The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits . III. The frequency of brown dwarfs and giant planets as companions to solar-type stars. Reggiani, M., Meyer, M., Chauvin, G., Vigan, A., Quanz, S., Biller, B., Bonavita, M., Desidera, S., Delorme, P., Hagelberg, J., Maire, A. -., Boccaletti, A., Beuzit, J. -., Buenzli, E., Carson, J., Covino, E., Feldt, M., Girard, J., Gratton, R., Henning, T., Kasper, M., Lagrange, A. -., Mesa, D., Messina, S., Montagnier, G., Mordasini, C., Mouillet, D., Schlieder, J., Segransan, D., Thalmann, C., & Zurlo, A. åp, 586:A147, February, 2016.
doi  bibtex   
@ARTICLE{2016A&A...586A.147R,
       author = {{Reggiani}, M. and {Meyer}, M.~R. and {Chauvin}, G. and {Vigan}, A. and {Quanz}, S.~P. and {Biller}, B. and {Bonavita}, M. and {Desidera}, S. and {Delorme}, P. and {Hagelberg}, J. and {Maire}, A. -L. and {Boccaletti}, A. and {Beuzit}, J. -L. and {Buenzli}, E. and {Carson}, J. and {Covino}, E. and {Feldt}, M. and {Girard}, J. and {Gratton}, R. and {Henning}, T. and {Kasper}, M. and {Lagrange}, A. -M. and {Mesa}, D. and {Messina}, S. and {Montagnier}, G. and {Mordasini}, C. and {Mouillet}, D. and {Schlieder}, J.~E. and {Segransan}, D. and {Thalmann}, C. and {Zurlo}, A.},
        title = "{The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits . III. The frequency of brown dwarfs and giant planets as companions to solar-type stars}",
      journal = {\aap},
     keywords = {methods: observational, methods: statistical, binaries: general, brown dwarfs, planetary systems, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
         year = 2016,
        month = feb,
       volume = {586},
          eid = {A147},
        pages = {A147},
          doi = {10.1051/0004-6361/201525930},
archivePrefix = {arXiv},
       eprint = {1510.08453},
 primaryClass = {astro-ph.EP},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016A&A...586A.147R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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