Rebecca Oppenheimer CV
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A Selected Bibliography of Publications By, and About, J
A Selected Bibliography of Publications by, and about, J. Robert Oppenheimer Nelson H. F. Beebe University of Utah Department of Mathematics, 110 LCB 155 S 1400 E RM 233 Salt Lake City, UT 84112-0090 USA Tel: +1 801 581 5254 FAX: +1 801 581 4148 E-mail: [email protected], [email protected], [email protected] (Internet) WWW URL: http://www.math.utah.edu/~beebe/ 17 March 2021 Version 1.47 Title word cross-reference $1 [Duf46]. $12.95 [Edg91]. $13.50 [Tho03]. $14.00 [Hug07]. $15.95 [Hen81]. $16.00 [RS06]. $16.95 [RS06]. $17.50 [Hen81]. $2.50 [Opp28g]. $20.00 [Hen81, Jor80]. $24.95 [Fra01]. $25.00 [Ger06]. $26.95 [Wol05]. $27.95 [Ger06]. $29.95 [Goo09]. $30.00 [Kev03, Kle07]. $32.50 [Edg91]. $35 [Wol05]. $35.00 [Bed06]. $37.50 [Hug09, Pol07, Dys13]. $39.50 [Edg91]. $39.95 [Bad95]. $8.95 [Edg91]. α [Opp27a, Rut27]. γ [LO34]. -particles [Opp27a]. -rays [Rut27]. -Teilchen [Opp27a]. 0-226-79845-3 [Guy07, Hug09]. 0-8014-8661-0 [Tho03]. 0-8047-1713-3 [Edg91]. 0-8047-1714-1 [Edg91]. 0-8047-1721-4 [Edg91]. 0-8047-1722-2 [Edg91]. 0-9672617-3-2 [Bro06, Hug07]. 1 [Opp57f]. 109 [Con05, Mur05, Nas07, Sap05a, Wol05, Kru07]. 112 [FW07]. 1 2 14.99/$25.00 [Ber04a]. 16 [GHK+96]. 1890-1960 [McG02]. 1911 [Meh75]. 1945 [GHK+96, Gow81, Haw61, Bad95, Gol95a, Hew66, She82, HBP94]. 1945-47 [Hew66]. 1950 [Ano50]. 1954 [Ano01b, GM54, SZC54]. 1960s [Sch08a]. 1963 [Kuh63]. 1967 [Bet67a, Bet97, Pun67, RB67]. 1976 [Sag79a, Sag79b]. 1981 [Ano81]. 20 [Goe88]. 2005 [Dre07]. 20th [Opp65a, Anoxx, Kai02]. -
Exoplanet.Eu Catalog Page 1 # Name Mass Star Name
exoplanet.eu_catalog # name mass star_name star_distance star_mass OGLE-2016-BLG-1469L b 13.6 OGLE-2016-BLG-1469L 4500.0 0.048 11 Com b 19.4 11 Com 110.6 2.7 11 Oph b 21 11 Oph 145.0 0.0162 11 UMi b 10.5 11 UMi 119.5 1.8 14 And b 5.33 14 And 76.4 2.2 14 Her b 4.64 14 Her 18.1 0.9 16 Cyg B b 1.68 16 Cyg B 21.4 1.01 18 Del b 10.3 18 Del 73.1 2.3 1RXS 1609 b 14 1RXS1609 145.0 0.73 1SWASP J1407 b 20 1SWASP J1407 133.0 0.9 24 Sex b 1.99 24 Sex 74.8 1.54 24 Sex c 0.86 24 Sex 74.8 1.54 2M 0103-55 (AB) b 13 2M 0103-55 (AB) 47.2 0.4 2M 0122-24 b 20 2M 0122-24 36.0 0.4 2M 0219-39 b 13.9 2M 0219-39 39.4 0.11 2M 0441+23 b 7.5 2M 0441+23 140.0 0.02 2M 0746+20 b 30 2M 0746+20 12.2 0.12 2M 1207-39 24 2M 1207-39 52.4 0.025 2M 1207-39 b 4 2M 1207-39 52.4 0.025 2M 1938+46 b 1.9 2M 1938+46 0.6 2M 2140+16 b 20 2M 2140+16 25.0 0.08 2M 2206-20 b 30 2M 2206-20 26.7 0.13 2M 2236+4751 b 12.5 2M 2236+4751 63.0 0.6 2M J2126-81 b 13.3 TYC 9486-927-1 24.8 0.4 2MASS J11193254 AB 3.7 2MASS J11193254 AB 2MASS J1450-7841 A 40 2MASS J1450-7841 A 75.0 0.04 2MASS J1450-7841 B 40 2MASS J1450-7841 B 75.0 0.04 2MASS J2250+2325 b 30 2MASS J2250+2325 41.5 30 Ari B b 9.88 30 Ari B 39.4 1.22 38 Vir b 4.51 38 Vir 1.18 4 Uma b 7.1 4 Uma 78.5 1.234 42 Dra b 3.88 42 Dra 97.3 0.98 47 Uma b 2.53 47 Uma 14.0 1.03 47 Uma c 0.54 47 Uma 14.0 1.03 47 Uma d 1.64 47 Uma 14.0 1.03 51 Eri b 9.1 51 Eri 29.4 1.75 51 Peg b 0.47 51 Peg 14.7 1.11 55 Cnc b 0.84 55 Cnc 12.3 0.905 55 Cnc c 0.1784 55 Cnc 12.3 0.905 55 Cnc d 3.86 55 Cnc 12.3 0.905 55 Cnc e 0.02547 55 Cnc 12.3 0.905 55 Cnc f 0.1479 55 -
CHARACTERIZATION of the COMPANION Μ HER Lewis C
The Astronomical Journal, 151:169 (7pp), 2016 June doi:10.3847/0004-6256/151/6/169 © 2016. The American Astronomical Society. All rights reserved. CHARACTERIZATION OF THE COMPANION μ HER Lewis C. Roberts Jr.1, Brian D. Mason2, Jonathan Aguilar3, Joseph Carson4, Justin Crepp5, Charles Beichman1,6,7, Douglas Brenner8, Rick Burruss1, Eric Cady1, Statia Luszcz-Cook8, Richard Dekany6, Lynne Hillenbrand6, Sasha Hinkley9, David King10, Thomas G. Lockhart1, Ricky Nilsson8,11, Rebecca Oppenheimer8, Ian R. Parry10, Laurent Pueyo3,12, Emily L. Rice13, Anand Sivaramakrishnan12, Rémi Soummer12, Gautam Vasisht1, Aaron Veicht8, Ji Wang14, Chengxing Zhai1, and Neil T. Zimmerman15 1 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena CA 91109, USA 2 U.S. Naval Observatory, 3450 Massachusetts Avenue, NW, Washington, DC 20392-5420, USA 3 Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA 4 Department of Physics & Astronomy, College of Charleston, 58 Coming Street, Charleston, SC 29424, USA 5 Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN, 46556, USA 6 Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA 7 NASA Exoplanet Science Institute, 770 S. Wilson Avenue, Pasadena, CA 911225, USA 8 American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024, USA 9 School of Physics, University of Exeter, Stocker Road, Exeter, EX4 4QL, UK 10 Institute of Astronomy, University -
New Sub-Millimeter Limits on Dust in the 55 Cancri Planetary System
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server New sub-millimeter limits on dust in the 55 Cancri planetary system Ray Jayawardhana1, Wayne S. Holland2, Paul Kalas1,JaneS.Greaves2, William R. F. Dent2,MarkC.Wyatt2, and Geoffrey W. Marcy1 ABSTRACT We present new, high-sensitivity sub-millimeter observations towards 55 Can- cri, a nearby G8 star with one, or possibly two, known planetary companion(s). Our 850 µm map, obtained with the SCUBA instrument on the James Clerk Maxwell Telescope, shows three peaks of emission at the 2.5 mJy level in the vicinity of the star’s position. However, the observed peaks are 2500–4000 away from the star and a deep R-band optical image reveals faint point sources that coincide with two of the sub-millimeter peaks. Thus, we do not find evidence for dust emission spatially associated with 55 Cancri. The excess 60 µmemis- sion detected with ISO may originate from one or more of the 850 µmpeaks that we attribute to background sources. Our new results, together with the HST/NICMOS coronographic images in the near-infrared, place stringent limits on the amount of dust in this planetary system, and argue against the existence of a detectable circumstellar dust disk around 55 Cnc. Subject headings: planetary systems – stars : individual (55 Cnc) – circumstellar matter 1. Introduction Dusty disks that are believed to be the debris of planetary formation have now been imaged at infrared and sub-millimeter wavelengths around several nearby main-sequence stars including β Pictoris, HR 4796A, Vega, Fomalhaut and Eridani (Smith & Terrile 1984; Holland et al. -
Exoplanet Meteorology: Characterizing the Atmospheres Of
Exoplanet Meteorology: Characterizing the Atmospheres of Directly Imaged Sub-Stellar Objects by Abhijith Rajan A Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy Approved April 2017 by the Graduate Supervisory Committee: Jennifer Patience, Co-Chair Patrick Young, Co-Chair Paul Scowen Nathaniel Butler Evgenya Shkolnik ARIZONA STATE UNIVERSITY May 2017 ©2017 Abhijith Rajan All Rights Reserved ABSTRACT The field of exoplanet science has matured over the past two decades with over 3500 confirmed exoplanets. However, many fundamental questions regarding the composition, and formation mechanism remain unanswered. Atmospheres are a window into the properties of a planet, and spectroscopic studies can help resolve many of these questions. For the first part of my dissertation, I participated in two studies of the atmospheres of brown dwarfs to search for weather variations. To understand the evolution of weather on brown dwarfs we conducted a multi- epoch study monitoring four cool brown dwarfs to search for photometric variability. These cool brown dwarfs are predicted to have salt and sulfide clouds condensing in their upper atmosphere and we detected one high amplitude variable. Combining observations for all T5 and later brown dwarfs we note a possible correlation between variability and cloud opacity. For the second half of my thesis, I focused on characterizing the atmospheres of directly imaged exoplanets. In the first study Hubble Space Telescope data on HR8799, in wavelengths unobservable from the ground, provide constraints on the presence of clouds in the outer planets. Next, I present research done in collaboration with the Gemini Planet Imager Exoplanet Survey (GPIES) team including an exploration of the instrument contrast against environmental parameters, and an examination of the environment of the planet in the HD 106906 system. -
HD 165054: an Astrometric Calibration Field for High-Contrast Imagers In
Draft version April 8, 2020 Typeset using LATEX twocolumn style in AASTeX63 HD 165054: an astrometric calibration field for high-contrast imagers in Baade's Window 1 2, 3 4, 1 1, 5 Meiji M. Nguyen, Robert J. De Rosa, Jason J. Wang, ∗ Thomas M. Esposito, Paul Kalas, James R. Graham,1 Bruce Macintosh,3 Vanessa P. Bailey,6 Travis Barman,7 Joanna Bulger,8, 9 Jeffrey Chilcote,10 Tara Cotten,11 Rene Doyon,12 Gaspard Duchene^ ,1, 13 Michael P. Fitzgerald,14 Katherine B. Follette,15 Benjamin L. Gerard,16, 17 Stephen J. Goodsell,18 Alexandra Z. Greenbaum,19 Pascale Hibon,2 Justin Hom,20 Li-Wei Hung,21 Patrick Ingraham,22 Quinn Konopacky,23 James E. Larkin,14 Jer´ ome^ Maire,23 Franck Marchis,5 Mark S. Marley,24 Christian Marois,17, 16 Stanimir Metchev,25, 26 6, 3 27 28 Maxwell A. Millar-Blanchaer, y Eric L. Nielsen, Rebecca Oppenheimer, David Palmer, Jennifer Patience,20 Marshall Perrin,29 Lisa Poyneer,28 Laurent Pueyo,29 Abhijith Rajan,29 Julien Rameau,13, 12 Fredrik T. Rantakyro¨,30 Bin Ren,31 Jean-Baptiste Ruffio,3 Dmitry Savransky,32 Adam C. Schneider,20 Anand Sivaramakrishnan,29 Inseok Song,11 Remi Soummer,29 Melisa Tallis,3 Sandrine Thomas,22 J. Kent Wallace,6 Kimberly Ward-Duong,15 Sloane Wiktorowicz,33 and Schuyler Wolff34 1Department of Astronomy, University of California, Berkeley, CA 94720, USA 2European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile 3Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305, USA 4Department of Astronomy, California Institute of Technology, -
UC San Diego UC San Diego Electronic Theses and Dissertations
UC San Diego UC San Diego Electronic Theses and Dissertations Title The new prophet : Harold C. Urey, scientist, atheist, and defender of religion Permalink https://escholarship.org/uc/item/3j80v92j Author Shindell, Matthew Benjamin Publication Date 2011 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA, SAN DIEGO The New Prophet: Harold C. Urey, Scientist, Atheist, and Defender of Religion A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in History (Science Studies) by Matthew Benjamin Shindell Committee in charge: Professor Naomi Oreskes, Chair Professor Robert Edelman Professor Martha Lampland Professor Charles Thorpe Professor Robert Westman 2011 Copyright Matthew Benjamin Shindell, 2011 All rights reserved. The Dissertation of Matthew Benjamin Shindell is approved, and it is acceptable in quality and form for publication on microfilm and electronically: ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ Chair University of California, San Diego 2011 iii TABLE OF CONTENTS Signature Page……………………………………………………………………...... iii Table of Contents……………………………………………………………………. iv Acknowledgements…………………………………………………………………. -
Ethical Standards in Astronomy
Ethical standards in astronomy Decadal Survey State of the Profession Position Paper 15 March 2009 Paul Kalas University of California, Berkeley (510) 642‐8285 [email protected] November, 2008 Cover Art: Cartoon indicating that the integrity of all professional astronomers and astronomy as a scientific discipline depends on the responsible analysis and dissemination of primary data. Though photoshopping an astronomical observation, or “fabrication” in general, may seem unprecedented, evidence shows that modern scientists have been doing it for decades, and research misconduct receives wide public attention, when caught. It is telling that cases of fabrication are typically discovered by junior colleagues and/or science writers, rather than senior scientists or institutional entities. Arguably the professional penalties are mild relative to the wider damage done. The response that science is self-correcting is valid, yet resources are wasted to disprove results from unprofessional research. ABSTRACT Ethical conduct in astronomical research and education underlies the integrity of the profession. Here we present a brief discussion of three areas where ethics training and awareness can be improved and result in substantial benefits: A) authorship and publication practices, B) data and the research record, and C) protection of the environment. Further reading on these and other important topics not included here may be found at: http://astro.berkeley.edu/~kalas/ethics/pages/lectures.html 1. INTRODUCTION Dozens of comprehensive books have been published within the past 20 years concerning ethical issues and responsible conduct in scientific research. Ethics guidelines and training have been established for the medical professions, engineering, and other disciplines involving human subjects. -
VITA David Jewitt Address Dept. Earth, Planetary and Space
VITA David Jewitt Address Dept. Earth, Planetary and Space Sciences, UCLA 595 Charles Young Drive East, Box 951567 Los Angeles, CA 90095-1567 [email protected], http://www2.ess.ucla.edu/~jewitt/ Education B. Sc. University College London 1979 M. S. California Institute of Technology 1980 Ph. D. California Institute of Technology 1983 Professional Experience Summer Student Royal Greenwich Observatory 1978 Anthony Fellowship California Institute of Technology 1979-1980 Research Assistant California Institute of Technology 1980-1983 Assistant Professor Massachusetts Institute of Technology 1983-1988 Associate Professor and Astronomer University of Hawaii 1988-1993 Professor and Astronomer University of Hawaii 1993-2009 Professor Dept. Earth, Planetary & Space Sciences, UCLA 2009- Inst. of Geophys & Planetary Physics, UCLA 2009-2011 Dept. Physics & Astronomy, UCLA 2010- Director Institute for Planets & Exoplanets, UCLA, 2011- Honors Regent's Medal, University of Hawaii 1994 Scientist of the Year, ARCS 1996 Exceptional Scientific Achievement Award, NASA 1996 Fellow of University College London 1998 Fellow of the American Academy of Arts and Sciences 2005 Fellow of the American Association for the Advancement of Science 2005 Member of the National Academy of Sciences 2005 National Observatory, Chinese Academy of Sciences, Honorary Professor 2006-2011 National Central University, Taiwan, Adjunct Professor 2007 The Shaw Prize for Astronomy 2012 The Kavli Prize for Astrophysics 2012 Foreign Member, Norwegian Academy of Sciences & Letters 2012 Research -
Max-Planck-Institut Für Astronomie 26.02.09 11:43
Max-Planck-Institut für Astronomie 26.02.09 11:43 Planeten- und Sternentstehung/ Planet and Star Formation (2007) Refereed Papers Adelman-McCarthy, J. K., M. A. Agüeros, S. S. Allam, K. S. J. Anderson, S. F. Anderson, J. Annis, N. A. Bahcall, C. A. L. Bailer-Jones, I. K. Baldry, J. C. Barentine, T. C. Beers, V. Belokurov, A. Berlind, M. Bernardi, M. R. Blanton, J. J. Bochanski, W. N. Boroski, D. M. Bramich, H. J. Brewington, J. Brinchmann, J. Brinkmann, R. J. Brunner, T. Budavári, L. N. Carey, S. Carliles, M. A. Carr, F. J. Castander, A. J. Connolly, R. J. Cool, C. E. Cunha, I. Csabai, J. J. Dalcanton, M. Doi, D. J. Eisenstein, M. L. Evans, N. W. Evans, X. Fan, D. P. Finkbeiner, S. D. Friedman, J. A. Frieman, M. Fukugita, B. Gillespie, G. Gilmore, K. Glazebrook, J. Gray, E. K. Grebel, J. E. Gunn, E. de Haas, P. B. Hall, M. Harvanek, S. L. Hawley, J. Hayes, T. M. Heckman, J. S. Hendry, G. S. Hennessy, R. B. Hindsley, C. M. Hirata, C. J. Hogan, D. W. Hogg, J. A. Holtzman, S.-i. Ichikawa, T. Ichikawa, Z. Ivezic, S. Jester, D. E. Johnston, A. M. Jorgensen, M. Juric, G. Kauffmann, S. M. Kent, S. J. Kleinman, G. R. Knapp, A. Y. Kniazev, R. G. Kron, J. Krzesinski, N. Kuropatkin, D. Q. Lamb, H. Lampeitl, B. C. Lee, R. F. Leger, M. Lima, H. Lin, D. C. Long, J. Loveday, R. H. Lupton, R. Mandelbaum, B. Margon, D. Martínez-Delgado, T. Matsubara, P. M. McGehee, T. -
A PLANET-SCULPTING SCENARIO for the HD 61005 DEBRIS DISK
UCLA UCLA Previously Published Works Title BRINGING "tHE MOTH" to LIGHT: A PLANET-SCULPTING SCENARIO for the HD 61005 DEBRIS DISK Permalink https://escholarship.org/uc/item/1h77k16g Journal Astronomical Journal, 152(4) ISSN 0004-6256 Authors Esposito, TM Fitzgerald, MP Graham, JR et al. Publication Date 2016-10-01 DOI 10.3847/0004-6256/152/4/85 Peer reviewed eScholarship.org Powered by the California Digital Library University of California The Astronomical Journal, 152:85 (16pp), 2016 October doi:10.3847/0004-6256/152/4/85 © 2016. The American Astronomical Society. All rights reserved. BRINGING “THE MOTH” TO LIGHT: A PLANET-SCULPTING SCENARIO FOR THE HD 61005 DEBRIS DISK Thomas M. Esposito1,2, Michael P. Fitzgerald1, James R. Graham2, Paul Kalas2,3, Eve J. Lee2, Eugene Chiang2, Gaspard Duchêne2,4, Jason Wang2, Maxwell A. Millar-Blanchaer5,6, Eric Nielsen3,7, S. Mark Ammons8, Sebastian Bruzzone9, Robert J. De Rosa2, Zachary H. Draper10,11, Bruce Macintosh7, Franck Marchis3, Stanimir A. Metchev9,12, Marshall Perrin13, Laurent Pueyo13, Abhijith Rajan14, Fredrik T. Rantakyrö15, David Vega3, and Schuyler Wolff16 1 Department of Physics and Astronomy, 430 Portola Plaza, University of California, Los Angeles, CA 90095-1547, USA; [email protected] 2 Department of Astronomy, University of California, Berkeley, CA 94720, USA 3 SETI Institute, Carl Sagan Center, 189 Bernardo Avenue, Mountain View, CA 94043, USA 4 Université Grenoble Alpes/CNRS, Institut de Planétologie et d’Astrophysique de Grenoble, F-38000 Grenoble, France 5 Department of -
Exoplanet.Eu Catalog Page 1 Star Distance Star Name Star Mass
exoplanet.eu_catalog star_distance star_name star_mass Planet name mass 1.3 Proxima Centauri 0.120 Proxima Cen b 0.004 1.3 alpha Cen B 0.934 alf Cen B b 0.004 2.3 WISE 0855-0714 WISE 0855-0714 6.000 2.6 Lalande 21185 0.460 Lalande 21185 b 0.012 3.2 eps Eridani 0.830 eps Eridani b 3.090 3.4 Ross 128 0.168 Ross 128 b 0.004 3.6 GJ 15 A 0.375 GJ 15 A b 0.017 3.6 YZ Cet 0.130 YZ Cet d 0.004 3.6 YZ Cet 0.130 YZ Cet c 0.003 3.6 YZ Cet 0.130 YZ Cet b 0.002 3.6 eps Ind A 0.762 eps Ind A b 2.710 3.7 tau Cet 0.783 tau Cet e 0.012 3.7 tau Cet 0.783 tau Cet f 0.012 3.7 tau Cet 0.783 tau Cet h 0.006 3.7 tau Cet 0.783 tau Cet g 0.006 3.8 GJ 273 0.290 GJ 273 b 0.009 3.8 GJ 273 0.290 GJ 273 c 0.004 3.9 Kapteyn's 0.281 Kapteyn's c 0.022 3.9 Kapteyn's 0.281 Kapteyn's b 0.015 4.3 Wolf 1061 0.250 Wolf 1061 d 0.024 4.3 Wolf 1061 0.250 Wolf 1061 c 0.011 4.3 Wolf 1061 0.250 Wolf 1061 b 0.006 4.5 GJ 687 0.413 GJ 687 b 0.058 4.5 GJ 674 0.350 GJ 674 b 0.040 4.7 GJ 876 0.334 GJ 876 b 1.938 4.7 GJ 876 0.334 GJ 876 c 0.856 4.7 GJ 876 0.334 GJ 876 e 0.045 4.7 GJ 876 0.334 GJ 876 d 0.022 4.9 GJ 832 0.450 GJ 832 b 0.689 4.9 GJ 832 0.450 GJ 832 c 0.016 5.9 GJ 570 ABC 0.802 GJ 570 D 42.500 6.0 SIMP0136+0933 SIMP0136+0933 12.700 6.1 HD 20794 0.813 HD 20794 e 0.015 6.1 HD 20794 0.813 HD 20794 d 0.011 6.1 HD 20794 0.813 HD 20794 b 0.009 6.2 GJ 581 0.310 GJ 581 b 0.050 6.2 GJ 581 0.310 GJ 581 c 0.017 6.2 GJ 581 0.310 GJ 581 e 0.006 6.5 GJ 625 0.300 GJ 625 b 0.010 6.6 HD 219134 HD 219134 h 0.280 6.6 HD 219134 HD 219134 e 0.200 6.6 HD 219134 HD 219134 d 0.067 6.6 HD 219134 HD