Future UV, X-ray, and sub-millimeter telescopes and spectrometers have the potential to revolutionize our understanding of the formation and habitability of the modern universe.[1-4] Star formation, dark energy, and the composition of the intergalactic medium are only some of the key scientific topics that can be addressed by UV astronomy and astrophysics. Sub-millimeter astronomy can probe the fine structure of the cosmic microwave background, giving glimpses into the early universe immediately following the Big Bang.[5] Unfortunately, harnessing the full potential of UV instruments is difficult as there are significant materials challenges that constrain their performance. Most materials are highly absorbing in the UV and those few materi...
I review the development of UV and EUV astronomy, covering the spectral range from 5 to 300 nm, with...
The Ultraviolet Imaging Telescope (UIT) was designed to be able to obtain deep images of nearby gala...
The UV spectral range is a crucial window to investigate a large area of phenomena for the objects o...
We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronom...
International audienceProgress of modern astrophysics requires the access to the electromagnetic spe...
International audienceWith this paper we participate to the call for ideas issued by the European Sp...
Modern astrophysics is a mature science that has evolved from its early phase of discovery and class...
The following subject areas are covered: (1) the science program (star formation and origins of plan...
International audienceThe investigation of the emergence of life is a major endeavour of science. As...
We discuss the status of ultraviolet knowledge of Solar System objects. We begin with a short histor...
New and unique science opportunities in several different fields of astrophysics are offered by cond...
The growth of luminous structures and the building blocks of life in the Universe began as primordia...
International audienceIn the era of Extremely Large Telescopes, the current generation of 8-10m faci...
A brief historical review of the development of Vacuum Ultraviolet Astrophysics is given, which show...
UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, invest...
I review the development of UV and EUV astronomy, covering the spectral range from 5 to 300 nm, with...
The Ultraviolet Imaging Telescope (UIT) was designed to be able to obtain deep images of nearby gala...
The UV spectral range is a crucial window to investigate a large area of phenomena for the objects o...
We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronom...
International audienceProgress of modern astrophysics requires the access to the electromagnetic spe...
International audienceWith this paper we participate to the call for ideas issued by the European Sp...
Modern astrophysics is a mature science that has evolved from its early phase of discovery and class...
The following subject areas are covered: (1) the science program (star formation and origins of plan...
International audienceThe investigation of the emergence of life is a major endeavour of science. As...
We discuss the status of ultraviolet knowledge of Solar System objects. We begin with a short histor...
New and unique science opportunities in several different fields of astrophysics are offered by cond...
The growth of luminous structures and the building blocks of life in the Universe began as primordia...
International audienceIn the era of Extremely Large Telescopes, the current generation of 8-10m faci...
A brief historical review of the development of Vacuum Ultraviolet Astrophysics is given, which show...
UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, invest...
I review the development of UV and EUV astronomy, covering the spectral range from 5 to 300 nm, with...
The Ultraviolet Imaging Telescope (UIT) was designed to be able to obtain deep images of nearby gala...
The UV spectral range is a crucial window to investigate a large area of phenomena for the objects o...