[PDF] from infn.itM Quinto, M Berretti, E David, F Garcia… - Nuclear Physics B- …, 2011 - Elsevier ... M. Quinto et al. / Nuclear Physics B (Proc. Suppl.) 215 (2011) 225 227226 3. THE T2 TELESCOPE TEST AND CHARACTERIZATION Each of the four T2 quarters has been tested and characterized during the test-beam campaign at the SPS beam line H8 (2008 - 2009). ... Related articles - All 3 versions
RA Kimble… - American Astronomical Society Meeting …, 2011 - adsabs.harvard.edu With the delivery of its flight scientific instruments and the completion of all telescope optics both scheduled to occur later this year, the James Webb Space Telescope (JWST) will enter into a challenging integration and test (I&T) program. Highlights of that program include cryo- ...
[PDF] from arxiv.orgK Kamegai, M Tsuboi… - Arxiv preprint arXiv:1101.5682, 2011 - arxiv.org ... corresponds to an additional noise temperature of 3 K. Therefore, an antenna surface material with a low noise factor and high mechanical robustness is essential for the construction of a space radio telescope. 3. Thermal Cycle Test 3.1. Test Conditions ... Related articles - All 3 versions
R Brillhart, K Napolitano… - Advanced Aerospace Applications, …, 2011 - Springer ... Following an extensive twenty-four-year development and flight test process, this flying telescope has now started its service phase with its first science missions. ... SOFIA overcomes these limitations by installing the telescope in a flying test bed 747SP aircraft. ... Related articles - All 3 versions
[PDF] from arxiv.orgS Jeong, KB Ahn, JW Nam, IH Park… - Arxiv preprint arXiv: …, 2011 - arxiv.org ... SMT is a Ritchey-Chrétien telescope of 100 mm in diameter with a mo- torized slewing mirror at the entrance providing 17×17 arcmin2 in Field of View (FOV) and 4 arcsec in pixel resolution. ... SMT was aligned to RMS 0.05 waves in WFE (test wavelength 632.8nm). ... Cited by 1 - Related articles - All 2 versions
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