"Laser frequency combs (LFCs) have found their way from laboratory spectroscopy into astronomy to serve as calibrators for spectrographs. We introduce the basic concepts of frequency combs and how they are used for astronomy. We present the results from test campaigns on HARPS, especially our last campaign in April 2015, when we permanently installed the LFC for HARPS and brought another LFC there for testing. Some lessons are learned from HARPS results for ESPRESSO. The ESPRESSO LFC in under building in Menlo and the laboratory characterization is showed."Content of this collection: presentation slides, Q&A transcript
Context. The solar spectrum is a primary reference for the study of physical processes in stars and ...
An important technique for discovering and characterizing planets beyond our solar system relies upo...
We describe the development of a broadband astro-comb providing wavelength coverage of 500 - 620 nm,...
<p>"Laser frequency combs (LFCs) have found their way from laboratory spectroscopy into astronomy to...
"Laser Frequency Combs (LFCs) for Astronomy are very promising alternatives to Hollow Cathode Lamps ...
Author Institution: Harvard-Smithsonian, Cambridge, MALaser frequency combs adapted to serve as wave...
Two of the science goals for the upcoming Extremely Large Telescope are the search for fundamental c...
Laser frequency comb sources promise to enable precision astronomical spectroscopy at the 10-11 leve...
An Optical Frequency Comb (OFC) is an optical spectrum consisting of uniformly spaced lines. The sta...
Astronomical spectroscopy allows detection of exoplanets and their atmospheres, and gives insights i...
Precision calibration of astronomical spectrographs is essential to the hunt for exoplanets, the stu...
A direct measurement of the universe's expansion history could be made by observing in real time the...
Large telescopes with increased light-collecting power have alleviated the photon-noise limitation t...
For the first time a mode filtered frequency comb has been used to calibrate an astronomical spectro...
Searches for extrasolar planets using the periodic Doppler shift of stellar spectral lines resulting...
Context. The solar spectrum is a primary reference for the study of physical processes in stars and ...
An important technique for discovering and characterizing planets beyond our solar system relies upo...
We describe the development of a broadband astro-comb providing wavelength coverage of 500 - 620 nm,...
<p>"Laser frequency combs (LFCs) have found their way from laboratory spectroscopy into astronomy to...
"Laser Frequency Combs (LFCs) for Astronomy are very promising alternatives to Hollow Cathode Lamps ...
Author Institution: Harvard-Smithsonian, Cambridge, MALaser frequency combs adapted to serve as wave...
Two of the science goals for the upcoming Extremely Large Telescope are the search for fundamental c...
Laser frequency comb sources promise to enable precision astronomical spectroscopy at the 10-11 leve...
An Optical Frequency Comb (OFC) is an optical spectrum consisting of uniformly spaced lines. The sta...
Astronomical spectroscopy allows detection of exoplanets and their atmospheres, and gives insights i...
Precision calibration of astronomical spectrographs is essential to the hunt for exoplanets, the stu...
A direct measurement of the universe's expansion history could be made by observing in real time the...
Large telescopes with increased light-collecting power have alleviated the photon-noise limitation t...
For the first time a mode filtered frequency comb has been used to calibrate an astronomical spectro...
Searches for extrasolar planets using the periodic Doppler shift of stellar spectral lines resulting...
Context. The solar spectrum is a primary reference for the study of physical processes in stars and ...
An important technique for discovering and characterizing planets beyond our solar system relies upo...
We describe the development of a broadband astro-comb providing wavelength coverage of 500 - 620 nm,...