@article{Petigura_Howard_Marcy_2013,
  title = {{Prevalence of Earth-size planets orbiting Sun-like stars}},
  volume = {110},
  url = {http://dx.doi.org/10.1073/pnas.1319909110},
  doi = {10.1073/pnas.1319909110},
  number = {48},
  journal = {Proceedings of the National Academy of Sciences},
  publisher = {Proceedings of the National Academy of Sciences},
  author = {Petigura, E. A. and Howard, A. W. and Marcy, G. W.},
  year = {2013},
  month = {Nov},
  pages = {19273-19278},
}


@ARTICLE{2013ApJ...764..105S,
  author = {{Swift}, J.~J. and {Johnson}, J.~A. and {Morton}, T.~D. and {Crepp}, J.~R. and {Montet}, B.~T. and {Fabrycky}, D.~C. and {Muirhead}, P.~S.},
  title = {{Characterizing the Cool KOIs. IV. Kepler-32 as a Prototype for the Formation of Compact Planetary Systems throughout the Galaxy}},
  journal = {\apj},
  archiveprefix = {arXiv},
  eprint = {1301.0023},
  primaryclass = {astro-ph.EP},
  keywords = {methods: statistical, planetary systems, planets and satellites: detection, planets and satellites: formation, stars: individual: KID 9787239/KOI-952/Kepler-32},
  year = {2013},
  month = {feb},
  volume = {764},
  eid = {105},
  pages = {105},
  doi = {10.1088/0004-637X/764/1/105},
  adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...764..105S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}


@ARTICLE{2012Natur.481..167C,
  author = {{Cassan}, A. and {Kubas}, D. and {Beaulieu}, J.-P. and {Dominik}, M. and {Horne}, K. and {Greenhill}, J. and {Wambsganss}, J. and {Menzies}, J. and {Williams}, A. and {J{\o}rgensen}, U.~G. and {Udalski}, A. and {Bennett}, D.~P. and {Albrow}, M.~D. and {Batista}, V. and {Brillant}, S. and {Caldwell}, J.~A.~R. and {Cole}, A. and {Coutures}, C. and {Cook}, K.~H. and {Dieters}, S. and {Prester}, D.~D. and {Donatowicz}, J. and {Fouqu{\'e}}, P. and {Hill}, K. and {Kains}, N. and {Kane}, S. and {Marquette}, J.-B. and {Martin}, R. and {Pollard}, K.~R. and {Sahu}, K.~C. and {Vinter}, C. and {Warren}, D. and {Watson}, B. and {Zub}, M. and {Sumi}, T. and {Szyma{\'n}ski}, M.~K. and {Kubiak}, M. and {Poleski}, R. and {Soszynski}, I. and {Ulaczyk}, K. and {Pietrzy{\'n}ski}, G. and {Wyrzykowski}, {\L}.},
  title = {{One or more bound planets per Milky Way star from microlensing observations}},
  journal = {\nat},
  archiveprefix = {arXiv},
  eprint = {1202.0903},
  primaryclass = {astro-ph.EP},
  year = {2012},
  month = {jan},
  volume = {481},
  pages = {167-169},
  doi = {10.1038/nature10684},
  adsurl = {http://adsabs.harvard.edu/abs/2012Natur.481..167C},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}


@article{Lineweaver_Davis_2002,
  title = {{Does the Rapid Appearance of Life on Earth Suggest that Life Is Common in the Universe?}},
  volume = {2},
  url = {http://dx.doi.org/10.1089/153110702762027871},
  doi = {10.1089/153110702762027871},
  number = {3},
  journal = {Astrobiology},
  publisher = {Mary Ann Liebert Inc},
  author = {Lineweaver, Charles H. and Davis, Tamara M.},
  year = {2002},
  month = {Aug},
  pages = {293-304},
}


@article{nishimichi_testing_2014,
  title = {{Testing the equal-time angular-averaged consistency relation of the gravitational dynamics in N-body simulations}},
  url = {http://arxiv.org/abs/1402.3293},
  abstract = {We explicitly test the equal-time consistency relation between the angular-averaged bispectrum and the power spectrum of the matter density field employing a large suite of cosmological {\$N\$-body} simulations. This is the lowest-order version of the relations between \$({\textbackslash}ell+n)-\$point and \$n-\$point polyspectra, where one averages over the angles of \${\textbackslash}ell\$ soft modes. This relation depends on two wave numbers, \$k'\$ in the soft domain and \$k\$ in the hard domain. We show that it holds up to a good accuracy, when \$k'/k{\textbackslash}ll 1\$ and \$k'\$ is in the linear regime, while the hard mode \$k\$ goes from linear (\$0.1{\textbackslash},h{\textbackslash},{\textbackslash}{mathrm\{Mpc\}{\textasciicircum}\{-1\}\$)} to nonlinear (\$1.0{\textbackslash},h{\textbackslash},{\textbackslash}{mathrm\{Mpc\}{\textasciicircum}\{-1\}\$)} scales. On scales \$k{\textbackslash}lesssim 0.4{\textbackslash},h{\textbackslash},{\textbackslash}{mathrm\{Mpc\}{\textasciicircum}\{-1\}\$} we confirm the relation within a \${\textbackslash}sim 5{\textbackslash}\%\$ accuracy, even though the bispectrum can already deviate from leading-order perturbation theory by more than \$30{\textbackslash}\%\$. We further show that the relation extends up to nonlinear scales, \$k {\textbackslash}sim 1.0{\textbackslash},h{\textbackslash},{\textbackslash}{mathrm\{Mpc\}{\textasciicircum}\{-1\}\$} within an accuracy of \${\textbackslash}sim 10{\textbackslash}\%\$.},
  urldate = {2014-02-17},
  journal = {{arXiv:1402.3293} [astro-ph]},
  author = {Nishimichi, Takahiro and Valageas, Patrick},
  month = {feb},
  year = {2014},
  keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics},
  annote = {Comment: 9 pages, 7 figures},
  file = {1402.3293 PDF:/Users/Matteo/Library/Application Support/Zotero/Profiles/422c33t5.default/zotero/storage/NUPWGC6Q/Nishimichi and Valageas - 2014 - Testing the equal-time angular-averaged consistenc.pdf:application/pdf;arXiv.org Snapshot:/Users/Matteo/Library/Application Support/Zotero/Profiles/422c33t5.default/zotero/storage/S6MBAE8T/1402.html:text/html},
}
