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TEXES

Gemini North
Last Modified: 
Friday, March 22, 2024 - 13:01

The Texas Echelon cross Echelle Spectrograph, TEXES (Lacy et al., 2002), is a mid-infrared (5-25 µm) imaging spectrograph capable of operating in several modes recording point and extended source spectra and maps at a variety of spectral resolutions.

Current Instruments

  • Altair
  • GHOST
  • NIRI
  • TEXES
    • Sensitivity and Time Requests
    • Integration Time Calculator
  • GNIRS
  • IGRINS-2
  • GMOS
  • GeMS
  • Flamingos 2
  • GSAOI
  • `Alopeke & Zorro
  • MAROON-X

Overview

The most frequently used TEXES instrument mode is “hi-med”, a high-resolution cross-dispersed (by the medium-resolution echelle) mode achieving a resolving power R≈λ/δλ~100,000, 0.5% spectral coverage with an ~0.4 x 3″ slit (varying with wavelength). “Hi-lo” mode is a high-resolution cross-dispersed (by low-resolution grating) mode achieving R≈100,000, 0.25 µm spectral coverage, and a very short 0.4″ x 1″ slit. Medium resolution long-slit mode (“med”) achieves R ≈ 15,000, 0.5% spectral coverage, and utilizes an 0.4″ x 16″ slit. Low resolution long slit mode (“low”) achieves δλ ≈ 0.004 µm, 0.25 µm coverage, with a ~0.4″ x 16″ slit. Additionally, two more modes (source acquisition imaging and pupil imaging) are available, though these modes are not used for science observations.

International Gemini Observatory

The International Gemini Observatory  provides the astronomical communities in six participant countries with state-of-the-art astronomical facilities that allocate observing time in proportion to each country's contribution. In addition to financial support, each country also contributes significant scientific and technical resources. The national research agencies that form the Gemini partnership include: the US National Science Foundation (NSF), the Canadian National Research Council (NRC), the Chilean Agencia Nacional de Investigación y Desarrollo (ANID), the Brazilian Ministério da Ciência, Tecnologia e Inovação, the Argentinean Ministerio de Ciencia, Tecnología e Innovación, and the Korea Astronomy and Space Institute (KASI). The observatory is managed by the Association of Universities for Research in Astronomy, Inc. (AURA) under a cooperative agreement with the NSF. The NSF also serves as the executive agency for the international partnership.     


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