Measurements of Extrasolar Planetary Transits

ORAL

Abstract

A campaign to measure properties of extrasolar planets using the transit method was undertaken at the University of Dallas using a C-14 telescope and SBIG 2000XM CCD camera. We successfully recorded transits of TrES-1b, Wasp-3, and HatP1. The C-14 exposure and tracking data (on WASP-3) indicate that we can probably effectively monitor stars to 13.5 or 14 magnitude with the C-14. We present the transit data, modeling, and determined planetary characteristics. The equipment used in this research was comparatively inexpensive and widely available and can be implemented at other small universities.

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Authors

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster

  • Sacha Kopp

    Texas Lutheran, Texas Lutheran University, Bastrop ISD, Lego Education, LEGO Education, South Texas Chapter, Health Physics Society, Waxahachie Early College High School, Navarro College, and Texas A\&M Commerce, PTRA/AAPT, National Instruments, Department of Physics, University of Texas at Austin, Texas A&M University - Commerce, University of Dallas, Austin Community College, Angelo State University, K-12 Science Consultant Birdville ISD, Energy Institute, University of Texas at Austin, Southern Univertisy Baton Rouge, Univ. of Arkansas, Univ. of Central Florida, JQI, NIST and Univ. of Maryland, UT Austin, Center for Ultrafast Optical Science, University of Michigan, Lawrence Berkeley National Laboratory, University of Texas at Austin, Lockheed Martin, NASA, South Plains College, LBNL-ALS, Berkeley, Denison U., Granville, U. of Nevada, Reno, Justus-Liebig-Universitat, Giessen, Western Michigan U., Kalamazoo, University of Texas at Austin, Department of Physics, Institute for Applied Physics, University of Muenster