Slide 1Formation and evolution of galaxies from UV/optical-NIR surveys Lucia Pozzetti INAF Osservatorio Astronomico di Bologna Slide 2 o Why a survey in UV/optical or near-IR…

Slide 1 what good are low frequencies? HI, neutral hydrogen, H 0, atomic hydrogen high redshifts and early times…. USS, GPS, … “enabling technologies” …multi-beaming,…

Slide 1 Slide 2 Transients in RHESSI and Chromospheric flares H. Hudson Space Sciences Lab, UC Berkeley Slide 3 Transients in RHESSI * and Chromospheric flares H. Hudson…

Slide 1 9/7/04Claus Leitherer: A Far-UV View1 Claus Leitherer (STScI) A Far-Ultraviolet View of Starburst Galaxies Claus Leitherer (STScI) Slide 2 9/7/04Claus Leitherer:…

Slide 1 Stellar Surface Structures Surface features associated with activity –Chromospheres –Spots –Plage –Coronal holes –Flares Types of stellar activity –Solar-type…

z > 6 Surveys Represent the Current Frontier Motivation: census of earliest galaxies (z=6, =0.95 Gyr) - contribution of SF to cosmic reionization - constraints on early…

z > 6 Surveys Represent the Current Frontier Motivation: census of earliest galaxies (z=6, =0.95 Gyr) - contribution of SF to cosmic reionization - constraints on early…

Dust Obscuration and Metallicity at z~2: Implications for the Selection and Stellar Populations of High-Redshift Galaxies Collaborators: Chuck Steidel (Caltech), Max Pettini…

Dynamical Properties of Forming Galaxies at Redshift z > 5 Yoshi Taniguchi Research Center for Space & Cosmic Evolution Ehime University ZOO of Star-Forming Galaxies…

Diapositive 1 Herschel observations: contraints on dust attenuation and star formation histories at high redshift Véronique Buat Laboratoire d’Astrophysique de Marseille…