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- W2064867553 abstract "Spectrograph slit is conventionally used to enhance the spectral resolution and manage how much light can be allowed to enter spectrograph. The narrow slit provides a higher resolution but sacrifices efficiency of spectrograph and results in a low signal to noise ratio (S/N) spectra product. We take GuoShouJing telescope as an example and carry out a series of experiments to study how its 2/3 slit mode affects the precision of stellar radial velocity measurement and atmosphere parameters estimate. By transforming the resolution and adding a Gaussian White Noise to the extremely high quality spectra from the Sloan Digital Sky Survey, we generate synthetic stellar spectra of various brightness with different S/Ns. Comparing the measurements on these noise added spectra with the original high quality ones, we summarize the influences of the 2/3 slit mode on the measurement accuracy of stellar radial velocity and atmospheric parameters." @default.
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- W2064867553 date "2013-07-25" @default.
- W2064867553 modified "2023-10-12" @default.
- W2064867553 title "The effects of spectrograph slit modes on the accuracy of stellar radial velocity measurement and atmospheric parameter estimation" @default.
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- W2064867553 doi "https://doi.org/10.1007/s11433-013-5272-5" @default.
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