Jun 27 @ 2:30 pm – 3:30 pm
Colloquium PhD Defense: Laura Mayorga @ Domenici Hall 102
The Orbital and Planetary Phase Variations of Jupiter-Sized Planets: Characterizing Present and Future Giants Laura Mayorga, NMSU It is commonly said that exoplanet science is 100 years behind planetary science. While we may be able...
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Jul 3 @ 2:00 pm – 3:00 pm
Colloquium PhD Defense: Nigel Mathes
The Vulture Survey of MgII and CIV Absorbers: Feasting on the Bones of Spectra Left to Die Nigel Mathes, NMSU Abstract: We present detailed measurements of the absorption properties and redshift evolution of MgII and...
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Sep 20 @ 3:00 pm – 4:15 pm
Colloquium PhD Defense: Jean McKeever @ Business College 103
Asteroseismology of Red Giants: The Detailed Modeling of Red Giants in Eclipsing Binary Systems Jean McKeever, NMSU Asteroseismology is an invaluable tool that allows one to peer into the inside of a star and know...
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Colloquium PhD Thesis Defense: Ethan Dederick @ Science Hall 109
Seismic Inferences of Gas Giant Planets: Excitation & Interiors Ethan Dederick, NMSU Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars. In...
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Colloquium: Dave Thilker (Host: Rene Walterbos) @ BX102
Fresh Perspectives on Star Formation from LEGUS, the Legacy ExtraGalactic Ultraviolet Survey David Thilker, Johns Hopkins University The Legacy ExtraGalactic Ultraviolet Survey (LEGUS) was a Cycle 21 Large Treasury HST program which obtained ~parsec resolution NUV- to I-band WFC3 imaging for 50 nearby, representative star-forming Local Volume galaxies, with a primary goal of...
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Jan 23 @ 3:00 pm – 4:00 pm
Colloquium Thesis Defense: Lauren Kahre
Extinction Mapping and Dust-to-Gas Ratios of Nearby Galaxies Lauren Kahre, NMSU We present a study of the dust{to{gas ratios in 31 nearby (D > 10 Mpc) galaxies. Using Hubble Space Telescope broad band WFC3/UVIS UV...
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Colloquium: Lisa Young (Host: Rene Walterbos) @ BX102
Cold Gas and the Evolution of Early-type Galaxies Lisa Young, New Mexico Tech A major theme of galaxy evolution is understanding how today’s Hubble sequence was established — what makes some galaxies red spheroidals and...
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