Andrew McCann


to Andrew McCann's personal website

I am a physicist working in the domain of experimental high-energy astrophysics and gamma-ray instrumentation. I received a PhD in physics from McGill University in 2011. From 2011 to 2014 I was a Kavli postdoctoral fellow at the Kavli Institute of Cosmological Physics at the University of Chicago and a post-doctoral fellow at the McGill Space Institute in 2015 and 2016. I am currently a Research Associate at the Canadian Hazard Information Service of Natural Resources Canada where I research terrestrial gamma-ray detectors for safety and security applications. I live in Ottawa, Ontario, Canada.

Contact me

Contact me through my contact page or vist my CV page.

Latest news from VERITAS

Check out the latest news from the VERITAS project here.

Read a recent article.

Read my recent article on the spectral shapes of gamma-ray pulsars here.

81st Aurthur H. Compton Lecture Series

Established in 1976 by The Enrico Fermi Institute at the University of Chicago, the bi-annual Compton Lecture are intended for the general public, members of the University community, and interested citizens of the Chicago area. Requiring no formal background in mathematics or science, each lecture series spans 8-10 weeks and is intended to share scientific research conducted at the University of Chicago with an general public audience.

I delivered the 81st Compton Lecture Series in the Spring of 2015. See the lecture material below.


by Dr. Andrew McCann

Neutron stars are born in the final moments of the supernova death of massive stars and, in keeping with their exotic origin, they exhibit unmatched extremes in a variety of ways. Not only are they the smallest stars we know of, neutron stars are the most dense solid objects in the known Universe. Their surface gravity is 100 billion times that of the Earth and their magnetic fields strengths, which can reach a quadrillion Gauss, are the strongest known to exist. Neutron stars are born rotating rapidly and their emission, like the beam from a lighthouse, is observed as a highly stable and regular periodic pulsation - hence the name 'pulsating star' or 'pulsar'. Although pulsars were discovered over 40 years ago and the number of known pulsars exceeds 2400, the physical processes which power the vast array of unique and often bizarre phenomena observed from pulsars are poorly understood. Explaining the observed behavior of neutron stars has become one of the most challenging puzzles in high-energy astrophysics. Despite the longstanding mystery of their emission, the steady and predictable pulsations from pulsars make them remarkably powerful astrophysical tools. This duality has put pulsars at the centre of some of the most compelling astrophysical research of the last few decades. Each week we will explore different aspects of this duality, by reviewing pulsar phenomena in different wave bands (radio, optical, x-ray, gamma-ray) and by discussing the role of pulsars in tests of Einstein's theory of relativity and in the search for gravitational waves.

04/04/2015 - Setting the Stage
04/11/2015 - From death comes new Life
04/18/2015 - How the lighthouse shines
04/25/2015 - Pulsars meet Einstein
05/02/2015 - Weirdos I (Magnetism and Magnetars)
05/09/2015 - Weirdos II (Nulling, Giant pulses, RRATs and more)
05/16/2015 - The gamma-ray pulsar revolution
05/30/2015 - Building a Gravitational Wave Observatory from Pulsars
06/06/2015 - Hunting for gravitational waves with LIGO (by Dr. Ben Farr)