As the next major X-ray astronomical mission of NASA, ESA, and JAXA, the International X-ray Observatory (IXO) requires a mirror assembly that has an unprecedented effective area and an angular resolution better than all past missions except Chandra. This mirror assembly consists of approximately 15,000 mirror segments, which need to be fabricated, measured, aligned and integrated. In this talk we will present the latest results from our effort of developing an efficient and fast process of making these mirror segments by slumping commercially available glass sheets. We will report on our progress both in terms of perfecting the slumping process as well as the metrology process. In particular, we will discuss what additional work needs to b...
In the last decade Very High Energy (VHE) gamma-ray astronomy has improved rapidly opening a new win...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
NASA has been developing technology for the large area IXO mirror based on precise slumping of glass...
As for all space missions, the limit imposed on the payload mass budget by the launcher is the main ...
The International X-ray Observatory (IXO) mission requires a lightweight and high throughput spectro...
The XEUS mission (X-ray Evolving-Universe Spectroscopy Mission) of ESA, in the present configuration...
Future astronomical projects on large space x-ray imaging telescopes require novel substrates and te...
The International X-ray Observatory (IXO) is the next major space X-ray observatory, performing both...
Future x-ray astronomical missions require x-ray mirror assemblies that provide both high angular re...
A suspension-mounting scheme is developed for the IXO (International X-ray Observatory) mirror segme...
Future x-ray astronomical missions, like the International X-ray Observatory (IXO), will likely requ...
We report on the production and implementation of 100 square panels 1 m x 1 m, based on the innovati...
Figure correction of thin x-ray telescope mirrors may be critical for future missions that require h...
In the last decade Very High Energy (VHE) gamma-ray astronomy has improved rapidly opening a new win...
In the last decade Very High Energy (VHE) gamma-ray astronomy has improved rapidly opening a new win...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
NASA has been developing technology for the large area IXO mirror based on precise slumping of glass...
As for all space missions, the limit imposed on the payload mass budget by the launcher is the main ...
The International X-ray Observatory (IXO) mission requires a lightweight and high throughput spectro...
The XEUS mission (X-ray Evolving-Universe Spectroscopy Mission) of ESA, in the present configuration...
Future astronomical projects on large space x-ray imaging telescopes require novel substrates and te...
The International X-ray Observatory (IXO) is the next major space X-ray observatory, performing both...
Future x-ray astronomical missions require x-ray mirror assemblies that provide both high angular re...
A suspension-mounting scheme is developed for the IXO (International X-ray Observatory) mirror segme...
Future x-ray astronomical missions, like the International X-ray Observatory (IXO), will likely requ...
We report on the production and implementation of 100 square panels 1 m x 1 m, based on the innovati...
Figure correction of thin x-ray telescope mirrors may be critical for future missions that require h...
In the last decade Very High Energy (VHE) gamma-ray astronomy has improved rapidly opening a new win...
In the last decade Very High Energy (VHE) gamma-ray astronomy has improved rapidly opening a new win...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...