SHARK-VIS: the upcoming high-resolution high-contrast visible imager for LBT
Aula GrattonSHARK-VIS is the visual channel (400-1000 nm) of SHARK, the upcoming extreme-AO instrument for the
10 eventi found.
SHARK-VIS: the upcoming high-resolution high-contrast visible imager for LBT
Aula GrattonSHARK-VIS is the visual channel (400-1000 nm) of SHARK, the upcoming extreme-AO instrument for the
Four years of science with SPHERE/VLT
Aula GrattonSPHERE/VLT is an extreme adaptive optics instrument designed to directly image exoplanets. It was designed
Four years of science with SPHERE/VLT
Aula GrattonSPHERE/VLT is an extreme adaptive optics instrument designed to directly image exoplanets. It was designed
The MESSIER surveyor: lifting the veil on the ultra low surface brightness universe
Aula GrattonThe MESSIER satellite has been designed to explore the extremely low surface brightness universe at
The MESSIER surveyor: lifting the veil on the ultra low surface brightness universe
Aula GrattonThe MESSIER satellite has been designed to explore the extremely low surface brightness universe at
Transient spiral arms and galaxy rotation curves
Aula GrattonThe complex spatial structure evident in spiral galaxies is understood either in terms of instabilities
Transient spiral arms and galaxy rotation curves
Aula GrattonThe complex spatial structure evident in spiral galaxies is understood either in terms of instabilities
What is the role of the environment in shaping early-type galaxy sizes? Has it changed in the last 10 Gyr?
Aula GrattonUnderstanding galaxy evolution requires understanding the impact of cosmic time, environment, mass, and halo growth
What is the role of the environment in shaping early-type galaxy sizes? Has it changed in the last 10 Gyr?
Aula GrattonUnderstanding galaxy evolution requires understanding the impact of cosmic time, environment, mass, and halo growth