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: Hot Planets and Cool Stars :. EPJ Web of Conferences . EDP Sciences, DEU.
Copy

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 (


picture_as_pdf
906857.pdf
subject
Published Version

View Download

Atom BibTeX OpenURL ContextObject in Span OpenURL ContextObject Dublin Core MPEG-21 DIDL Data Cite XML EndNote HTML Citation METS MODS RIOXX2 XML Reference Manager Refer ASCII Citation
Export

Downloads