High-resolution spectroscopy in the near-infrared could become the leading method for discovering extra-solar planets around very low mass stars and brown dwarfs. In order to help to achieve an accuracy of ∼ m s-1, we are developing a gas cell which consists of a mixture of gases whose absorption spectral lines span all over the near-infrared region. We present the most promising mixture, made of acetylene, nitrous oxide, ammonia, chloromethanes, and hydrocarbons. The mixture is contained in a small size 13cm long gas cell and covers most of the H and K bands. It also shows small absorptions in the J band, but they are few and not sharp enough for near-infrared wavelength calibration. We describe the working method and experiments, and compare our results with the state of the art for near-infrared gas cells. © 2010. The American Astronomical Society. All rights reserved.
CITATION STYLE
Valdivielso, L., Esparza, P., Martín, E. L., Maukonen, D., & Peale, R. E. (2010). A new gas cell for high-precision Doppler measurements in the near-infrared. Astrophysical Journal, 715(2), 1366–1369. https://doi.org/10.1088/0004-637X/715/2/1366
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