Inclusion of events on the AAS Calendar is for viewer information only and does not imply endorsement by the American Astronomical Society.
Aspen Center for Physics Summer Workshop: Black Hole Formation, Accretion, and Outflows Through Cosmic Time
The major topics of this workshop encompass a wide variety of physics that will bring together a multi-disciplinary group with common interests. Discussion will emphasize the role of new observational facilities...
Assessing Uncertainties in Hubble’s Constant Across the Universe
Multiphase Gas in Galaxy Groups
Time Domain Astronomy in the High Redshift Universe
The First Penn State SETI Symposium
The First Penn State SETI Symposium, Presented by the Penn State Extraterrestrial Intelligence Center.
Lyman Alpha Emitters Workshop and Lager Meeting
Compact Objects and Energetic Phenomena in the Multi-Messenger Era
Key words: neutron stars, black holes on all mass scales, electromagnetic waves, high-energy particles, gravitational waves, time domain
2020 Sagan Summer Workshop on Extreme Precision Radial Velocity
The Sagan Exoplanet Summer Workshops are held annually and provide opportunities for students, postdocs, and researchers to learn about the engineering and scientific application of exoplanet-related techniques used in...
Rubin Observatory (LSST) Project and Community Workshop
43rd Scientific Assembly of the Committee on Space Research (COSPAR) and Associated Events “COSPAR 2020”
Fundamentals of Gaseous Halos
Gas in the halos of galaxies dominates the universe's baryon budget, traces its dark-matter potential wells, and supplies the fuel for star formation. Circumgalactic gas has also long been suspected to regulate galaxy...
Multiwavelength Probes of Galactic Atmospheres
The circumgalactic medium (CGM) can be viewed as an atmosphere that surrounds a galaxy and sustains star formation within it. Much of what we know about the CGM has come from absorption-line spectroscopy, mainly in the...
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.