Pro-Am Photometry Projects with Robotic Observatories
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INFRARED TRANSMISSION SPECTROSCOPY of the EXOPLANETS HD 209458B and XO-1B USING the WIDE FIELD CAMERA-3 on the HUBBLE SPACE TELESCOPE
INFRARED TRANSMISSION SPECTROSCOPY OF THE EXOPLANETS HD 209458b AND XO-1b USING THE WIDE FIELD CAMERA-3 ON THE HUBBLE SPACE TELESCOPE The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Deming, Drake, Ashlee Wilkins, Peter McCullough, Adam Burrows, Jonathan J. Fortney, Eric Agol, Ian Dobbs-Dixon, et al. “INFRARED TRANSMISSION SPECTROSCOPY OF THE EXOPLANETS HD 209458b AND XO-1b USING THE WIDE FIELD CAMERA-3 ON THE HUBBLE SPACE TELESCOPE.” The Astrophysical Journal 774, no. 2 (September 10, 2013): 95. As Published http://dx.doi.org/10.1088/0004-637X/774/2/95 Publisher IOP Publishing Version Author's final manuscript Citable link http://hdl.handle.net/1721.1/81284 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike 3.0 Detailed Terms http://creativecommons.org/licenses/by-nc-sa/3.0/ Accepted for the Astrophysical Journal, July 10, 2013 A Preprint typeset using L TEX style emulateapj v. 11/12/01 INFRARED TRANSMISSION SPECTROSCOPY OF THE EXOPLANETS HD 209458B AND XO-1B USING THE WIDE FIELD CAMERA-3 ON THE HUBBLE SPACE TELESCOPE Drake Deming1,2, Ashlee Wilkins1, Peter McCullough3, Adam Burrows4, Jonathan J. Fortney5, Eric Agol6, Ian Dobbs-Dixon6,7, Nikku Madhusudhan8, Nicolas Crouzet3, Jean-Michel Desert9,10, Ronald L. Gilliland11, Korey Haynes12,13, Heather A. Knutson9, Michael Line9, Zazralt Magic14,15, Avi M. Mandell13, Sukrit Ranjan16, David Charbonneau16, Mark Clampin13, Sara Seager17, and Adam P. Showman18 Accepted for the Astrophysical Journal, July 10, 2013 ABSTRACT Exoplanetary transmission spectroscopy in the near-infrared using Hubble/NICMOS is currently am- biguous because different observational groups claim different results from the same data, depending on their analysis methodologies. -
Infrared Spectroscopy of the Exoplanets Corot-2B, XO-1B, HD 209458B Using the Wide-Field Camera-3 on the Hubble Space Telescope
Geophysical Research Abstracts Vol. 15, EGU2013-10914-1, 2013 EGU General Assembly 2013 © Author(s) 2013. CC Attribution 3.0 License. Infrared Spectroscopy of the Exoplanets CoRoT-2b, XO-1b, HD 209458b Using the Wide-Field Camera-3 On the Hubble Space Telescope Ashlee Wilkins (1), Drake Deming (1), Peter McCullough (2), Adam Burrows (3), Nikku Madhusudhan (4), Jonathan Fortney (5), Jean-Michel Desert (6,7), Ronald Gilliland (8), Korey Haynes (9,10) (1) Department of Astronomy, University of Maryland, College Park, MD, United States ([email protected]), (2) Space Telescope Science Institute, Baltimore, MD, United States, (3) Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA, (4) Yale Center for Astronomy & Astrophysics, Yale University, New Haven, CT, USA, (5) Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA, USA, (6) Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA, (7) Sagan Fellow, (8) Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, PA, USA, (9) Department of Physics and Astronomy, George Mason University, Fairfax, VA, USA, (10) NASA’s Goddard Space Flight Center, Greenbelt, MD, USA Exoplanetary transmisison spectroscopy requires exquisite precision of measurement. Due to telluric water vapor, reliable detections of water vapor in exoplanets is practical only with space-based instruments, such as the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST). With this work, we present HST WFC3 grism spectroscopy of two hot Jupiters, HD209458b and XO-1b in transit, and one very hot Jupiter, CoRoT-2b, in sec- ondary eclipse, in the wavelength range of 1.1-1.7 µm. -
Cover Page/Proposal Summary the XO Planet Finding System Peter R
Cover Page/Proposal Summary The XO Planet Finding System Peter R. McCullough Jeff Valenti Chris Johns-Krull Kenneth Janes James N. Heasley We describe a three year plan to continue discovering and characterizing planets that transit bright stars. To date, astronomers have reported more than 25 such transiting planets orbiting bright stars, and their numbers are increasing rapidly (both the number of planets and the number of astronomers studying them). The brightest typically are discovered by oscillating radial velocities, and somewhat fainter ones in much larger numbers are discovered by transits. The XO observatory has recently been expanded to six 0.1-meter diameter cameras, two of which have been operating robotically on Haleakala, Maui, HI since Sep 2003 and with which we have discovered five transiting planets. We evaluate transiting-planet candidates produced by the XO survey cameras with precise photometric observations, which significantly reduces the number of candidates we observe spectroscopically. For the follow-up photometry, we have recruited a global network of privately-funded and operated observatories, in addition to our team's institutional access to observatories in Hawaii, Texas, and Arizona. Dozens of candidates per year will be scrutinized with moderate-precision (∼1 km/s) radial velocity observations and a few of those will be confirmed to be planets with (∼10 m/s) precision. We will pursue precise photometric and spectroscopic follow up observations of transiting planets discovered by XO, HAT, WASP, etc. Our team has prior experience with scintillation- limited ground-based photometry, time-series photometry with SST IRAC, spectrophotometry with HST instruments NICMOS, STIS, ACS, and WFC3 (in ground-tests), and is developing spectroscopic analysis techniques to improve the precision of radial velocities from Keck and HET. -
Spitzer Approved Warm Mission Abstracts
Printed by SSC Jan 29, 20 19:21 Spitzer Approved Warm Mission Abstracts Page 1/750 Jan 29, 20 19:21 Spitzer Approved Warm Mission Abstracts Page 2/750 Spitzer Space Telescope − Directors Discretionary Time Proposal #13159 Spitzer Space Telescope − General Observer Proposal #60167 Variability at the edge: highly accreting objects in Taurus Disk tomography and dynamics: a time−dependent study of known mid−infrared Principal Investigator: Peter Abraham variable young stellar objects Institution: Konkoly Observatory Principal Investigator: Peter Abraham Technical Contact: Peter Abraham, Konkoly Observatory Institution: Konkoly Observatory of the Hungarian Academy of Science Co−Investigators: Technical Contact: Peter Abraham, Konkoly Observatory of the Hungarian Agnes Kospal, Konkoly Observatory Academy of Science Robert Szabo, Konkoly Observatory Co−Investigators: Science Category: YSOs Jose Acosta−Pulido, Instituto de Astrofisica de Canarias Observing Modes: IRAC Post−Cryo Mapping Cornelis P. Dullemond, Max−Planck−Institut fur Astronomie Hours Approved: 9.3 Carol A. Grady, Eureka Sci/NASA Goddard Thomas Henning, Max−Planck−Institut fur Astronomie Abstract: Attila Juhasz, Max−Planck−Institut fur Astronomie In Kepler K2, Campaign 13, we will obtain 80−days−long optical light curves of Csaba Kiss, Konkoly Observatory seven highly accreting T Tauri stars in the benchmark Taurus star forming Agnes Kospal, Leiden Observatory region. Here we propose to monitor our sample simultaneously with Kepler and Maria Kun, Konkoly Observatory Spitzer, to -
From Giant Planets to Super Earths Program and Abstracts
Exploring Strange New Worlds: From Giant Planets to Super Earths May 1 - 6, 2011 High Country Conference Center Flagstaff, Arizona Program and Abstracts Table of Contents Organizing Committees……………………………………………………. ……... 3 Conference Sponsors………………………………………………………………. 4 Conference Agenda………………………………………………………………… 5 Monday……………………………………………………………….... 5 Tuesday………………………………………………………….…....... 6 Wednesday……………………………………………………………... 7 Thursday……………………………………………………………….. 8 Friday…………………………………………………………………... 9 Poster for Geoff Marcy’s Public Lecture on Monday Evening……………………. 10 Table of Posters in Alphabetical Order by Author…….………………………....... 11 Table of Posters by Science Category……………….……………………….......... 17 List of Conference Participants…………………………………………………….. 23 Invited and Contributed Talk Abstracts in Agenda Order…………………………. 29 Poster Abstracts by Science Category……………………………………………... 70 Disks…………………………………………………………………… 70 Exoplanet Characterization…………………………………………….. 77 Habitability…………………………………………………………….. 90 Missions………………………………………………………………... 95 Planet Formation……………………………………………………….. 110 Planet-hosting Stars…………………………………………………..... 114 Planetary System Architecture…………………………………………. 120 Author Index……………………………………………………………………….. 129 Table of Contents Exploring Strange New Worlds | 3 Scientific Organizing Committee Charles Beichman, NExScI, California Institute of Technology (Co-chair) Malcolm Fridlund, European Space Agency (Co-chair) Willie Benz, Observatoire de Besancon Adam Burrows, Princeton University Mark Clampin, Goddard Space Flight