Quicklinks: JWST | NICER | STROBE-X | Stingray software

A 90-second overview of my research, submitted to a science communication competition with Skype A Scientist. I’m sorry, I spoke really quickly! Also, my office background has come together quite nicely since then.

As an astronomer, I’m fascinated by super-strong gravitational fields and the strange effects they have on matter. Black holes and neutron stars (together called ‘compact objects’ because scientists are clever) are host to extreme environments that cannot be re-created on Earth. In a binary orbit with a low-mass star like our Sun, a compact object will slowly drain the regular star of its matter over millions of years in a process called accretion. This accreted material forms an accretion disk around the compact object like a tutu on a ballerina. Some material from the accretion disk will accrete onto the compact object itself, but compact objects are messy eaters so there are winds blowing material off the disk and strong jets like firehoses of energetic particles that often shoot out from the north and south poles of the compact object. Accretion is a powerful process and accretion disks reach temperatures of about 20 million degrees Fahrenheit (100x hotter than the surface of the Sun), which produces bright heat-light in the form of X-rays. So, these systems are called X-ray binaries.

Listen to me talk about my research on the podcast Abstract: The Future of Science.
An artist’s impression of a stellar-mass black hole in orbit with a normal star companion, together called an X-ray binary. Credit: NASA/CXC/M. Weiss.

How do we know this?

There are two ways we can study emission from an accreting black hole or neutron star: spectra and timing. Spectral observations (the energy or color of the light) indicate what produced the light and therefore where the light is coming from. Timing observations (when the individual photons hit the detector) can tell us how the light is changing on very short (sub-second) timescales. By analyzing X-ray light from the innermost regions of X-ray binaries with spectral and timing observations, we can learn more about how matter behaves in the strong gravity of curved spacetime.

Me explaining my research on X-raying Black Holes in ~10 minutes as part of the No Time Like The Presentation competition with Skype A Scientist.

When I was a PhD student and postdoctoral fellow, I used data taken by telescopes. Since X-ray binaries are just a single point of light in the sky, I didn’t look at pretty pictures like those taken by Hubble or Chandra — instead, I did a lot of signal processing and data analysis of digital tables of X-ray photons. If you want to become an astronomer, computer programming, data analysis, and statistics skills will be very helpful.

Watch me explain my research accompanied by free-improvisational jazz music and video mixing.

Space telescopes

JWST: an infrared view of jets

Testing the mirror deployment in the clean room. Credit: NASA/STScI.

JWST is a joint NASAESACSA flagship space telescope for the highest quality infrared observations of the Universe. I’m a member of two teams that were selected to get data of bright-but-dead objects in our galaxy. We’ll use this to help improve the timing calibration of some of the scientific instruments, and to learn how the jets are launched out of the top and bottom of a stellar black hole. The principal investigator of both proposals is Prof. Poshak Gandhi at the University of Southampton, and the co-principal investigators for both are Dr. Aarran Shaw at the University of Nevada Reno and Prof. Tom Maccarone at Texas Tech University. Astronomy is a highly collaborative science, and working on a team with great people makes it lots of fun.

In November 2021 I organized and hosted a ‘JWST Day’ event at the Abrams Planetarium with Dr. Shannon Schmoll to celebrate the upcoming launch. We featured Michigan scientists using JWST for their science research, and had hands-on demonstrations of astronomy, physics, and space science.

NICER: X-rays on the Space Station

A picture of the International Space Station taken by a remote camera on a resupply mission,
with NICER indicated with an arrow. Credit: NASA.

My favorite telescope (and not coincidentally, the one I used the most in my research) is NICER, the Neutron Star Interior Composition ExploreR. It’s a one-meter-cube X-ray telescope built at NASA Goddard Space Flight Center that’s attached to the International Space Station. X-rays from space can’t get through Earth’s atmosphere, which is great for humans but inconvenient for X-ray astronomers, so we have to put X-ray telescopes up on satellites. NICER was launched in June 2017 in the ‘trunk’ of a SpaceX resupply mission, and is fully remotely operated without any input from the astronauts. Its detectors are sensitive to low-energy (‘soft’) X-ray photons in the 0.2 – 12 keV range, and it has roughly 100 nanosecond time resolution when recording photon arrival time, which is the fastest yet in an X-ray telescope. I’m a member of the NICER Science Team and I’ve been awarded observation time and NASA grant funding as both a Principal Investigator and Co-Investigator on different proposals.

STROBE-X: next-generation space telescope

STROBE-X initial diagram
Digital rendering of STROBE-X fully deployed in low-Earth orbit. Credit: NASA/NRL.

STROBE-X is a proposed X-ray space telescope that would provide an unprecedented view of the X-ray sky on timescales from microseconds to years. We received NASA funding for a concept study and submitted a mission proposal to the Astro2020 Decadal Survey (read the white paper here). If selected, STROBE-X would be the high-energy astrophysics telescope with the largest surface area and biggest data capabilities, so that we can stare at the brightest X-ray sources in the night sky without blinking. The amount of surface area on the detectors for collecting light is really important, to get as many X-ray photons as possible. STROBE-X‘s core science goals include measuring how fast black holes in our galaxy are spinning, mathematically understanding the ultra-dense cores of neutron stars, and catching X-ray counterparts to LIGO-Virgo gravitational wave source.

Medium-sized “Probe-class” missions like STROBE-X have a ~$1-1.5B budget for development and 5-year nominal mission lifetime. Our fearless team leader and principal investigator is Dr. Paul Ray at the Naval Research Lab. As a member of the steering committee, I’m in charge of education and public outreach, including social media (check out our Facebook, Twitter, Youtube, and interviews on Soundcloud).

Open-source science with Stingray

Stingray logo

I’m one of three founding developers and the release manager for Stingray, an Astropy-affiliated Python library for timing and spectral-timing analysis of astronomical data. Along with Daniela Huppenkothen, Matteo Bachetti, and the many other people who’ve contributed to Stingray so far, we are making powerful modern statistical tools openly accessible to the fields of X-ray timing and spectral-timing. Read the Stingray paper for more details. If you want to get involved with Stingray, we’d love to hear from you, via a pull request, an issue, or on our Slack! See all my coding resources here.

Above: slides for an invited presentation I gave on Stingray at “The 9th Microquasar Workshop: Celebrating over 50 years of discovery” (Sept 2021, virtual).

If you’d like me to give a talk or write something about astronomy, either for an academic or general public audience, please get in touch.

2 thoughts on “Research”

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