June 2020 Education, Professional Experience and Honors
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![Arxiv:2006.14546V1 [Astro-Ph.EP] 25 Jun 2020](https://docslib.b-cdn.net/cover/4588/arxiv-2006-14546v1-astro-ph-ep-25-jun-2020-134588.webp)
Arxiv:2006.14546V1 [Astro-Ph.EP] 25 Jun 2020
Draft version June 26, 2020 Typeset using LATEX twocolumn style in AASTeX62 TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host Shubham Kanodia,1, 2 Caleb I. Canas~ ,1, 2, 3 Gudmundur Stefansson,4, 5 Joe P. Ninan,1, 2 Leslie Hebb,6 Andrea S.J. Lin,1, 2 Helen Baran,1, 2 Marissa Maney,1, 2 Ryan C. Terrien,7 Suvrath Mahadevan,1, 2 William D. Cochran,8, 9 Michael Endl,8, 9 Jiayin Dong,1, 2 Chad F. Bender,10 Scott A. Diddams,11, 12 Eric B. Ford,1, 2, 13 Connor Fredrick,11, 12 Samuel Halverson,14 Fred Hearty,1, 2 Andrew J. Metcalf,15, 16, 17 Andrew Monson,1, 2 Lawrence W. Ramsey,1, 2 Paul Robertson,18 Arpita Roy,19, 20 Christian Schwab,21 and Jason T. Wright1, 2 1Department of Astronomy & Astrophysics, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA, 16802, USA 2Center for Exoplanets and Habitable Worlds, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA, 16802, USA 3NASA Earth and Space Science Fellow 4Henry Norris Russell Fellow 5Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Princeton, NJ 08540, USA 6Department of Physics, Hobart and William Smith Colleges, 300 Pulteney Street, Geneva, NY, 14456, USA 7Department of Physics and Astronomy, Carleton College, One North College Street, Northfield, MN 55057, USA 8McDonald Observatory and Department of Astronomy, The University of Texas at Austin 9Center for Planetary Systems Habitability, The University of Texas at Austin 10Steward Observatory, The University of Arizona, 933 N. -
First Results from Planet Hunters: Exploring the Inventory of Short Period Planets from Kepler
EPSC Abstracts Vol. 6, EPSC-DPS2011-1226, 2011 EPSC-DPS Joint Meeting 2011 c Author(s) 2011 First Results from Planet Hunters: Exploring the Inventory of Short Period Planets from Kepler C. J. Lintott (1,2), M. E. Schwamb(3,4), D. A. Fischer(5), M. J. Giguere(5), S. Lynn(1), J. M. Brewer(5), K. Schawinski(3,4), R. J. Simpson(1), A. Smith(1), J. Spronck(5) (1) Department of Physics, University of Oxford, (2) Adler Planetarium, Chicago, (3) Department of Physics, Yale University, (4) Yale Center for Astronomy and Astrophysics, Yale University, (5) Department of Astronomy, Yale Abstract suited to picking out outliers and can find most transits that cannot be detected in periodograms and We present the first results and planet candidates identify transit signals that may be missed by the from Planet Hunters, part of the Zooniverse sophisticated TPS. It is unrealistic to expect a single collection of citizen science projects. [3,4]. Planet individual or a small group of experts to review the Hunters enlists more than 40,000 members of the entire Kepler dataset, but with over 40,000 volunteers general public to visually identify transits in the examining the light curves on the Planet Hunters publicly released Kepler data via the World Wide interface, we have the ability to visually inspect the Web in order to provide a completely independent entire public dataset for signatures of exoplanet assessment of planet frequencies derived from the transits. Kepler light curves. We examine the abundance of large planets (> 2 earth radii) on short period (< 15 2. -
Refereed Publications That Name
59 Refereed Publications Since 2011 with Named Co-Authors who are NASA Citizen Scientists Compiled by Marc Kuchner February 2021 Authors in bold are citizen scientists. Aurorasaurus Semeter, J., Hunnekuhl, M., MacDonald, E., Hirsch, M., Zeller, N., Chernenkoff, A., & Wang, J. (2020). The mysterious green streaks below STEVE. AGU Advances, 1, e2020AV000183. https://doi.org/10.1029/2020AV000183 Hunnekuhl, M., & MacDonald, E. (2020). Early ground‐based work by auroral pioneer Carl Størmer on the high‐altitude detached subauroral arcs now known as “STEVE”. Space Weather, 18, e2019SW002384. https://doi.org/10.1029/2019SW002384 S. B. Mende. B. J. Harding, & C. Turner. “Subauroral Green STEVE Arcs: Evidence for Low- Energy Excitation” Geophysical Research Letters, Volume 46, Issue 24, Pages 14256-14262 (2019) http://doi.org/10.1029/2019GL086145 S. B. Mende. & C. Turner. “Color Ratios of Subauroral (STEVE) Arcs” Journal of Geophysical Research (Space Physics),Volume 124, Issue 7, Pages 5945-5955 (2019) http://doi.org/10.1029/2019JA026851 Y. Nishimura, Y., B, Gallardo-Lacourt, B., Y, Zou, E. Mishin, D.J. Knudsen, E. F. Donovan, V. Angelopoulos, R. Raybell, “Magnetospheric Signatures of STEVE: Implications for the Magnetospheric Energy Source and Interhemispheric Conjugacy” Geophysical Research Letters, Volume 46, Issue 11, Pages 5637-5644 (2019) Elizabeth A. MacDonald, Eric Donovan, Yukitoshi Nishimura, Nathan A. Case, D. Megan Gillies, Bea Gallardo-Lacourt, William E. Archer, Emma L. Spanswick, Notanee Bourassa, Martin Connors, Matthew Heavner, Brian Jackel, Burcu Kosar, David J. Knudsen, Chris Ratzlaff and Ian Schofield, “New science in plain sight: Citizen scientists lead to the discovery of optical structure in the upper atmosphere” Science Advances, vol. -
Planet Hunters, Zooniverse Evaluation Report
Planet Hunters | Evaluation Report 2019 Planet Hunters, Zooniverse Evaluation report Authored by Dr Annaleise Depper Evaluation Officer, Public Engagement with Research Research Services, University of Oxford 1 Planet Hunters | Evaluation Report 2019 Contents 1. Key findings and highlights ..................................................................................... 3 2. Introduction ............................................................................................................ 4 3. Evaluating Planet Hunters ....................................................................................... 5 4. Exploring impacts and outcomes on citizen scientists ............................................. 6 4.1 Increased knowledge and understanding of Astronomy ..................................................................... 7 4.2 An enjoyable and interesting experience ......................................................................................... 12 4.3 Raised aspirations and interests in Astronomy ................................................................................ 13 4.4 Feeling of pride and satisfaction in helping the scientific community ............................................... 17 4.5 Benefits to individual wellbeing ...................................................................................................... 19 5. Learning from the evaluation ................................................................................ 20 5.1 Motivations for taking part in Planet Hunters -
Planet Hunters. VI: an Independent Characterization of KOI-351 and Several Long Period Planet Candidates from the Kepler Archival Data
Accepted to AJ Planet Hunters VI: An Independent Characterization of KOI-351 and Several Long Period Planet Candidates from the Kepler Archival Data1 Joseph R. Schmitt2, Ji Wang2, Debra A. Fischer2, Kian J. Jek7, John C. Moriarty2, Tabetha S. Boyajian2, Megan E. Schwamb3, Chris Lintott4;5, Stuart Lynn5, Arfon M. Smith5, Michael Parrish5, Kevin Schawinski6, Robert Simpson4, Daryll LaCourse7, Mark R. Omohundro7, Troy Winarski7, Samuel Jon Goodman7, Tony Jebson7, Hans Martin Schwengeler7, David A. Paterson7, Johann Sejpka7, Ivan Terentev7, Tom Jacobs7, Nawar Alsaadi7, Robert C. Bailey7, Tony Ginman7, Pete Granado7, Kristoffer Vonstad Guttormsen7, Franco Mallia7, Alfred L. Papillon7, Franco Rossi7, and Miguel Socolovsky7 [email protected] ABSTRACT We report the discovery of 14 new transiting planet candidates in the Kepler field from the Planet Hunters citizen science program. None of these candidates overlapped with Kepler Objects of Interest (KOIs) at the time of submission. We report the discovery of one more addition to the six planet candidate system around KOI-351, making it the only seven planet candidate system from Kepler. Additionally, KOI-351 bears some resemblance to our own solar system, with the inner five planets ranging from Earth to mini-Neptune radii and the outer planets being gas giants; however, this system is very compact, with all seven planet candidates orbiting . 1 AU from their host star. A Hill stability test and an orbital integration of the system shows that the system is stable. Furthermore, we significantly add to the population of long period 1This publication has been made possible through the work of more than 280,000 volunteers in the Planet Hunters project, whose contributions are individually acknowledged at http://www.planethunters.org/authors. -
Optical and Near-Infrared Observations of SN 2011Dh-The First 100 Days
Astronomy & Astrophysics manuscript no. sn2011dh-astro-ph-v2 c ESO 2018 November 4, 2018 Optical and near-infrared observations of SN 2011dh - The first 100 days. M. Ergon1, J. Sollerman1, M. Fraser2, A. Pastorello3, S. Taubenberger4, N. Elias-Rosa5, M. Bersten6, A. Jerkstrand2, S. Benetti3, M.T. Botticella7, C. Fransson1, A. Harutyunyan8, R. Kotak2, S. Smartt2, S. Valenti3, F. Bufano9; 10, E. Cappellaro3, M. Fiaschi3, A. Howell11, E. Kankare12, L. Magill2; 13, S. Mattila12, J. Maund2, R. Naves14, P. Ochner3, J. Ruiz15, K. Smith2, L. Tomasella3, and M. Turatto3 1 The Oskar Klein Centre, Department of Astronomy, AlbaNova, Stockholm University, 106 91 Stockholm, Sweden 2 Astrophysics Research Center, School of Mathematics and Physics, Queens University Belfast, Belfast, BT7 1NN, UK 3 INAF, Osservatorio Astronomico di Padova, vicolo dell’Osservatorio n. 5, 35122 Padua, Italy 4 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany 5 Institut de Ciències de l’Espai (IEEC-CSIC), Facultat de Ciències, Campus UAB, E-08193 Bellaterra, Spain. 6 Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan 7 INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello, 16 80131 Napoli, Italy 8 Fundación Galileo Galilei-INAF, Telescopio Nazionale Galileo, Rambla José Ana Fernández Pérez 7, 38712 Breña Baja, TF - Spain 9 INAF, Osservatorio Astrofisico di Catania, Via Santa Sofia, I-95123, Catania, Italy 10 Departamento de Ciencias Fisicas, Universidad Andres Bello, Av. Republica 252, Santiago, Chile 11 Las Cumbres Observatory Global Telescope Network, 6740 Cortona Dr., Suite 102, Goleta, CA 93117 12 Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland 13 Isaac Newton Group, Apartado 321, E-38700 Santa Cruz de La Palma, Spain 14 Observatorio Montcabrer, C Jaume Balmes 24, Cabrils, Spain 15 Observatorio de Cántabria, Ctra. -
Kavli IPMU Annual 2014 Report
ANNUAL REPORT 2014 REPORT ANNUAL April 2014–March 2015 2014–March April Kavli IPMU Kavli Kavli IPMU Annual Report 2014 April 2014–March 2015 CONTENTS FOREWORD 2 1 INTRODUCTION 4 2 NEWS&EVENTS 8 3 ORGANIZATION 10 4 STAFF 14 5 RESEARCHHIGHLIGHTS 20 5.1 Unbiased Bases and Critical Points of a Potential ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙20 5.2 Secondary Polytopes and the Algebra of the Infrared ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙21 5.3 Moduli of Bridgeland Semistable Objects on 3- Folds and Donaldson- Thomas Invariants ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙22 5.4 Leptogenesis Via Axion Oscillations after Inflation ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙23 5.5 Searching for Matter/Antimatter Asymmetry with T2K Experiment ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ 24 5.6 Development of the Belle II Silicon Vertex Detector ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙26 5.7 Search for Physics beyond Standard Model with KamLAND-Zen ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙28 5.8 Chemical Abundance Patterns of the Most Iron-Poor Stars as Probes of the First Stars in the Universe ∙ ∙ ∙ 29 5.9 Measuring Gravitational lensing Using CMB B-mode Polarization by POLARBEAR ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ 30 5.10 The First Galaxy Maps from the SDSS-IV MaNGA Survey ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙ ∙32 5.11 Detection of the Possible Companion Star of Supernova 2011dh ∙ ∙ ∙ ∙ ∙ ∙ -
January 2019, the Role of Citizen Scientists in New Discoveries
Astrobiology News January 2019: The Role of Citizen Scientists in New Discoveries Zooniverse is the world’s largest and most popular platform for online citizen science.1 Last month, I mentioned the launch of Planet Hunters TESS; this month, I want to tell you about two exciting new discoveries by citizen scientists participating in Exoplanet Explorers, which uses data from the Kepler Observatory’s Second Mission.2 Both discoveries are described extensively in Zooniverse blogs posted on January 7th.3 Exoplanet K2-288b orbits in the habitable zone of the smaller of two low- mass red dwarf stars that form a binary system. Its size places it in a rare category of planets being dubbed “sub-Neptunes” – worlds thought to lie in a transition region between potentially habitable “super-Earths” and worlds more like the gas giants in our Solar System. K2-138g, just a bit smaller than Neptune, is the 6th planet discovered in the K2-138 system, which harbors a somewhat more massive “orange dwarf” star. The K2- 138 system shares some similarities with the TRAPPIST-1 system, which you can read more about in the Astrobiology News posts from March and May 2017.4 What makes the K2-138 and TRAPPIST-1 systems similar is that the planets all orbit close to their stars, with very short periods. Five of the 6 planets in K2-138, and all 7 planets in the TRAPPIST-1 system, form a so- called resonant chain, where the planet orbits are related by the ratios of small integers. The orbiting bodies in such systems exert periodic gravitational influence on each other. -
![Arxiv:2009.08338V2 [Astro-Ph.EP] 30 Nov 2020 Loses It Over Time](https://docslib.b-cdn.net/cover/5197/arxiv-2009-08338v2-astro-ph-ep-30-nov-2020-loses-it-over-time-525197.webp)
Arxiv:2009.08338V2 [Astro-Ph.EP] 30 Nov 2020 Loses It Over Time
Astronomy & Astrophysics manuscript no. main ©ESO 2020 December 1, 2020 A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776? R. Luque1;2, L. M. Serrano3, K. Molaverdikhani4;5, M. C. Nixon6, J. H. Livingston7, E. W. Guenther8, E. Pallé1;2, N. Madhusudhan6, G. Nowak1;2, J. Korth9, W. D. Cochran10, T. Hirano11, P. Chaturvedi8, E. Goffo3, S. Albrecht12, O. Barragán13, C Briceño14, J. Cabrera15, D. Charbonneau16, R. Cloutier16, K. A. Collins16, K. I. Collins17, K. D. Colón18, I. J. M. Crossfield19, Sz. Csizmadia15, F. Dai20, H. J. Deeg1;2, M. Esposito8, M. Fridlund21;22, D. Gandolfi3, I. Georgieva22, A. Glidden23;24, R. F. Goeke23, S. Grziwa9, A. P. Hatzes8, C. E. Henze25, S. B. Howell25, J. Irwin16, J. M. Jenkins25, E. L. N. Jensen26, P. Kábath27, R. C. Kidwell Jr.28, J. F. Kielkopf29, E. Knudstrup12, K. W. F. Lam30, D. W. Latham16, J. J. Lissauer25, A. W. Mann31, E. C. Matthews24, I. Mireles24, N. Narita32;33;34;1, M. Paegert16, C. M. Persson22, S. Redfield35, G. R. Ricker24, F. Rodler36, J. E. Schlieder18, N. J. Scott25, S. Seager24;23;37, J. Šubjak27, T. G. Tan38, E. B. Ting25, R. Vanderspek24, V. Van Eylen39, J. N. Winn40, and C. Ziegler41 (Affiliations can be found after the references) Received 17.09.2020 / Accepted 30.11.2020 ABSTRACT We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8:5 mag,M = 0:54±0:03 M ) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). -
Exploring Exoplanet Populations with NASA's Kepler Mission
SPECIAL FEATURE: PERSPECTIVE PERSPECTIVE SPECIAL FEATURE: Exploring exoplanet populations with NASA’s Kepler Mission Natalie M. Batalha1 National Aeronautics and Space Administration Ames Research Center, Moffett Field, 94035 CA Edited by Adam S. Burrows, Princeton University, Princeton, NJ, and accepted by the Editorial Board June 3, 2014 (received for review January 15, 2014) The Kepler Mission is exploring the diversity of planets and planetary systems. Its legacy will be a catalog of discoveries sufficient for computing planet occurrence rates as a function of size, orbital period, star type, and insolation flux.The mission has made significant progress toward achieving that goal. Over 3,500 transiting exoplanets have been identified from the analysis of the first 3 y of data, 100 planets of which are in the habitable zone. The catalog has a high reliability rate (85–90% averaged over the period/radius plane), which is improving as follow-up observations continue. Dynamical (e.g., velocimetry and transit timing) and statistical methods have confirmed and characterized hundreds of planets over a large range of sizes and compositions for both single- and multiple-star systems. Population studies suggest that planets abound in our galaxy and that small planets are particularly frequent. Here, I report on the progress Kepler has made measuring the prevalence of exoplanets orbiting within one astronomical unit of their host stars in support of the National Aeronautics and Space Admin- istration’s long-term goal of finding habitable environments beyond the solar system. planet detection | transit photometry Searching for evidence of life beyond Earth is the Sun would produce an 84-ppm signal Translating Kepler’s discovery catalog into one of the primary goals of science agencies lasting ∼13 h. -
Výroční Zpráva České Astronomické Společnosti 2011
Výroční zpráva České astronomické společnosti 2011 stručná charakteristika V České astronomické společnosti v roce 2011 pracovalo 8 místních poboček (Praha, Západočeská, Východočeská, Jihočeská, Astronomická společnost Most se statutem pobočky, Třebíč, Valašská astronomická společnost se statutem pobočky a Klub astronomů Liberecka), 9 odborných sekcí (Sekce proměnných hvězd a exoplanet, Zákrytová a astrometrická sekce, Sluneční, Přístrojová a optická sekce, Historická, Astronautická, Kosmologická, Sekce pro mládež a Společnost pro meziplanetární hmotu se statutem sekce), dále Odborná skupina pro temné nebe a Terminologická komise. ČAS měla v závěru roku přes 500 individuálních členů a 22 kolektivních členů (o 2 více než v minulém roce), z nichž nejvýznamnější je Astronomický ústav AV ČR. Společnost vydává věstník Kosmické rozhledy, distribuuje členům navíc popularizační časopis Astropis, provozuje informační a popularizační web www.astro.cz pro nejširší veřejnost a vydává prostřednictvím Odboru mediální komunikace AV ČR tisková prohlášení a zprávy z oblasti astronomie a kosmonautiky. Mezi významné činnosti v roce 2011 patřila odborná činnost sekcí, popularizace astronomie, vyhledávání a podpora mladých talentů v podobě Astronomické olympiády, udělení tří cen, ochrana před světelným znečištěním, role národního koordinátora astronomického programu Evropské noci vědců v ČR a provozování Keplerova muzea v Praze. 1 Výroční zpráva České astronomické společnosti za rok 2011 podrobná O společnosti Česká astronomická společnost je dobrovolné sdružení odborných a vědeckých pracovníků v astronomii, amatérských astronomů a zájemců o astronomii z řad veřejnosti. ČAS dbá o rozvoj astronomie v českých zemích a vytváří pojítko mezi profesionálními a amatérskými astronomy. ČAS je sdružena v Radě vědeckých společností a je kolektivním členem Evropské astronomické společnosti. Volené orgány ČAS pracovaly v roce 2011 v tomto složení Výkonný výbor Předseda Ing. -
Benjamin V. Rackham
Benjamin V. Rackham 51 Pegasi b Postdoctoral Fellow Massachusetts Institute of Technology 77 Massachusetts Ave, 54-1726 • Cambridge, MA 02139 [email protected] • +1 (617) 258-6910 • http://rackham.space EDUCATION 2012—2018 University of Arizona, Tucson, AZ Ph.D. in Astronomy & Astrophysics Astrobiology Minor Magna Cum Laude Advisor: Dr. Dániel Apai 2005—2009 Westminster College, Salt Lake City, UT B.S. in Neuroscience, Honors Degree Social Science Minor Magna Cum Laude EMPLOYMENT 2019—present 51 Pegasi b Fellow, Massachusetts Institute of Technology, Cambridge, MA 2018—2019 Postdoctoral Research Associate, University of Arizona, Tucson, AZ 2017—2018 Graduate Research Assistant, University of Arizona, Tucson, AZ 2014—2017 NSF Graduate Research Fellow, University of Arizona, Tucson, AZ 2014—2014 Graduate Teaching Assistant, University of Arizona, Tucson, AZ 2012—2013 Graduate Research Assistant, University of Arizona, Tucson, AZ 2010—2012 Biological Technician, WestLand Resources, Inc., Tucson, AZ 2009—2010 Wildlife Technician, Utah Division of Wildlife Resources, Salt Lake City, UT HONORS AND AWARDS 2019 51 Pegasi b Fellowship in Planetary Astronomy, Heising-Simons Foundation (Three-year, $375,000 grant) 2019 CSH Fellowship (declined), Center for Space and Habitability, University of Bern 2014 Graduate Research Fellowship, National Science Foundation (Three-year, $138,000 grant) 2009 Trustees’ Character Award, Westminster College Board of Trustees (One of only three student awards given at graduation) 2008 Dr. Barry Quinn and Dr. Bob Warnock Endowed Science Scholarship, Westminster College 2007 Barnett Honors Scholarship, Westminster College Benjamin V. Rackham, CV 1 REFEREED PUBLICATIONS 15 total (284 citations) | 3 first-author (136 citations) | ADS: https://goo.gl/T1Dzwf First-author publications: 1.