Zobrazeno 1 - 4
of 4
pro vyhledávání: '"B. R. Hohl"'
Autor:
Michael P. Biskach, Kai-Wing Chan, Rebecca A. Espina, William W. Zhang, Timo T. Saha, B. R. Hohl, Ryan S. McClelland
Publikováno v:
SPIE Proceedings.
Lightweight and high resolution optics are needed for future space-based x-ray telescopes to achieve advances in highenergy astrophysics. NASA’s Next Generation X-ray Optics (NGXO) project has made significant progress towards building such optics,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a9bc5404767765d8790060a4a32e96e
https://doi.org/10.1117/12.2056820
https://doi.org/10.1117/12.2056820
Autor:
W. W. Zhang, M. P. Biskach, V. T. Bly, J. M. Carter, K. W. Chan, J. A. Gaskin, M. Hong, B. R. Hohl, W. D. Jones, J. J. Kolodziejczak, L. D. Kolos, J. R. Mazzarella, R. S. McClelland, K. P. McKeon, T. M. Miller, S. L. O'Dell, R. E. Riveros, T. T. Saha, M. J. Schofield, M. V. Sharpe, H. C. Smith
Publikováno v:
SPIE Proceedings.
Future x-ray astronomical missions require x-ray mirror assemblies that provide both high angular resolution and large photon collecting area. In addition, as x-ray astronomy undertakes more sensitive sky surveys, a large field of view is becoming in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::85c66b6bb5703c11cbfedaffa2e68d24
https://doi.org/10.1117/12.2055339
https://doi.org/10.1117/12.2055339
Autor:
Ryan S. McClelland, Rebecca A. Espina, William W. Zhang, Michael P. Biskach, B. R. Hohl, Timo T. Saha, Elizabeth A. Matson, Kai-Wing Chan
Publikováno v:
SPIE Proceedings.
Lightweight and high resolution optics are needed for future space-based X-ray telescopes to achieve advances in high-energy astrophysics. The Next Generation X-ray Optics (NGXO) team at NASA GSFC is nearing mission readiness for a 10 arc-second Half
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::69697a9a1bb2a273564f35f5e4ff49cc
https://doi.org/10.1117/12.2024269
https://doi.org/10.1117/12.2024269
Autor:
Kai-Wing Chan, James R. Mazzarella, Linette D. Kolos, Timo T. Saha, William W. Zhang, Melinda Hong, B. R. Hohl, Ryan S. McClelland, Marton V. Sharpe
Publikováno v:
SPIE Proceedings.
Next generations lightweight, high resolution, high throughput optics for x-ray astronomy requires integration of very thin mirror segments into a lightweight telescope housing without distortion. Thin glass substrates with linear dimension of 200 mm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac6016fdc70b73957c23ba04b734671c
https://doi.org/10.1117/12.2022444
https://doi.org/10.1117/12.2022444