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MIDI – the 10 μm instrument on the VLTI
After more than five years of preparation, the mid-infrared interferometric instrument MIDI has been transported to Paranal where it will undergo testing and commissioning on theVery Large TelescopeExpand
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CARMENES instrument overview
This paper gives an overview of the CARMENES instrument and of the survey that will be carried out with it during the first years of operation. CARMENES (Calar Alto high-Resolution search for MExpand
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Ten-micron instrument MIDI: getting ready for observations on the VLTI
The mid-infrared interferometric instrument MIDI is currently undergoing testing in preparation for commissioning on the Very Large Telescope Interferometer VLTI at the end of this year 2002. It willExpand
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Calculated refractivity of water vapor and moist air in the atmospheric window at 10 microm.
  • R. Mathar
  • Materials Science, Medicine
  • Applied optics
  • 1 February 2004
The HITRAN 2000 database of infrared line transitions has been used to calculate the dispersion coefficient of water vapor at room temperature in the atmospheric window up to 25 microm, confirming anExpand
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Chebyshev series expansion of inverse polynomials
The Chebyshev series expansion Σn=0∞anTn(x) of the inverse of a polynomial Σj=0kbjTj(x) is well defined if the polynomial has no roots in [-1,1]. If the inverse polynomial is decomposed into partialExpand
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CARMENES: high-resolution spectra and precise radial velocities in the red and infrared
The design and construction of CARMENES has been presented at previous SPIE conferences. It is a next-generation radial-velocity instrument at the 3.5m telescope of the Calar Alto Observatory, whichExpand
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Refractive index of humid air in the infrared: model fits
The theory of summation of electromagnetic line transitions is summarized in terms of the Taylor expansion of the refractive index of humid air as a function of the basic independent parametersExpand
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MATISSE: perspective of imaging in the mid-infrared at the VLTI
MATISSE is foreseen as a mid-infrared spectro-interferometer combining the beams of up to four UTs/ATs of the Very Large Telescope Interferometer (VLTI) of the European Southern Observatory. TheExpand
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CARMENES: an overview six months after first light
The CARMENES instrument is a pair of high-resolution (R⪆80,000) spectrographs covering the wavelength range from 0.52 to 1.71 μm, optimized for precise radial velocity measurements. It was installedExpand
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The CARMENES search for exoplanets around M dwarfs : First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems
This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, Expand
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