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The image of the field should be a reduced (co-added) GMOS image supplied by Gemini, or a similarly reduced image. The image should be a MEF file. More information about MEF files can be found on the data formats page.
The Gemini e-newscast #45 (Mar. 15, 2013) features:
- Discovery of an Extremely Nearby Brown Dwarf Pair
- Semester 2013B Proposals
- The Journey Continues
Because TEXES is background photon noise limited and both the instrumental response and the background flux depend on wavelength, the instrument sensitivity depends strongly on wavelength and spectral resolution. Proposers are encouraged to contact TEXES team members for sensitivity estimates for observations at specific wavelengths, but can make initial estimates based on the table below.