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Upcoming Events

Billion km coherent telescopes: using the ISM lenses for pico-arcsecond measurements of pulsar properties.

Billion km coherent telescopes: using the ISM... 2/5/2015 4:00pm

Lecture / Astronomy

Abstract: We present a new technique ‘VLBI scintillometry’ which uses VLBI to resolve the interstellar plasma lenses and then in turn uses these billion km...

The Maryanne Shelley Jessup MacConochie Colloquium: “Small Planets, Small Stars"

The Maryanne Shelley Jessup MacConochie... 2/12/2015 4:00pm

Lecture / Astronomy

The Maryanne Shelley Jessup MacConochie Colloquium: Abstract: Small stars and small planets are ubiquitous in the Galaxy. Planets smaller than ~2.5 Earth...

The Josephine Lawrence Hopkins Foundation Colloquium Presents: Many rocky exoplanets around red dwarf stars are likely to be tidally locked, with permanent day and night sides. In such cases, condensation of the atmosphere on the planet's night side can o

The Josephine Lawrence Hopkins Foundation... 2/19/2015 4:00pm

Lecture / Astronomy

The Josephine Lawrence Hopkins Foundation Colloquium Presents: Many rocky exoplanets around red dwarf stars are likely to be tidally locked, with permanent...

Salpeter Lecture, Astronomy Colloquium: Baryon Acoustic Oscillations: A Robust and Precise Route to the Cosmological Distance Scale

Salpeter Lecture, Astronomy Colloquium: Baryon... 2/26/2015 4:00pm

Lecture / Astronomy

I will discuss how the acoustic oscillations that propagate in the photon-baryon fluid during the first million years of the Universe provide a robust method...

Dwarfs Structural Properties: Feedback and Environmental Effects

Dwarfs Structural Properties: Feedback and... 3/5/2015 4:00pm

Lecture / Astronomy

Reproducing the properties of dwarf galaxies in the field but also as satellites of larger objects often challenges our models of galaxy formation within...

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