ROME/REA: a gravitational microlensing search for exoplanets beyond the snow line on a global network of robotic telescopes

Planet population synthesis models predict an abundance of planets with semimajor axes between 1 and 10 au, yet they lie at the edge of the detection limits of most planet finding techniques. Discovering these planets and studying their distribution is critical to understanding the physical processe...

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Main Authors: Tsapras, Yiannis (Author) , Street, R. A. (Author) , Hundertmark, Markus (Author) , Bachelet, E. (Author) , Dominik, M. (Author) , Bozza, V. (Author) , Cassan, A. (Author) , Wambsganß, Joachim (Author) , Horne, K. (Author) , Mao, S. (Author) , Zang, W. (Author) , Bramich, D. M. (Author) , Saha, A. (Author)
Format: Article (Journal)
Language:English
Published: 2019 October 11
In: Publications of the Astronomical Society of the Pacific
Year: 2019, Volume: 131, Issue: 1006
ISSN:1538-3873
DOI:10.1088/1538-3873/ab3b19
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1088/1538-3873/ab3b19
Verlag, lizenzpflichtig, Volltext: https://iopscience.iop.org/article/10.1088/1538-3873/ab3b19
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Author Notes:Yiannis Tsapras, R.A. Street, M. Hundertmark, E. Bachelet, M. Dominik, V. Bozza, A. Cassan, J. Wambsganss, K. Horne, S. Mao, W. Zang, D.M. Bramich, and A. Saha

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