%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% 木曜日用
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%\Day{月を書いてください}{日にちを書いてください}{木}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\Day{5}{21}{木}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%\AID{ArxiveのIDを入れる(ex. 1234.5678)  空白を置かないように注意！}
%\Dai{タイトル}
%\Chosha{著者}
%\Comments{コメント}
%\Subjects{ex. Earth and Planetary Astrophysics (astro-ph.EP)}
%\Setsumei{理論, 観測, 実験 etc.}
%{
%	コメント
%}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\AID{1505.05403}
\Dai{The effect of craters on the lunar neutron flux}
\Chosha{\href{http://arxiv.org/find/astro-ph/1/au:+Eke_V/0/1/0/all/0/1}{V. R. Eke}, \href{http://arxiv.org/find/astro-ph/1/au:+Bower_K/0/1/0/all/0/1}{K. E. Bower}, \href{http://arxiv.org/find/astro-ph/1/au:+Diserens_S/0/1/0/all/0/1}{S. Diserens}, \href{http://arxiv.org/find/astro-ph/1/au:+Ryder_M/0/1/0/all/0/1}{M. Ryder}, \href{http://arxiv.org/find/astro-ph/1/au:+Yeomans_P/0/1/0/all/0/1}{P. E. L. Yeomans}, \href{http://arxiv.org/find/astro-ph/1/au:+Teodoro_L/0/1/0/all/0/1}{L. F. A. Teodoro}, \href{http://arxiv.org/find/astro-ph/1/au:+Elphic_R/0/1/0/all/0/1}{R. C. Elphic}, \href{http://arxiv.org/find/astro-ph/1/au:+Feldman_W/0/1/0/all/0/1}{W. C. Feldman}, \href{http://arxiv.org/find/astro-ph/1/au:+Hermalyn_B/0/1/0/all/0/1}{B. Hermalyn}, \href{http://arxiv.org/find/astro-ph/1/au:+Lavelle_C/0/1/0/all/0/1}{C. M. Lavelle}, \href{http://arxiv.org/find/astro-ph/1/au:+Lawrence_D/0/1/0/all/0/1}{D. J. Lawrence}}
\Comments{14 pages, 13 pages, JGR submitted }
\Subjects{Earth and Planetary Astrophysics (astro-ph.EP)}
\Setsumei{理論/観測/実験 etc....}
{
	Comment!!!!
}

\AID{1505.05384}
\Dai{Tidal synchronization of close-in satellites and exoplanets. II. Spin  dynamics and extension to Mercury and exoplanets host stars}
\Chosha{\href{http://arxiv.org/find/astro-ph/1/au:+Ferraz_Mello_S/0/1/0/all/0/1}{Sylvio Ferraz-Mello}}
\Comments{Results of this paper were presented as Paper DDA 202.01 at the 45th Annual Meeting of the AAS Division of Dynamical Astronomy, 2014, Philadelphia, USA. Accepted for publication in Celestial Mechanics and Dynamical Astronomy }
\Subjects{Earth and Planetary Astrophysics (astro-ph.EP)}
\Setsumei{理論/観測/実験 etc....}
{
	Comment!!!!
}

\AID{1505.05363}
\Dai{Influence of Stellar Multiplicity On Planet Formation. III. Adaptive  Optics Imaging of Kepler Stars With Gas Giant Planets}
\Chosha{\href{http://arxiv.org/find/astro-ph/1/au:+Wang_J/0/1/0/all/0/1}{Ji Wang}, \href{http://arxiv.org/find/astro-ph/1/au:+Fischer_D/0/1/0/all/0/1}{Debra A. Fischer}, \href{http://arxiv.org/find/astro-ph/1/au:+Horch_E/0/1/0/all/0/1}{Elliott P. Horch}, \href{http://arxiv.org/find/astro-ph/1/au:+Xie_J/0/1/0/all/0/1}{Ji-Wei Xie}}
\Comments{18 pages, 5 figures, accepted by ApJ }
\Subjects{Earth and Planetary Astrophysics (astro-ph.EP)}
\Setsumei{理論/観測/実験 etc....}
{
	Comment!!!!
}

\AID{1505.05492}
\Dai{The Properties of G-modes in Layered Semi-Convection}
\Chosha{\href{http://arxiv.org/find/astro-ph/1/au:+Belyaev_M/0/1/0/all/0/1}{Mikhail Belyaev}, \href{http://arxiv.org/find/astro-ph/1/au:+Quataert_E/0/1/0/all/0/1}{Eliot Quataert}, \href{http://arxiv.org/find/astro-ph/1/au:+Fuller_J/0/1/0/all/0/1}{Jim Fuller}}
\Comments{13 pages, 5 figures, submitted to MNRAS }
\Subjects{Solar and Stellar Astrophysics (astro-ph.SR); Earth and Planetary Astrophysics (astro-ph.EP)}
\Setsumei{理論/観測/実験 etc....}
{
	Comment!!!!
}

\AID{1505.05325}
\Dai{Asymmetric features in the protoplanetary disk MWC758}
\Chosha{\href{http://arxiv.org/find/astro-ph/1/au:+Benisty_M/0/1/0/all/0/1}{M. Benisty}, \href{http://arxiv.org/find/astro-ph/1/au:+Juhasz_A/0/1/0/all/0/1}{A. Juhasz}, \href{http://arxiv.org/find/astro-ph/1/au:+Boccaletti_A/0/1/0/all/0/1}{A. Boccaletti}, \href{http://arxiv.org/find/astro-ph/1/au:+Avenhaus_H/0/1/0/all/0/1}{H. Avenhaus}, \href{http://arxiv.org/find/astro-ph/1/au:+Milli_J/0/1/0/all/0/1}{J. Milli}, \href{http://arxiv.org/find/astro-ph/1/au:+Thalmann_C/0/1/0/all/0/1}{C. Thalmann}, \href{http://arxiv.org/find/astro-ph/1/au:+Dominik_C/0/1/0/all/0/1}{C. Dominik}, \href{http://arxiv.org/find/astro-ph/1/au:+Pinilla_P/0/1/0/all/0/1}{P. Pinilla}, \href{http://arxiv.org/find/astro-ph/1/au:+Buenzli_E/0/1/0/all/0/1}{E. Buenzli}, \href{http://arxiv.org/find/astro-ph/1/au:+Pohl_A/0/1/0/all/0/1}{A. Pohl}, \href{http://arxiv.org/find/astro-ph/1/au:+Beuzit_J/0/1/0/all/0/1}{J.-L. Beuzit}, \href{http://arxiv.org/find/astro-ph/1/au:+Birnstiel_T/0/1/0/all/0/1}{T. Birnstiel}, \href{http://arxiv.org/find/astro-ph/1/au:+Boer_J/0/1/0/all/0/1}{J. de Boer}, \href{http://arxiv.org/find/astro-ph/1/au:+Bonnefoy_M/0/1/0/all/0/1}{M. Bonnefoy}, \href{http://arxiv.org/find/astro-ph/1/au:+Chauvin_G/0/1/0/all/0/1}{G. Chauvin}, \href{http://arxiv.org/find/astro-ph/1/au:+Christiaens_V/0/1/0/all/0/1}{V. Christiaens}, \href{http://arxiv.org/find/astro-ph/1/au:+Garufi_A/0/1/0/all/0/1}{A. Garufi}, \href{http://arxiv.org/find/astro-ph/1/au:+Grady_C/0/1/0/all/0/1}{C. Grady}, \href{http://arxiv.org/find/astro-ph/1/au:+Henning_T/0/1/0/all/0/1}{T. Henning}, \href{http://arxiv.org/find/astro-ph/1/au:+Huelamo_N/0/1/0/all/0/1}{N. Huelamo}, \href{http://arxiv.org/find/astro-ph/1/au:+Isella_A/0/1/0/all/0/1}{A. Isella}, \href{http://arxiv.org/find/astro-ph/1/au:+Langlois_M/0/1/0/all/0/1}{M. Langlois}, \href{http://arxiv.org/find/astro-ph/1/au:+Menard_F/0/1/0/all/0/1}{F. Menard}, \href{http://arxiv.org/find/astro-ph/1/au:+Mouillet_D/0/1/0/all/0/1}{D. Mouillet}, \href{http://arxiv.org/find/astro-ph/1/au:+Olofsson_J/0/1/0/all/0/1}{J. Olofsson}, \href{http://arxiv.org/find/astro-ph/1/au:+Pantin_E/0/1/0/all/0/1}{E. Pantin}, \href{http://arxiv.org/find/astro-ph/1/au:+Pinte_C/0/1/0/all/0/1}{C. Pinte}, \href{http://arxiv.org/find/astro-ph/1/au:+Pueyo_L/0/1/0/all/0/1}{L. Pueyo}}
\Comments{Accepted by A\&A Letters }
\Subjects{Solar and Stellar Astrophysics (astro-ph.SR); Earth and Planetary Astrophysics (astro-ph.EP)}
\Setsumei{理論/観測/実験 etc....}
{
	Comment!!!!
}
