1/2010 · adshelp[at]cfa.harvard.edu The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A, The difference is due to resolution of the calibration of the LVOF microspectrometer with spectral channels that are 0.5 nm apart. The algorithm yields spectral peaks at 637.1 nm, 639 nm and 640.5 for the Neon spectral lines at 638.3 nm and 640.2 nm.
