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In this paper we present a novel telescope composed exclusively of thin, flat optical elements, each being a hot-pressed multi-layered structure combining the properties of a lens, its anti-reflection coating and frequency selection or…

天体物理仪器与方法 · 物理学 2025-01-03 Giorgio Savini , Peter Hargrave , Peter A. R. Ade , Alexey Shitvov , Rashmi Sudiwala , Giampaolo Pisano , Carole Tucker , Jin Zhang

Ground-based millimeter and sub-millimeter telescopes are attempting to image the sky with ever-larger cryogenically-cooled bolometer arrays, but face challenges in mitigating the infrared loading accompanying large apertures. Absorptive…

天体物理仪器与方法 · 物理学 2014-07-23 Z. Ahmed , J. A. Grayson , K. L. Thompson , C. L. Kuo , G. Brooks , T. Pothoven

Equipped with a suitable optical relay system, telescopes employing low-cost fixed primary mirrors could point and track while delivering high-quality images to a fixed location. Such an optical tracking system would enable liquid-mirror…

天体物理学 · 物理学 2009-11-06 Paul Hickson

A modified version of the folded aplanatic Gregory telescope equipped with a spherical two-lens corrector is proposed for observations requiring a high signal-to-noise ratio. The basic telescope model has an aperture of 400 mm (f/3.0), its…

天体物理仪器与方法 · 物理学 2017-12-06 V. Yu. Terebizh

Reflective imaging systems form an important part of photonic devices such as spectrometers, telescopes, augmented and virtual reality headsets or lithography platforms. Reflective optics provide unparalleled spectral performance and can be…

光学 · 物理学 2021-06-10 Yunfeng Nie , David R. Shafer , Heidi Ottevaere , Hugo Thienpont , Fabian Duerr

A microwave lens with highly reduced reflectance, as compared to conventional dielectric lenses, is proposed. The lens is based on two-dimensional or three-dimensional transmission-line networks that can be designed to have an effective…

光学 · 物理学 2009-11-13 Pekka Alitalo , Olli Luukkonen , Joni Vehmas , Sergei Tretyakov

High precision astrometry aims at source position determination to a very small fraction of the diffraction image size, in high SNR regime. One of the key limitations to such goal is the optical response variation of the telescope over a…

Active reflector is one of the key technologies for constructing large telescopes, especially for the millimeter/sub-millimeter radio telescopes. This article introduces a new efficient laser angle metrology system for the active reflector…

天体物理仪器与方法 · 物理学 2015-06-04 Yong Zhang , Jie Zhang , Dehua Yang , Guohua Zhou , Aihua Li , Guoping Li

Highly ambitious initiatives aspire to propel a miniature spacecraft to a neighboring star within a human generation, leveraging the radiation pressure of lasers for propulsion. One of the main challenges to achieving this enormous feat is…

光学 · 物理学 2025-01-16 Jin Chang , Wenye Ji , Xiong Yao , Arnold J. van Run , Simon Gröblacher

The distortion of images of faint background galaxies by (weak) gravitational lensing can be used to measure the mass distribution of the deflector. The image distortions can be used to define a weighted mean of the mass inside a circular…

天体物理学 · 物理学 2015-06-24 Peter Schneider

The spaceborne laser emission telescope is a core and critical component of the space gravitational wave detection system.Compared with ground-based telescopes, the on-orbit space environment is more complex and harsh, presenting higher…

天体物理仪器与方法 · 物理学 2026-03-10 Long Yongtao , Mo Yan , Cao Shengyi , Cao Jiamin , Zhao Lujia , Wang Haibo , Wang Shuangbao , Tan Hao , Liu Xiaohong , Wang Dawei , Ma Donglin

A form of prime focus corrector for the Gregory system is proposed that provides the sub-arcsecond field of view up to 3 degrees in diameter for the spectral range 0.35-0.90 microns. The corrector includes five lenses made of same glass…

天体物理学 · 物理学 2009-11-11 V. Yu. Terebizh

Technological advances will allow the placement of many Terahertz detectors at the focal plane of a single telescope. For a telescope of a given diameter and wavelength of operation, there is a limit to the number of usable detectors…

天体物理学 · 物理学 2007-05-23 Antony A. Stark

To explore capabilities of moderate-size optical telescopes in surveys, the set of 9 new wide-field designs having apertures up to 1 m is considered. All but one systems have angular field of view in a range 3.5-10 degrees and flat focal…

天体物理仪器与方法 · 物理学 2016-10-26 V. Yu. Terebizh

We propose a form of a lens corrector at the prime focus of a hyperboloidal mirror that provides a flat field of view up to 3 deg diameter at image quality D_{80} < 0.8 arcsec in integrated (0.32-1.10 mcm) light. The corrector consists of…

天体物理学 · 物理学 2014-10-13 V. Yu. Terebizh

We present near-field radio holography measurements of the Simons Observatory Large Aperture Telescope Receiver optics. These measurements demonstrate that radio holography of complex millimeter-wave optical systems comprising cryogenic…

A metasurface lens (meta-lens) bends light using nanostructures on a flat surface. Macroscopic meta-lenses (mm- to cm-scale diameter) have been quite difficult to simulate and optimize, due to the large area, the lack of periodicity, and…

光学 · 物理学 2016-03-04 Steven J. Byrnes , Alan Lenef , Francesco Aieta , Federico Capasso

Metalenses, artificially engineered subwavelength nanostructures to focus light within ultrathin thickness, promise potential for a paradigm shift of conventional optical devices. However, the aperture sizes of metalenses are usually bound…

A new 10 meter diameter telescope is being constructed for deployment at the NSF South Pole research station. The telescope is designed for conducting large-area millimeter and sub-millimeter wave surveys of faint, low contrast emission, as…

Optical spectroscopy techniques such as differential reflectance and transmittance have proven to be very powerful techniques to study 2D materials. However, a thorough description of the experimental setups needed to carry out these…

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