机译:HAT-P-44b, HAT-P-45b, AND HAT-P-46b: THREE TRANSITING HOT JUPITERS IN POSSIBLE MULTI-PLANET SYSTEMS
Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA;
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA;
Konkoly Observatory, Budapest, HungaryDepartment of Astrophysics, California Institute of Technology, Pasadena, CA 91125, USAInstitute for Astronomy, University of Hawaii, Honolulu, HI 96822, USADepartment of Astronomy, University of California, Berkeley, CA 94720, USANiels Bohr Institute, Copenhagen University, DK-2100 Copenhagen, DenmarkDepartment of Astronomy, Yale University, New Haven, CT 06520-8101, USANational Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719, USAHungarian Astronomical Association, 1461 Budapest, HungaryResearch School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, AustraliaKavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA;
planetary systems; stars: individual (HAT-P-44; HAT-P-45; HAT-P-46); techniques: photometric; techniques: spectroscopic;