期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 454, 期 1, 页码 129-143出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv1928
关键词
methods: data analysis; techniques: high angular resolution; stars: individual: Sirius A; planetary systems
资金
- ESO Telescopes at the La Silla Paranal Observatory [60.A-9365, 60.A-9382]
- French National Research Agency (ANR) [ANR10-BLANC0504-01]
- Italian Ministry of Education, University, and Research
- European Research Council under European Community [247060]
- Collaborative Research Centre of the German Research Foundation (DFG) [SFB 881]
Sirius has always attracted a lot of scientific interest, especially after the discovery of a companion white dwarf at the end of the 19th century. Very early on, the existence of a potential third bodywas put forward to explain some of the observed properties of the system. We present new coronagraphic observations obtained with VLT/SPHERE (Very Large Telescope/SpectroPolarimetric High-contrast Exoplanet REsearch) that explore, for the very first time, the innermost regions of the system down to 0.2 arcsec(0.5 au) from Sirius A. Our observations cover the near-infrared from 0.95 to 2.3 mu m and they offer the best on-sky contrast ever reached at these angular separations. After detailing the steps of our SPHERE/IRDIFS data analysis, we present a robust method to derive detection limits for multispectral data from high-contrast imagers and spectrographs. In terms of raw performance, we report contrasts of 14.3 mag at 0.2 arcsec, similar to 16.3 mag in the 0.4-1.0 arcsec range and down to 19 mag at 3.7 arcsec. In physical units, our observations are sensitive to giant planets down to 11 M-Jup at 0.5 au, 6-7 M-Jup in the 1-2 au range and similar to 4 M-Jup at 10 au. Despite the exceptional sensitivity of our observations, we do not report the detection of additional companions around Sirius A. Using a Monte Carlo orbital analysis, we show that we can reject, with about 50 per cent probability, the existence of an 8 M-Jup planet orbiting at 1 au.
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