Development of high-sensitive 1.2 mm imaging radiometer with two-polarization antenna-coupled TES-bolometer array for ground-based 6-m optical telescope

2008 ◽  
Author(s):  
Alexander N. Vystavkin ◽  
Alla G. Kovalenko ◽  
Sergey V. Shitov ◽  
Andrey V. Pestryakov ◽  
Sergey E. Bankov ◽  
...  
Keyword(s):  
Optical Telescope ◽  
Tes Bolometer ◽  
Bolometer Array

Further Optimization of the APEX-SZ TES Bolometer Array

2009 ◽  
Author(s):  
B. Westbrook ◽  
P. A. R. Ade ◽  
A. N. Bender ◽  
H. M. Cho ◽  
J. Clarke ◽  
...  
Keyword(s):  
Tes Bolometer ◽  
Bolometer Array

Method for rapid performance validation of large TES bolometer array for POLARBEAR-2A using a coherent millimeter-wave source

2021 ◽  
Author(s):  
Yuuko Segawa ◽  
Haruaki Hirose ◽  
Daisuke Kaneko ◽  
Masaya Hasegawa ◽  
Shunsuke Adachi ◽  
...  
Keyword(s):  
Millimeter Wave ◽  
Wave Source ◽  
Tes Bolometer ◽  
Bolometer Array ◽  
Millimeter Wave Source ◽  
Performance Validation

scholarly journals TES Bolometer Array for the APEX-SZ Camera

2008 ◽  
Vol 151 (3-4) ◽  
pp. 697-702 ◽  
Author(s):  
J. Mehl ◽  
P. A. R. Ade ◽  
K. Basu ◽  
D. Becker ◽  
A. Bender ◽  
...  
Keyword(s):  
Tes Bolometer ◽  
Bolometer Array

scholarly journals The Swift Ultra-Violet/Optical Telescope

2005 ◽  
Vol 120 (3-4) ◽  
pp. 95-142 ◽  
Author(s):  
Peter W. A. Roming ◽  
Thomas E. Kennedy ◽  
Keith O. Mason ◽  
John A. Nousek ◽  
Lindy Ahr ◽  
...  
Keyword(s):  
Ultra Violet ◽  
Optical Telescope

scholarly journals ESA’s X-Ray Astronomy Mission, XMM

1990 ◽  
Vol 123 ◽  
pp. 129-140
Author(s):  
B.G. Taylor ◽  
A. Peacock
Keyword(s):  
Resolving Power ◽  
Science Program ◽  
Eccentric Orbit ◽  
Ccd Cameras ◽  
Optical Telescope ◽  
X Ray ◽  
Medium Resolution ◽  
Reflection Gratings ◽  
Better Than

AbstractESA’s X-ray Astronomy Mission, XMM, scheduled for launch in 1998, is the second of four cornerstones of ESA’s long term science program Horizon 2000. Covering the range from about 0.1 to 10 keV, it will provide a high throughput of 5000 cm2 at 7 keV with three independant telescopes, and have a spatial resolution better than 30 arcsec. Broadband spectrophotometry is provided by CCD cameras while reflection gratings provide medium resolution spectroscopy (resolving power of about 400) in the range 0.3–3 keV. Long uninterrupted observations will be made from the 24 hr period, highly eccentric orbit, reaching a sensitivity approaching 10−15 erg cm−2 s−1 in one orbit. A 30 cm UV/optical telescope is bore-sighted with the x-ray telescopes to provide simultaneous optical counterparts to the numerous serendipitous X-ray sources which will be detected during every observation.

Perspectives on primary mirror figure control for a space-based optical telescope

2000 ◽  
Author(s):  
Douglas C. Neam ◽  
Paul A. Lightsey ◽  
James H. Crocker
Keyword(s):  
Optical Telescope ◽  
Primary Mirror

Application of carbon-carbon composite for load-carrying cylinder in lunar optical telescope

2011 ◽  
Author(s):  
Fu Li ◽  
Ping Ruan ◽  
Ting Li ◽  
Gang-zhou Xu ◽  
Di Lu ◽  
...  
Keyword(s):  
Carbon Composite ◽  
Optical Telescope ◽  
Load Carrying
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