BRAS Newsletter October 2013
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Lurking in the Shadows: Wide-Separation Gas Giants As Tracers of Planet Formation
Lurking in the Shadows: Wide-Separation Gas Giants as Tracers of Planet Formation Thesis by Marta Levesque Bryan In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2018 Defended May 1, 2018 ii © 2018 Marta Levesque Bryan ORCID: [0000-0002-6076-5967] All rights reserved iii ACKNOWLEDGEMENTS First and foremost I would like to thank Heather Knutson, who I had the great privilege of working with as my thesis advisor. Her encouragement, guidance, and perspective helped me navigate many a challenging problem, and my conversations with her were a consistent source of positivity and learning throughout my time at Caltech. I leave graduate school a better scientist and person for having her as a role model. Heather fostered a wonderfully positive and supportive environment for her students, giving us the space to explore and grow - I could not have asked for a better advisor or research experience. I would also like to thank Konstantin Batygin for enthusiastic and illuminating discussions that always left me more excited to explore the result at hand. Thank you as well to Dimitri Mawet for providing both expertise and contagious optimism for some of my latest direct imaging endeavors. Thank you to the rest of my thesis committee, namely Geoff Blake, Evan Kirby, and Chuck Steidel for their support, helpful conversations, and insightful questions. I am grateful to have had the opportunity to collaborate with Brendan Bowler. His talk at Caltech my second year of graduate school introduced me to an unexpected population of massive wide-separation planetary-mass companions, and lead to a long-running collaboration from which several of my thesis projects were born. -
A Temperate Rocky Super-Earth Transiting a Nearby Cool Star Jason A
LETTER doi:10.1038/nature22055 A temperate rocky super-Earth transiting a nearby cool star Jason A. Dittmann1, Jonathan M. Irwin1, David Charbonneau1, Xavier Bonfils2,3, Nicola Astudillo-Defru4, Raphaëlle D. Haywood1, Zachory K. Berta-Thompson5, Elisabeth R. Newton6, Joseph E. Rodriguez1, Jennifer G. Winters1, Thiam-Guan Tan7, Jose-Manuel Almenara2,3,4, François Bouchy8, Xavier Delfosse2,3, Thierry Forveille2,3, Christophe Lovis4, Felipe Murgas2,3,9, Francesco Pepe4, Nuno C. Santos10,11, Stephane Udry4, Anaël Wünsche2,3, Gilbert A. Esquerdo1, David W. Latham1 & Courtney D. Dressing12 15 16,17 M dwarf stars, which have masses less than 60 per cent that of Ks magnitude and empirically determined stellar relationships , the Sun, make up 75 per cent of the population of the stars in the we estimate the stellar mass to be 14.6% that of the Sun and the stellar Galaxy1. The atmospheres of orbiting Earth-sized planets are radius to be 18.6% that of the Sun. We estimate the metal content of the observationally accessible via transmission spectroscopy when star to be approximately half that of the Sun ([Fe/H] = −0.24 ± 0.10; the planets pass in front of these stars2,3. Statistical results suggest 1σ error), and we measure the rotational period of the star to be that the nearest transiting Earth-sized planet in the liquid-water, 131 days from our long-term photometric monitoring (see Methods). habitable zone of an M dwarf star is probably around 10.5 parsecs On 15 September 2014 ut, MEarth-South identified a potential away4. A temperate planet has been discovered orbiting Proxima transit in progress around LHS 1140, and automatically commenced Centauri, the closest M dwarf5, but it probably does not transit and high-cadence follow-up observations (see Extended Data Fig. -
Musical Composition Graduate Portfolio
University of Northern Iowa UNI ScholarWorks Dissertations and Theses @ UNI Student Work 2021 Musical composition graduate portfolio Juan Marulanda University of Northern Iowa Let us know how access to this document benefits ouy Copyright ©2021 Juan Marulanda Follow this and additional works at: https://scholarworks.uni.edu/etd Recommended Citation Marulanda, Juan, "Musical composition graduate portfolio" (2021). Dissertations and Theses @ UNI. 1102. https://scholarworks.uni.edu/etd/1102 This Open Access Thesis is brought to you for free and open access by the Student Work at UNI ScholarWorks. It has been accepted for inclusion in Dissertations and Theses @ UNI by an authorized administrator of UNI ScholarWorks. For more information, please contact [email protected]. Copyright by JUAN MARULANDA 2021 All Rights Reserved MUSICAL COMPOSITION GRADUATE PORTFOLIO An Abstract Submitted in Partial Fulfillment of the Requirements for the Degree Master of Music Juan Marulanda University of Northern Iowa May 2021 This Study By: Juan Carlos Marulanda Entitled: Musical Composition Graduate Portfolio has been approved as meeting the thesis requirement for the Degree of Master of Music: Composition Date Dr. Daniel Swilley, Chair, Recital Committee Date Dr. Michael Conrad, Recital Committee Member Date Dr. Jonathan Schwabe, Recital Committee Member Date Dr. Jennifer Waldron, Dean, Graduate College This Recital Performance By: Juan Marulanda Entitled: Musical Composition Graduate Portfolio has been approved as meeting the thesis requirement for the Degree of Master of Music: Composition Date Dr. Daniel Swilley, Chair, Recital Committee Date Dr. Michael Conrad, Recital Committee Member Date Dr. Jonathan Schwabe, Recital Committee Member Date Dr. Jennifer Waldron, Dean, Graduate College ABSTRACT The musical works included in this portfolio were composed between Fall 2019 and Spring 2021. -
An Extreme Planetary System Around HD 219828 One Long-Period Super Jupiter to a Hot-Neptune Host Star?,??
A&A 592, A13 (2016) Astronomy DOI: 10.1051/0004-6361/201628374 & c ESO 2016 Astrophysics An extreme planetary system around HD 219828 One long-period super Jupiter to a hot-Neptune host star?,?? N. C. Santos1; 2, A. Santerne1, J. P. Faria1; 2, J. Rey3, A. C. M. Correia4; 5, J. Laskar5, S. Udry3, V. Adibekyan1, F. Bouchy3; 6, E. Delgado-Mena1, C. Melo7, X. Dumusque3, G. Hébrard8; 9, C. Lovis3, M. Mayor3, M. Montalto1, A. Mortier10, F. Pepe3, P. Figueira1, J. Sahlmann11, D. Ségransan3, and S. G. Sousa1 1 Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal e-mail: [email protected] 2 Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre, 4169-007 Porto, Portugal 3 Observatoire de Genève, Université de Genève, 51 ch. des Maillettes, 1290 Sauverny, Switzerland 4 CIDMA, Departamento de Física, Universidade de Aveiro, Campus de Santiago, 3810-193 Aveiro, Portugal 5 ASD, IMCCE-CNRS UMR 8028, Observatoire de Paris, PSL Research University, 77 Av. Denfert-Rochereau, 75014 Paris, France 6 Aix-Marseille Université, CNRS, Laboratoire d’Astrophysique de Marseille UMR 7326, 13388 Marseille Cedex 13, France 7 European Southern Observatory (ESO), 19001 Casilla, Santiago, Chile 8 Observatoire de Haute-Provence, CNRS/OAMP, 04870 Saint-Michel-l’Observatoire, France 9 Institut d’Astrophysique de Paris, UMR 7095 CNRS, Université Pierre & Marie Curie, 98bis boulevard Arago, 75014 Paris, France 10 SUPA, School of Physics and Astronomy, University of St. Andrews, St. Andrews, KY16 9SS, UK 11 European Space Agency (ESA), Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA Received 24 February 2016 / Accepted 10 May 2016 ABSTRACT Context. -