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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SIFTIR: Spectro-Polarimetric Imaging Fourier Transform Spectrometer for the InfraRed,n with TNTCAM2 (Klebe et al. 1998), an imaging polarimeter. The FTS component will enhance TNTCAM2, giving the instrument a maximum resolution of 2000 at 10 .m. The FTS is capable of operating between 2–15 .m, but polarimetry for the instrument is limited to the 8–15 .m region due to waveplate/wiregrid characteristics.

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CRIRES: Context and Status,ower of 10. from 1 to 5 .m. It will complement the comparable resolution provided by UVES at visible and ultraviolet wavelengths. Many new scientific prospects will also be opened up by the availability of this new capability for high sensitivity observations at high spectral and spatial resolution

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Science Highlights from 4 Years of NIRSPEC on the Keck II Telescope,ensively and successfully over the last four years. In high-resolution mode (R ~ 20,000–30,000), NIRSPEC science includes studies of comets and solar system bodies, abundance studies in red giants, the kinematics of the population of stars near the Galactic Center, protostars and disks, low-mass spe

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High Resolution Mid-Infrared Spectroscopy of Star and Planet Forming Regions with TEXES,rption and emission toward several embedded young stars. Here, we concentrate on observations of C.H., HCN, SiO, and H. toward the KL region in Orion, with some discussion of molecules observed toward NGC 7538 IRS1. High spectral, and in some cases spatial, resolution is found to be necessary to det

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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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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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