Formation and evolution of galaxies from UV/optical-NIR surveys Lucia Pozzetti INAF Osservatorio Astronomico di Bologna.
Herschel observations: contraints on dust attenuation and star formation histories at high redshift Véronique Buat Laboratoire dAstrophysique de Marseille.
Lyα Pumped Molecular Hydrogen Emission in the Planetary Nebulae NGC 6853 and NGC 3132 R.E. Lupu, K. France and S.R. McCandliss Johns Hopkins University,
What good are low frequencies? HI, neutral hydrogen, H 0, atomic hydrogen high redshifts and early times…. USS, GPS, … “enabling technologies” …multi-beaming,
Transients in RHESSI and Chromospheric flares H. Hudson Space Sciences Lab, UC Berkeley.
9/7/04Claus Leitherer: A Far-UV View1 Claus Leitherer (STScI) A Far-Ultraviolet View of Starburst Galaxies Claus Leitherer (STScI)
Z > 6 Surveys Represent the Current Frontier Motivation: - census of earliest galaxies (z=6, =0.95 Gyr) - contribution of SF to cosmic reionization -
FUSE LWRS aperture overlays on the NGC 6853 VLT 8.2-m image, obtained from ESO.
z > 6 Surveys Represent the Current Frontier
Shedding (Quasar) Light on High Redshift Galaxies Joseph F. Hennawi UC Berkeley Hubble Fellowship Symposium April 2, 2007.
Extremely Red NICMOS Objects in the Chandra Deep Fields
Shedding (Quasar) Light on High Redshift Galaxies
