HATS-4b: A DENSE HOT-JUPITER TRANSITING A SUPER METAL-RICH G STAR †

摘要: Development of the HATSouth project was funded by NSFMRI grant NSF/AST-0723074, operations have been supported by NASA grants NNX09AB29G and NNX12AH91H, followup observations receive partial support from grant NSF/AST- 1108686. A.J. acknowledges FONDECYT project 1130857, BASAL CATA PFB-06, projects IC120009 “Millennium Institute Astrophysics (MAS)” P10-022-F the Millennium Science Initiative, Chilean Ministry Economy. R.B. N.E. are CONICYT-PCHA/Doctorado Nacional. R.B. additional Nucleus P10-022-F Millennium Ministry of Economy. V.S. form BASAL CATA PFB-06. M.R. FONDECYT postdoctoral fellowship 3120097. Australian access to Magellan Telescopeswas supported through National Collaborative Research Infrastructure Strategy Federal Government. Work at University is by ARC Laureate Fellowship Grant FL0992131. We acknowledge the use AAVSO Photometric All-Sky Survey (APASS), funded RobertMartin Ayers Sciences Fund, NASA’s Astrophysics Data System Bibliographic Services, SIMBADdatabase, operated CDS, Strasbourg, France. Operations at MPG/ESO 2.2 m Telescope jointly performed the Max Planck Gesellschaft European Southern Observatory.