I am proud of this essay primarily because the words flowed from the heart. That is a big deal to me since I do not consider myself a great writer, and because I do not practice writing as much as I want to I often have a blank screen for the first 30 minutes when writing essays. The flow takes time to begin. I am also proud of this essay because I was blessed with the opportunity to actually do exactly the things I promised to do. (As all applicants know, the NSF wants you to predict certain things about your future but will not hold you to such promises if you are award the fellowship.) For example, I was a tutor for the Banneker Institute classes throughout the entire summer right before I started graduate classes.
I can provide a lot of tips as to why specifically this was a winning essay but I won't go into such extensive detail on this post. However, I will say that this essay intertwines nicely with my NSF research proposal and that is part of the reason why I won. So read that as well (in the next post).
My blog uses simple terms to discuss complex topics in astrophysics research. The purpose of this blog is to teach the intimate details that usually get overlooked when people describe the job of an astronomer. These details include an astronomer’s knowledge of mathematics and writing code. In my blog (http://bi-mwilson.blogspot.com), I demonstrate how my many Python scripts fit models to astrophysical data. I even allow my readers to run my code for themselves! I also give a simple explanation of the statistics employed by my code. As my blog shows, I have fun explaining the variety of statistical methods that astronomers can use in their research. This blog is currently my primary way of increasing scientific literacy across the globe.
My website gives the world a chance to learn about the research projects I have worked on in the past. My website (http://mwilson1.github.io) shows that one of these projects is my search for stars that have magnetic activity cycles in their coronae. When I was an NSF REU intern at the CfA during the summer after my sophomore year, I used X-ray data gathered by the Chandra and XMM-Newton Observatories to examine flux variation over a period of ~11 years among the 10 brightest stars within the Chandra Deep Field South. To study these stars, I learned Python and wrote scripts that performed a variety of tasks, including fit satisfactory models to the stellar spectra, calculate the flux of the star for each epoch of observations, and produce pretty light curves. It was a challenging but rewarding experience to write all of the scripts from scratch. Furthermore, I wrote a 16-page document reporting the background information, methodologies and results of my research. I also presented this research as a poster talk at the winter AAS conference in 2015. Near the end of that summer, the uncertainties in my light curves suggested that I did not have enough data—i.e. X-ray photons—to conclude whether or not I found the 5th star in our Universe that has a confirmed X-ray coronal cycle, but we did conclude that none of my stars exhibited flux variability about a factor of 10 like the Sun does over ~11 years. Fortunately, my advisors and I will have plenty of Chandra data in 2016 to further analyze the same stars. I am eager to see them again at the upcoming AAS conference in January of 2016 when I utilize my skills in elocution to present another engaging poster talk.
Elocution is too powerful of an art form to neglect when seeking to capture the attention and support of a large body of people. I first discerned the power of public speaking during my candidacy campaign and office of Student Government President at my high school. I later found that this skill transitions nicely to my astronomy research. I have given talks to scientists at Chicago’s Adler Planetarium, my university—Embry-Riddle Aeronautical University (ERAU)—, the CfA, the FIU McNair Research Conference and the AAS Meeting. Throughout my experiences at conferences and colloquia, I have discerned that most scientists need to take the art of public speaking more seriously. Seeing, in person, a younger audience’s dissatisfaction and disdain for science after listening to someone deliver a dry and excessively complex scientific presentation is the primary reason for why I am consistently earnest when I prepare a talk or give a speech. This reason is also why I enjoy the frequent practice of describing my research to friends and colleagues. Such practice allows me to go to the Adler Planetarium whenever I am on winter or summer break from college and, with simplicity, teach youth about astronomy and inspire their growing imaginations. Fortunately, this GRFP Fellowship’s annual stipend will help with my costs of travel as I journey back and forth between Cambridge and Chicago every summer and winter as I currently do between Daytona Beach and Chicago. Furthermore, with the additional time I will have to focus on increasing diversity in the astronomy community—as opposed to working more as a teaching fellow to cover tuition—I will be a graduate student mentor for future Banneker Institute (BI) undergraduates at the CfA.
My activism will be focused on supporting the BI and mentoring its interns. This institute seeks to increase the participation of minority groups and awareness of social justice issues in the astronomy community. Interns will benefit from my breadth of research experiences that have given me the skills to see a variety of perspectives when approaching research questions and issues. During my second year at ERAU, I used MATLAB and IDL to analyze Doppler shifts in the spectra of the Moon’s diffuse sodium and potassium atmosphere. The velocity of these atoms insinuated the mechanisms (such as meteoric impact ablation) that may be the primary cause for why atoms—even from the lunar regolith—reach speeds sufficient for escaping the lunar atmosphere. During my third year, I studied terrestrial, high-altitude Hydrogen-Alpha emission in order to ameliorate the MSIS-90 model that is used for specifying geocoronal atomic hydrogen column densities. The summer after my third year, I used Python to analyze data and produce light curves of defocused bright stars—as described near the end of my research proposal. My background with lunar, terrestrial, stellar and exoplanet research will help interns see various techniques astronomers can use to approach different problems. I will also expose the interns to the work I do at the Adler Planetarium, with hopes that the impact I have made at the planetarium will inspire the BI interns to participate in public outreach as well. This is important because as more minority students project their excellence and teach their science to the public, the social constructs that have, for so long, discouraged minorities from pursuing careers in STEM fields will be mitigated.
Throughout my research career, I have found that my activism couples well with my elocution. During my first research project, I tutored 5th grade students, who were predominantly African-American, at an elementary school in Daytona Beach. The 5th grade teacher frequently asked me to give the class an update on my research and show them how cool it was that organizations provided funding for me to travel across the US to give talks or observe on a telescope. At ERAU, I am the student mentor for two freshmen and one sophomore. Two of my mentees are women of color. However, even if I had mentees that did not belong to an underrepresented group, I have found that merely discussing my research or giving a talk causes people to ponder the notion that people of a race or ethnicity unlike their own can be just as intelligent and beneficial to society as they are. With this NSF Fellowship, I can reinforce this truth. Moreover, with the support of this fellowship and my friends at ERAU, the BI, the CfA and the Adler Planetarium, my current efforts towards increasing scientific literacy, diversity in STEM fields and awareness of social justice issues will receive a great reinforcement that I will then use to inspire my mentees and young science enthusiasts around the world.