Red Optical Planet Survey : A radial velocity search for low mass M dwarf planets

Barnes, J.R., Jenkins, J. S., Jones, H.R.A., Rojo, P., Arriagada, P., Jordan, A., Minniti, D., Tuomi, M., Jeffers, S.V. and Pinfield, D.J. (2013) Red Optical Planet Survey : A radial velocity search for low mass M dwarf planets. In: Conference on Hot Planets and Cool Stars, 2012-11-12 - 2012-11-16, Garching.
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We present radial velocity results from our Red Optical Planet Survey (ROPS), aimed at detecting low-mass planets orbiting mid-late M dwarfs. The similar to 10 ms(-1) precision achieved over 2 consecutive nights with the MIKE spectrograph at Magellan Clay is also found on week long timescales with UVES at VLT. Since we find that UVES is expected to attain photon limited precision of order 2 ms-1 using our novel deconvolution technique, we are limited only by the (
Item Type Conference or Workshop Item (Other)
Additional information This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
Date Deposited 15 May 2025 16:34
Last Modified 10 Jul 2025 23:32

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