Laura Newburgh headshot.

Laura Newburgh

she/her/hers
Associate Professor of Physics
Physics

Biographical Sketch: 

Laura Newburgh is an Assistant Professor of Physics at Yale University. She received her Ph.D. in physics from Columbia University on her work building, characterizing, deploying, and analyzing data on the polarized CMB experiment QUIET. She worked on low-temperature detector characterization, integration, and deployment for polarized CMB experiment ACTPol as a postdoc at Princeton University, and began working on novel methods of calibration for the 21cm experiment CHIME as a postdoctoral fellow at the University of Toronto. Her work spans hardware, software, and analysis for CMB and 21cm cosmology through her current projects CHIME, HIRAX, Simons Observatory, and CMB-S4.

Research:

Laura Newburgh studies the past 13 billion years of cosmic history through measurements of the Cosmic Microwave Background (CMB) and 21 cm hydrogen emission from faraway galaxies. Her work involves designing, building, and using instruments that go on radio telescopes around the world. The data from these instruments enable her to probe the nature of dark energy, dark matter, neutrinos, and cosmic inflation.

Education: 

Ph.D., Columbia University, 2010

Honors & Awards: 

Newburgh received a National Science Foundation (NSF) CAREER award in 2018. With CHIME collaborators, she shared both the 2022 Berkeley Prize for breakthroughs in understanding Fast Radio Bursts (FRBs) and the 2024 Buchalter Cosmology Prize for measuring the clustering of hydrogen gas over a large region of the observable Universe. 

Selected Publications: 

  • CHIME/FRB Collaboration, A Second Source of Repeating Fast Radio Bursts, Nature, Volume 566, Issue 7743
  • CHIME/FRB Collaboration, First Detection of Fast Radio Bursts between 400 and 800 MHz by CHIME/FRB, Astronomer’s Telegram #11901
  • Louis et al, The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters, ArXiv
  • Newburgh et al, HIRAX: A Probe of Dark Energy and Radio Transients, Proc. SPIE, ArXiv
  • Berger et al, Holographic Beam Mapping of the CHIME Pathfinder Array, Proc. SPIE , ArXiv
  • Newburgh et al, Calibrating CHIME, A New Radio Interferometer to Probe Dark Energy, Proc. SPIE, 2014, ArXiv

Contact Info

laura.newburgh@yale.edu

+1 (203) 432-9168

WL 210

Research Website

Research Areas: Astrophysics & Cosmology

Research Type: Experimentalist

Experiments

CV

Experiments

CHIME

Newburgh

Science goal: Measure the expansion history of the Universe and discover insights about dark energy. 

WL involvement: The Newburgh group uses a technique called holography to map the beam shape of CHIME to be able to identify and remove emission from unintended sources.

CHIME radio telescopes.

CMB-S4

Newburgh

Science Goal: Make measurements of the Cosmic Microwave Background with an order of magnitude greater than any current experiment.

WL Involvement: Newburgh leads the data acquisition and control group, mainly building software to control and acquire data from the telescopes.

CMB-S4 telescope.

HIRAX

Newburgh

Science goal: Study high-redshift large-scale structure for a constraint on dark energy and transient science to understand the nature of Fast Radio Bursts (FRBs).

WL involvement: The Newburgh group is leading the development of techniques, hardware, and analysis to measure and map the HIRAX beam shape with a quadcopter drone.

HIRAX Telescope

Simons Observatory

Newburgh

Science goal: Probe the Cosmic Microwave Background to learn more about the beginning of the Universe. 

WL involvement: The Newburgh group is part of the team commissioning SO. Newburgh leads the data acquisition and control group, mainly building software to control and acquire data.

Simons Observatory telescope.

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