I began working in cosmic microwave background (CMB) cosmology in Nils Halverson’s lab as an undergraduate at the University of Colorado. I had previously worked on solar satellite telemetry code at the Laboratory for Atmospheric and Space Physics, but I was drawn to the big questions that cosmology posed: What is the universe composed of? Where did we come from? What will happen to the universe in the future? What can we learn about the physics of our universe from the CMB? In the two and a half years that I worked for Nils, I developed hardware and analysis code for detector testing and characterization. The two and a half years I worked there only made me more curious and passionate about the subject. I owe a lot to everyone who worked in the lab at that time because they were all really amazing mentors.
I decided to continue research in the CMB at Princeton University, where I worked on several experiments through my NASA Space Technology Research Fellowship, including the Atacama B-mode Search (ABS), ACTPol, and Advanced ACTPol (AdvACT). ABS deployed just as I was beginning my degree, so I spent a lot of time in Chile operating and characterizing the telescope and detectors. ABS was really exciting because it was a pathfinder experiment testing out novel instrumental technologies, which also left room to develop new analysis and characterization techniques. Princeton is the heart of the array assembly and integration for ACTPol and AdvACT. While it wasn’t my primary focus, I helped with array assembly when it was crunch time. I continued to be interested in novel technologies and designed new feedhorns (which couple light onto our detectors) for AdvACT.
I earned my Ph.D. in 2016, and I am currently a postdoctoral fellow at the University of Michigan. I’ve continued my work on AdvACT by designing the feedhorns and detectors for the low-frequency (27/39 GHz) array, and I am also a member of TolTEC, a high-resolution microwave camera for the Large Millimeter Telescope (LMT) in Mexico. I’m interested in combining these data sets with optical data sets to better understand galaxy clusters, which are the largest gravitationally bound objects in the universe and could thus help us better understand dark energy and dark matter. As a member of SO, I am active in the detector group and a leader of the calibration, sensitivity, and systematics (CSS) group. The CSS group is responsible for determining the sensitivity and systematics of various telescope configurations to aid in instrument selection and scientific forecasts, making a plan for characterizing and calibrating the telescope to minimize systematics, and acting as the main interface between the science and design groups.
Equality in STEM fields is one of my core principles. As a graduate student, I was the leader of the graduate women in physics group, where I became very active in working toward equal access and opportunity for all in physics through mentorship, providing career development resources, and improving the climate in STEM fields. It is this experience and passion that have driven me to develop a mentorship program for SO with the mentorship committee, which I also lead. The mentorship program is open to all in SO and will offer one-on-one mentoring between junior and senior members of SO. We’ll begin accepting applications in June around the SO meeting, so keep your eyes peeled! Outside of work, I like to keep busy with lots of hobbies, including baking, cooking, gardening, and photography. Many people in our lab like cooking and/or baking, so there’s always something to eat whether it be caramel, croissants, or smoked pulled pork!
I first started working on cosmic microwave background measurements as a graduate student at UC San Diego. As an undergraduate, I had worked in several labs on various technical projects, and really enjoyed the day-to-day building, tinkering, and troubleshooting that comes with getting an experiment to work. I decided to join Professor Brian Keating’s experimental cosmology group building telescopes to measure the cosmic microwave background (CMB) because it shared much of the lab work I enjoyed, but also came with an appealing grand goal of measuring new properties of our universe. I helped commission our first telescope, POLARBEAR-1, and continued to help design and build the next series of telescopes as we expand and improve our experiment, adding two more telescopes as part of the Simons Array. When I first arrived in Chile, our site was just some shipping containers and a bare telescope structure. By the time I graduated, our site wasn’t much more than that, but we had completed our initial CMB observations and published exciting new results detecting the signal we had set out to measure, the B-mode gravitational lensing signal.
In 2015, I finished my Ph.D. at UC San Diego and moved to UC Berkeley to continue working on the POLARBEAR/Simons Array project. I received an NSF Astronomy and Astrophysics postdoctoral fellowship, which supports me to continue my research as well as expand my involvement in education and outreach. Through the Multiverse group at UC Berkeley’s Space Sciences Lab, I am leading an NSF-funded research experience for undergraduates (REU) program, aimed at first-generation college students and community college students. The program brings a group of students to the lab for the summer to complete a research project in support of one of the NASA missions or other projects at the lab. I get to teach the students important skills and tools for research they wouldn't have encountered in their classes, as well as follow each student’s project and learn about new topics myself.
For Simons Observatory, I have begun working on optimization: helping study how to build the best experiment we can, given our capabilities and budget. While my research background helps me to frame and understand the technical problems we are studying, the question of how to best spend our resources also interests me. As a student, as I became more involved in research and learned along the way about the sources of funding, I became more interested in science policy and how these funding decisions are made. Advancements in astronomy and particle physics can require large (and expensive!) collaborative hardware projects to progress the field. The community and funding agencies must coordinate not just at the largest scales for mega projects like James Webb Space Telescope, but with overall priorities. Writing papers describing the current state of our field and what we plan to do next is an important part of this process, and I really enjoy being a part of it.
Outside of lab, I enjoy spending as much time as I can in the mountains backpacking, hiking, and stargazing. As a graduate student, I volunteered for the local Mountain Rescue Association team. In addition to all the useful technical training I received, being part of such a large team, running like a well-oiled machine, was an amazing experience. I have always enjoyed leading backpacking trips with friends, but this took the organization and preparedness to a whole new level. You quickly learn that self-sufficiency isn’t enough to be prepared to accomplish difficult tasks, or to help others in need.
I also enjoy the traveling that do as part of my job and research. My favorite part is trying new foods, whether it’s new dishes at restaurants or exploring snacks at a local grocery store. I’ve probably eaten over a hundred kinds of chips in the past several years! Most recently, I had fried pasta chips from a 7-Eleven in Japan; they were delicious.
Many people ask me why I chose Cosmology over other “more concrete” fields, and my answer is always “wouldn’t you do something that keeps you awake at night (and lets you travel a lot)?!”. I have been working on the Cosmic Microwave Background since I was an undergraduate student in Rome (Italy), where I investigated different designs for future balloon-borne experiments aiming to detect the signature of the first instances of the universe (called Inflation). During my masters, I worked on two aspects of the proposed Large-Scale Polarization Explorer: optimizing the strategy for pointing our telescope and putting our raw data into maps of the sky (in this field we call this “map-making”). In 2012, I moved to the US and started my graduate studies at the University of Pittsburgh under the guidance of Prof. Arthur Kosowsky, with the desire of focusing on more theoretical aspects of cosmology. For a couple of years, I studied the statistics and anomalies of CMB photons that emanate from two points on the sky that are far apart (i.e. large angular scales). Following these studies, I got involved with the Atacama Cosmology Telescope collaboration and started working in three quite different areas ranging from analyzing the raw data to looking for cosmological signals (for the experts out there… map-making, time-domain analyses, as well as the detection of the kinetic Sunyaev-Zeldovich effect via pair-wise momentum). In September 2016, I became a postdoc at Princeton University, where I have the pleasure to keep analyzing the raw data coming from the ACTPol/AdvACT polarimeters, making high-quality CMB maps, and, more recently, looking at the gravitational-lensing effects of CMB photons coming from nearly the same point on the sky (i.e. small angular scales).
As a member of the SO collaboration, I am active in the time-domain working group. There is a lot that can be learnt from currently operating CMB experiments, and this group can offer insightful guidance towards realistic forecasting and an optimized telescope design.
Although my work keeps me awake at night, I do like to set the weekends away from my job. I am not much of a “nature” person; rather I enjoy the vibes of big, vivid, and active European and American cities –– Princeton is only one hour away from either Philadelphia or New York City! I like art, photography (although I am not great at producing breath-taking shots), and good food, especially if I make it. I used to practice a lot of classical and modern dance when I was young. Currently, I moved that need to jump up and down in the gym, just to make sure that “mens sana in corpore sano (healthy mind in a healthy body)”.