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Building a Physical Understanding of Galaxy Evolution with Data-driven Astronomy
This program will initiate a discussion between the empirical exploration of the extremely large and diverse data sets from both observations and simulations and the deduction of the underlying physics, aiming to answer...
The Cosmic Web: Connecting Galaxies to Cosmology at High and Low Redshift
During this program, through talks and focussed discussion sessions, we expect to understand the web itself and its connections to galaxy formation, re-ionisation, and cosmology.
Applying for the NASA Hubble Fellowship: Q&A with Fellows
A group of current and incoming NHFP fellows will be holding a Zoom Q&A for early career astronomers from 12-1 pm EDT on August 31, 2022 to help demystify the fellowship application process and the fellowship experience...
CSQCD IX: From RHIC to Astrophysics, Probing the Quark-Gluon Plasma
The Banff meeting will focus on recent explorations of the quark-gluon phase using colliders (e.g. RHIC and LHC) and on the renewed interest in neutron and quark matter in astrophysics, particularly in the gravitational...
Our Galactic Ecosystem: Opportunities and Diagnostics in the Infrared and Beyond
The Galactic Ecosystems: Far Infrared Diagnostics and Opportunities
The Past, Present and Future of the VLA: Celebrating 40 Years
The National Radio Astronomy Observatory is organizing a science meeting to commemorate 40 years of operations of the Very Large Array, with VLA past, current, and future science highlights while looking forward toward...
White Dwarfs as Probes of the Evolution of Planets, Stars, the Milky Way and the Expanding Universe
This program is motivated by the recent observational insights concerning white dwarfs as individuals and as a population, based on the astrometry from Gaia and large photometric (e.g. Kepler,TESS, ZTF) and spectroscopic...
White Dwarfs from Physics to Astrophysics
Astrometric, photometric and spectroscopic all-sky surveys provide the first complete, unbiased view of the Galactic population of the most abundant type of stellar remnants: white dwarfs.
LISA Canada 2021 Workshop
The Laser Interferometer Space Antenna (LISA) mission is a space-based gravitational wave interferometer planned for launch in 2032. It promises major advances across a wide range of fields in physics and astronomy...
AAVSO Webinar, with Dr. David Whelan (Austin College)
AAVSO's free webinar is from 2:00 pm to about 3:00 pm ET, and features Dr. David Whelan (Austin College) presenting on "Classifying Algol C, the Non-Eclipsing Member of the beta Persei System."