Titlebook: High Resolution Infrared Spectroscopy in Astronomy; Proceedings of an ES Hans Ulrich Käufl,Ralf Siebenmorgen,Alan F. M. Moo Conference proc

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,Atomic Data in the 1–5 Micron Region: Present Status,the CRIRES region (1–5 .m). There is a clear distinction between the atomic lines that will appear in absorption in stellar spectra and in emission in nebular spectra. For abundance analyses different classes of lines can be defined on the basis of the energy level structure, either along particular

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High-Resolution Spectroscopy on the Milliarcsecond Scale,illiarcsecond scale. This enables completely new observational approaches to many open problems in stellar and circumstellar astrophysics. Fiber coupling of the output from a relatively simple beam combiner to existing spectrographs offers a cost-effective way to implement interferometric high-resol

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Mri485

Invertebrate

T-ReCS and Michelle: The Mid-Infrared Spectroscopic Capabilities of the Gemini Observatory,llow observers the unique opportunity to apply to one observatory for all-sky spectroscopic access in the mid-infrared with the light gathering power of 8-meter telescopes. Gemini South has recently commissioned the Thermal-Region Camera and Spectrograph (T-ReCS) and is now available to perform queu

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Improving the Accuracy of HCN/HNC Opacity Data and Accounting for Isotopomers, the inherent accuracy problems of ab initio data. The band centres of some overtone bands deviate by up to 10 cm. from experimental values. To improve the quality of many of our line frequencies we are in the process of substituting the available experimentally determined HCN energy levels for thei

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SIFTIR: Spectro-Polarimetric Imaging Fourier Transform Spectrometer for the InfraRed,ith which to diagnose grain characteristics. We are currently developing an instrument that will employ a Fourier transform spectrometer in conjunction with TNTCAM2 (Klebe et al. 1998), an imaging polarimeter. The FTS component will enhance TNTCAM2, giving the instrument a maximum resolution of 2000

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Mid Infrared Spectroscopic Standards: Observations and Models,MI2 instrument at the ESO/La Silla observatory. The low resolution spectra (R ≈ 160) were analyzed with an optimal extraction procedure specifically designed for TIMMI2 spectroscopy. The wavelength calibration was done using atmospheric lines. Our analysis package is based on IDL and will be made av

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GIANO: An Ultra-Stable IR Echelle Spectrometer for the TNG Telescope,dial velocity measurements. It also includes polarimetric capabilities and a low resolution mode that make it a very versatile, common user instrument which will be permanently mounted and available at one of the Nasmyth foci of the Telescopio Nazionale Galileo (TNG) located at Roque de Los Muchacho

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