Add to ORKGWe present a new solution for the dispersive element in astronomical spectrographs that, in many cases, can provide an upgrade path to enhance the spectral resolution of existing moderate-resolution reflection-grating spectrographs. We demonstrate that in the case of LRIS-R at the Keck 1 Telescope, a spectral resolution of 18,000 can be achieved with reasonable throughput under good seeing conditions
© 2016, Pleiades Publishing, Ltd.We present a new scheme of a moderate-resolution spectrograph based...
HISPEC (High-resolution Infrared Spectrograph for Exoplanet Characterization) is a proposed diffract...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
We present a new solution for the dispersive element in astronomical spectrographs that, in many cas...
This paper describes a technique which has been applied to the new AAT coudé échelle spectrograph, u...
An externally dispersed interferometer (EDI) is a series combination of a fixed delay interferometer...
Many focal-reducer spectrographs, currently available at state-of-the-art telescopes facilities, wou...
Massively multiplexed spectroscopic stellar surveys such as MSE present enormous challenges in the s...
The combination of high spatial and spectral resolution in optical astronomy enables new observation...
© 2016, Pleiades Publishing, Ltd.We present a new scheme of a moderate-resolution spectrograph based...
The Low Resolution Imaging Spectrometer (LRIS) for the Cassegrain focus of the Keck 10-m telescope o...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
The Low Resolution Imaging Spectrometer (LRIS) for the Cassegrain focus of the Keck 10-m telescope o...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
© 2016, Pleiades Publishing, Ltd.We present a new scheme of a moderate-resolution spectrograph based...
HISPEC (High-resolution Infrared Spectrograph for Exoplanet Characterization) is a proposed diffract...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
We present a new solution for the dispersive element in astronomical spectrographs that, in many cas...
This paper describes a technique which has been applied to the new AAT coudé échelle spectrograph, u...
An externally dispersed interferometer (EDI) is a series combination of a fixed delay interferometer...
Many focal-reducer spectrographs, currently available at state-of-the-art telescopes facilities, wou...
Massively multiplexed spectroscopic stellar surveys such as MSE present enormous challenges in the s...
The combination of high spatial and spectral resolution in optical astronomy enables new observation...
© 2016, Pleiades Publishing, Ltd.We present a new scheme of a moderate-resolution spectrograph based...
The Low Resolution Imaging Spectrometer (LRIS) for the Cassegrain focus of the Keck 10-m telescope o...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
The Low Resolution Imaging Spectrometer (LRIS) for the Cassegrain focus of the Keck 10-m telescope o...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...
© 2016, Pleiades Publishing, Ltd.We present a new scheme of a moderate-resolution spectrograph based...
HISPEC (High-resolution Infrared Spectrograph for Exoplanet Characterization) is a proposed diffract...
Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar l...