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Past Colloquia

Our Lonely Sun: How Multiple Star Systems Form (or don’t)

Cody Hall

Stella Offner, University of Texas at Austin

November 15, 2023
2:00pm - 3:00pm

Abstract: Most stars are born with one or more stellar companions. Observational advances over the last decade have enabled high-resolution, interferometric studies of forming multiple systems and statistical surveys of multiplicity in star-forming regions. These have yielded new insights into how such systems form and how multiplicity…

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Accreting massive black holes and QUVIK a Czech UV space telescope

Cody Hall

Norbert Werner,

November 08, 2023
2:00pm - 3:00pm

Most galaxies comparable to or larger than the mass of the Milky Way host hot, X-ray emitting atmospheres and accreting supermassive black holes. I will present results based on radio and X-ray observations, which indicate that in massive early-type galaxies, the central radio sources are…

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Sub-clusters and Gas and Binaries, oh my: Star Cluster Formation is Messy

Cody Hall

Alison Sills, McMaster University

November 01, 2023
2:00pm - 3:00pm

Stars are primarily formed in clustered environments in giant molecular clouds. Stars are also primarily found in binary or higher order multiple systems. This hierarchy of binaries inside clusters, particularly at early times, means that binary systems interact with other stars from the first moments…

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Reconstructing the physics of transients using machine learning

Cody Hall

Wolfgang Kerzendorf, Michigan State University

October 25, 2023
2:00pm - 3:00pm

Supernova explosions are some of the most energetic and luminous events in the universe, andunderstanding them is crucial for many areas of astrophysics. One way to gain insight into the physicalprocesses involved in these explosions is through supernova tomography, which involves reconstructinga spatially resolved explosion…

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How Black Holes Shine

Cody Hall

Prof. Bart Ripperda, CITA, University of Toronto

October 18, 2023
2pm - 3pm

Astrophysical black holes are surrounded by accretion disks, jets, and coronae consisting of magnetized relativistic plasma. They produce observable high-energy radiation from nearby the event horizon and it is currently unclear how this emission is exactly produced. The radiation typically has a non-thermal component, implying…

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Mind the Gap: The far-infrared gap and Canadian milestones on the Far-Infrared astrophysical roadmap

Cody Hall

Prof. Locke Spencer, University of Lethbridge

October 11, 2023
2:00pm - 3:00pm

Abstract: Over half of the energy emitted by the Universe appears in the relatively unexplored Far-Infrared (Far-IR) spectral region, which is virtually opaque from the ground and must be observed by space-borne instrumentation. The dominant limiting factor of many current open questions in astrophysics is…

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The Quantitative Reasoning Skills and Numerical Affect of Astronomy Students

Cody Hall

Kate Follette, Amherst College

October 04, 2023
2:00pm - 3:00pm

Much of the dialogue surrounding effective pedagogy for college-level general education astronomy courses has been focused on how best to engender  “science literacy”, yet students cannot be scientifically literate without also being quantitatively literate. Basic numerical skills such as graph reading, proportional reasoning, and estimation are tools that…

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From Pixels to Parameters

Cody Hall

Prof. Stephen Portillo, Concordia University

September 27, 2023
2:00pm - 3:00pm

Much of astronomy uses pixelized data, but the size and complexity of these data often strain the capability of existing data analysis techniques. I will present algorithms built on advances in statistics and machine learning that allow more science to be done with the same…

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U of T Astronomy Jamboree

BA 1130

Various Speakers from UofT Astro Units

September 20, 2023
2:00pm - 4:00pm

More information coming soon.

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Transcending the Limits of Astrostatistics with Machine Learning Methods

Virtual Colloquium

Yuan-Sen Ting, Australian National University

April 11, 2023
9:00 am - 10:00am

Astronomy has undergone a profound transformation in recent years, as the acquisition of ever-growing amounts of data through increasingly powerful instruments has opened up a wealth of new avenues of exploration. However, this boon is not without its own set of challenges, as astronomical observations…

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