Slide 1 What can electromagnetic waves tell us about the movement of planets, stars, and galaxies? Slide 2 What happens when an object is emitting a constant frequency…
First impressions on Brewer processing methods survey Tomi Karppinen COST WG1/WG2 meeting Manchester, 27. September 2013 Replies By 24th September, 9 replies Arosa (Swizerland),…
WFC3 slitless spectroscopy Harald Kuntschner Martin Kümmel, Jeremy R. Walsh (ST-ECF) WFC3-team at STScI and NASA WFC3 Grism Parameters Disperser Channel Wavelength Resolution*…
Physics 1C Lecture 28B Compton effect: photons behave like particles when colliding with electrons. Electrons and particles in general can behave like a wave. Heisenberg…
WFC3 slitless spectroscopy Harald Kuntschner Martin Kümmel, Jeremy R. Walsh (ST-ECF) WFC3-team at STScI and NASA WFC3 Grism Parameters Disperser Channel Wavelength Resolution*…
Some Fact about LEDs and UV-radiation Labino AB Adisa Paulsson M.Sc., Product Development Engineer August 2010 Labino We develop and manufacture the UV and white light lamps…
Black Holes and the Universe – How the LHC re-creates the beginning of time Rene Bellwied Wayne State University ([email protected]) A public lecture Lessons from…
Galaxy Rotation: How we know Galaxy Rotation: How we knowAS41310/28/2014D. Clemens OutlineWays to detect that galaxies rotateMeasuring rotations of external galaxiesOur problematic…