• DOI:10.1093/mnras/stv1928
• Corpus ID: 119260068

High-contrast imaging of Sirius A with VLT/SPHERE: looking for giant planets down to one astronomical unit

@article{Vigan2015HighcontrastIO,
  title={High-contrast imaging of Sirius A with VLT/SPHERE: looking for giant planets down to one astronomical unit},
  author={Arthur Vigan and C{\'e}cile Gry and Graeme S. Salter and Dino Mesa and Derek Homeier and Claire Moutou and France Allard},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2015},
  volume={454},
  pages={129-143}
}

• A. Vigan, C. Gry, +4 authors F. Allard
• Published 31 August 2015
• Physics, Geology
• Monthly Notices of the Royal Astronomical Society

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.