Wide-field-of-view PtSi infrared focal plane array

1990 ◽  
Author(s):  
Edward T. Nelson ◽  
Kwok Y. Wong ◽  
Shozo Yoshizumi ◽  
D. Rockafellow ◽  
William Des Jardin ◽  
...  
Keyword(s):  
Focal Plane ◽  
Focal Plane Array ◽  
Field Of View ◽  
Wide Field ◽  
Infrared Focal Plane Array ◽  
Wide Field Of View

Wide field-of-view dual-focal-plane augmented reality display

2019 ◽  
Author(s):  
Ugur Yekta Basak ◽  
Seyedmahdi M. K. Kazempourradi ◽  
Erdem Ulusoy ◽  
Hakan Urey
Keyword(s):  
Augmented Reality ◽  
Focal Plane ◽  
Field Of View ◽  
Wide Field ◽  
Wide Field Of View

scholarly journals Focal plane tuning in wide-field-of-view microscope with Talbot pattern illumination

2011 ◽  
Vol 36 (12) ◽  
pp. 2179 ◽  
Author(s):  
Jigang Wu ◽  
Guoan Zheng ◽  
Zheng Li ◽  
Changhuei Yang
Keyword(s):  
Focal Plane ◽  
Field Of View ◽  
Wide Field ◽  
Wide Field Of View

scholarly journals Okayama Astrophysical Observatory Wide-Field Camera

2019 ◽  
Vol 71 (6) ◽  
Author(s):  
Kenshi Yanagisawa ◽  
Yasuhiro Shimizu ◽  
Kiichi Okita ◽  
Daisuke Kuroda ◽  
Hironori Tsutsui ◽  
...  
Keyword(s):  
Focal Plane ◽  
Near Infrared ◽  
Galactic Plane ◽  
Focal Plane Array ◽  
Variable Stars ◽  
Field Of View ◽  
Wide Field

Abstract We report on the development of a wide-field near-infrared (0.9–2.5$\, \mu$m) camera built as a renewal of the existing classical Cassegrain 0.91 m telescope at Okayama Astrophysical Observatory. The optics system was replaced with fast hybrid optics (f/2.5) composed of forward Cassegrain optics and quasi-Schmidt optics, which results in an effective image circle of 52 mm diameter on the focal plane. The new camera, called the Okayama Astrophysical Observatory Wide-Field Camera (OAOWFC), has imaging capabilities in the $Y$, $J$, $H$, and $K_{\rm s}$ bands over a field of view of $0.^{\!\!\!\circ }47 \times 0.^{\!\!\!\circ }47$ with a HAWAII-1 HgCdTe PACE focal plane array. The primary purpose of OAOWFC is to search for variability in the Galactic plane in the $K_{\rm s}$ band and to promptly follow up transients. We have demonstrated a photometric repeatability of 2% in the densest field in the northern Galactic plane and successfully discovered previously unreported variable stars. The observations of OAOWFC are fully autonomous, and we started scientific operations in 2015 April.

Lessons learned from the optics and focal plane alignment of a wide field of view RC telescope

2005 ◽  
Author(s):  
Eugene D. Kim ◽  
Young-Wan Choi ◽  
Myung-Seok Kang ◽  
Ee-Eul Kim ◽  
Ho-Soon Yang ◽  
...  
Keyword(s):  
Focal Plane ◽  
Lessons Learned ◽  
Field Of View ◽  
Wide Field ◽  
Wide Field Of View

STM studies of crystal growth

1991 ◽  
Vol 49 ◽  
pp. 374-375
Author(s):  
M. G. Lagally
Keyword(s):  
Crystal Growth ◽  
Molecular Beam ◽  
Chemical Vapor ◽  
Sputter Deposition ◽  
Field Of View ◽  
Scanning Tunneling ◽  
Wide Field ◽  
Tunneling Microscopy ◽  
Wide Field Of View ◽  
The One

It has been recognized since the earliest days of crystal growth that kinetic processes of all Kinds control the nature of the growth. As the technology of crystal growth has become ever more refined, with the advent of such atomistic processes as molecular beam epitaxy, chemical vapor deposition, sputter deposition, and plasma enhanced techniques for the creation of “crystals” as little as one or a few atomic layers thick, multilayer structures, and novel materials combinations, the need to understand the mechanisms controlling the growth process is becoming more critical. Unfortunately, available techniques have not lent themselves well to obtaining a truly microscopic picture of such processes. Because of its atomic resolution on the one hand, and the achievable wide field of view on the other (of the order of micrometers) scanning tunneling microscopy (STM) gives us this opportunity. In this talk, we briefly review the types of growth kinetics measurements that can be made using STM. The use of STM for studies of kinetics is one of the more recent applications of what is itself still a very young field.

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