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arXiv · 1502.03172

Making FORS2 fit for exoplanet observations (again)

H. M. J. Boffin·G. Blanchard·O. A. Gonzalez·S. Moehler·E. Sedaghati·N. Gibson·M. E. van den Ancker·J. Smoker·J. Anderson·C. Hummel·D. Dobrzycka·A. Smette·G. Rupprecht
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Abstract

For about three years, it was known that precision spectrophotometry with FORS2 suffered from systematic errors that made quantitative observations of planetary transits impossible. We identified the Longitudinal Atmospheric Dispersion Compensator (LADC) as the most likely culprit, and therefore engaged in a project to exchange the LADC prisms with the uncoated ones from FORS1. This led to a significant improvement in the depth of FORS2 zero points, a reduction in the systematic noise, and should make FORS2 again competitive for transmission spectroscopy of exoplanets.

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H. M. J. Boffin, G. Blanchard, O. A. Gonzalez, S. Moehler, E. Sedaghati, N. Gibson, M. E. van den Ancker, J. Smoker, J. Anderson, C. Hummel, D. Dobrzycka, A. Smette, G. Rupprecht. 2015-02-11. Making FORS2 fit for exoplanet observations (again). https://arxiv.org/abs/1502.03172

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