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Physical parameters of late M-type members of Chamaleon I and TW Hydrae Association: Dust settling, age dispersion and activity

, , , , , , , , and . (2016)cite arxiv:1610.06951Comment: 26 pages, 22 figures, 10 tables. Accepted in MNRAS.

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Close-in planets around giant stars. Lack of hot-Jupiters and prevalence of multi-planetary systems, , and . (2016)cite arxiv:1603.09719Comment: Accepted for publication in A&A. 5 pages, 4 figures, 1 table.Physical parameters of late M-type members of Chamaleon I and TW Hydrae Association: Dust settling, age dispersion and activity, , , , , , , , and . (2016)cite arxiv:1610.06951Comment: 26 pages, 22 figures, 10 tables. Accepted in MNRAS.The CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars, , , , , , , , , and 163 other author(s). (2017)cite arxiv:1711.06576Comment: accepted for publication in A&A, 13 pages plus 40 pages spectral atlas, first 10 atlas pages are reduced in quality to fit arXiv size limit; one CARMENES spectrum for each of the 324 stars is published in electronic format at http://carmenes.cab.inta-csic.es/.A tidal disruption-like X-ray flare from the quiescent galaxy SDSS J120136.02+300305.5, , , , , , and . (2012)cite arxiv:1202.5900Comment: Accepted for publication in Astronomy and Astrophysics. 11 pages, 11 figures.VOSA: virtual observatory SED analyzer. An application to the Collinder 69 open cluster, , , , , , and . \aap, (December 2008)