NGO: Revealing a Hidden Universe Bernard Schutz AEI, Potsdam, Germany & Cardiff University, Wales.
Hunt for Molecules in Local Universe Galaxies Santiago GARCIA-BURILLO Observatorio Astronómico Nacional (OAN)-Spain Hunt for Molecules, November 19-20,
The Birth and Assembly of Galaxies: the Relationship Between Science Capabilities and Telescope Aperture Betsy Barton Center for Cosmology University of.
Understand Galaxy Evolution with IR Surveys: Comparison between ISOCAM 15- m and Spitzer 24- m Source Counts as a Tool Carlotta Gruppioni – INAF OAB.
The Far-Infrared Universe: from the Universe’s oldest light to the birth of its youngest stars Jeremy P. Scott, on behalf of Locke D. Spencer Physics and.
Lecture #4 Observational facts Olivier Le Fèvre – LAM Cosmology Summer School 2014.
Image Credit: NASA,ESA and the Hubble SM4 ERO Team Michelle Cluver [email protected].
Dark Halos of Fossil Groups and Clusters Observations and Simulations Ali Dariush, Trevor Ponman Graham Smith University of Birmingham, UK Frazer Pearce.
Eric M. Wilcots University of Wisconsin-Madison. How and when did galaxies accrete their gas? Where and when did/do galaxies stop accreting gas?
1. A(n) ____ emits large amounts of energy but photographically appears to be a single point of light much like a star. a.a planet like Venus b.E galaxy.
Variability: who cares? or…. Photometric redshift for XMM-COSMOS sources M.Salvato, G. Hasinger, O. Ilbert, G. Zamorani, M.Brusa + COSMOS collaboration.
Malaysia09:Galaxy evolution and Environment Compact Groups’ Group: S. Borthakur, T. Ponman, J. Ramussen, M. S. Yun, D. Espada, U. Lisenfeld Malaysia09:Galaxy.
