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Left Swift, right Kepler. Credit NASA.

Two Steward Published Research Projects Noted By AAS-NOVA

AAS-NOVA, a set of research highlights from journals sponsored by the American Astronomical Society, has recognized two Steward papers in 2015.  The first, with local authors Peter Milne and Gautham Narayan, announced the discovery that type Ia supernovae change with redshift in a way that lowers the amount of cosmological acceleration.  A goal for Milne for 2016 is to quantify how much this lessens the amount of dark energy required by supernova distances.

The second, by local authors Gijs Mulders, Ilaria Pascucci, and Dániel Apai, using the Kepler spacecraft, showed that M dwarf stars host fewer large planets at small "heliocentric" distances than do more massive stars. These same M dwarfs, though, have more small planets within these smaller orbits than do the more massive stars.

A list of all of the cited research papers, including one by former Steward PhD student Eric Mamajek (a professor at Rochester) and former Steward PhD student Chris Fryer (an Affiliate at UA Physics, and a staff scientist at Los Alamos National Labs), can be found HERE.

5/5/16: SO/NOAO Joint Colloquium Series: Doug Finkbeiner, Harvard

Date: 
Thursday, May 5, 2016 - 4:00pm to 5:00pm
Room: 

Title: Mapping Galactic Dust in 3 Dimensions with Pan-STARRS1 and 2MASS

4/28/16: SO/NOAO Joint Colloquium Series: Scott Tremaine, IAS

Date: 
Thursday, April 28, 2016 - 4:00pm to 5:00pm
Room: 

Title: Three Problems in Exoplanet Dynamics

Abstract:
(i) Are exoplanet systems flat? Laplace argued, correctly, that the small inclinations of planetary orbits implied that the solar system formed from a flat disk. I will review the direct and circumstantial evidence on whether extrasolar planetary systems are also flat and discuss the implications for planet formation.

4/21/16: SO/NOAO Joint Colloquium Series: Christoph Baranec, Univ. of Hawaii

Date: 
Thursday, April 21, 2016 - 4:00pm to 5:00pm
Room: 

Title: Robo-AO and the Rapid Transient Surveyor

Abstract:
As new large-scale astronomical surveys greatly increase the number of objects targeted and discoveries made, the requirement for efficient follow-up observations is crucial. Adaptive optics imaging, which compensates for the image-blurring effects of Earth's turbulent atmosphere, is essential for these surveys, but the scarcity, complexity and high demand of current systems limits their availability for following up large numbers of targets.

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