English
Related papers

Related papers: Three-Mirror Anastigmat Telescope with an Unvignet…

200 papers

A complete description is given of two-mirror telescopes with a flat medial focal surface, on which the images of stars are circles of least confusion. Particular attention is paid to aplanats, since their field of view is noticeably larger…

Instrumentation and Methods for Astrophysics · Physics 2022-07-20 V. Yu. Terebizh

We present the development of Linear Astigmatism Free - Three Mirror System (LAF-TMS). This is a prototype of an off-axis telescope that enables very wide field of view (FoV) infrared satellites that can observe Paschen-$\alpha$ emission,…

Instrumentation and Methods for Astrophysics · Physics 2020-03-25 Woojin Park , Seunghyuk Chang , Jae Hyuk Lim , Sunwoo Lee , Hojae Ahn , Yunjong Kim , Sanghyuk Kim , Arvid Hammar , Byeongjoon Jeong , Geon Hee Kim , Hyoungkwon Lee , Dae Wook Kim , Soojong Pak

The utilization of a 6.5m monolithic primary mirror in a compact three-mirror anastigmat (TMA) telescope design offers unprecedented capabilities to accommodate various next generation science instruments. This design enables the rapid and…

Instrumentation and Methods for Astrophysics · Physics 2023-09-12 Daewook Kim , Heejoo Choi , Ewan S. Douglas

We investigate whether a three-mirror system, having secondary and the tertiary mirrors with surfaces warped by Zernike polynomials generated by active vase mirrors, is suitable to do the corrections of a fixed parabolic mirror observing at…

Astrophysics · Physics 2009-10-30 Gilberto Moretto , Ermanno F. Borra

Telescopes with unobstructed pupil are known to deliver clean point spread function (PSF) to their focal plane, in contrast to traditional telescopes with obstructed pupil. Recent progress in the manufacturing aspheric surfaces and mounting…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 Balasubramanian Singaravelu , Remi A. Cabanac

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…

Astrophysics · Physics 2007-05-23 Antony A. Stark

High throughput optical system is defined to possess the features of both large field of view (FOV) and high resolution. However, it is full of challenge to design such a telescope with the two conflicting specifications at the same time.…

Instrumentation and Methods for Astrophysics · Physics 2021-04-07 Huiru Ji , Zhengbo Zhu , Hao Tan , Yuefan Shan , Wei Tan , Donglin Ma

We consider using toroidal curved detectors to improve the performance of imaging optical systems. We demonstrate that some optical systems have an anamorphic field curvature. We consider an unobscured re-imaging three-mirror anastigmat as…

Instrumentation and Methods for Astrophysics · Physics 2018-06-22 Eduard Muslimov , Emmanuel Hugot , Marc Ferrari , Thibault Behaghel , Gerard R. Lemaitre , Melanie Roulet , Simona Lombardo

Aberration compensation with emphasis on the generalized spherical aberration components is discussed for plane-symmetric and anamorphic optical systems. A narrow field-of-view double-plane symmetric telescope objective containing…

Optics · Physics 2025-07-14 Dmitry Zhuridov

Active optics techniques in astronomy provide high imaging quality. This paper is dedicated to highly deformable active optics that can generate non-axisymmetric aspheric surfaces-or freeform surfaces-by use of a minimum number of…

Instrumentation and Methods for Astrophysics · Physics 2019-01-23 Gerard Lemaitre , Pascal Vola , Eduard Muslimov

Axially symmetric telescopes produce well known "Seidel" off-axis third-order aberration patterns: coma, astigmatism, curvature of field and distortion. When axial symmetry is broken by the small misalignments of optical elements,…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Paul L. Schechter , Rebecca Sobel Levinson

A perfect focus telescope is one in which all rays parallel to the axis meet at a point and give equal magnification there. It is shown that these two conditions define the shapes of both primary and secondary mirrors. Apart from scale, the…

Optics · Physics 2009-11-07 D. Lynden-Bell

We present two novel designs for a telescope suitable for massively-multiplexed spectroscopy. The first is a very wide field Cassegrain telescope optimised for fibre feeding. It provides a Field Of View (FOV) of 2.5 degrees diameter with a…

Instrumentation and Methods for Astrophysics · Physics 2016-11-23 L. Pasquini , B. Delabre , R. Ellis , T. de Zeeuw

It is generally thought that correcting chromatic aberrations in imaging requires multiple surfaces. Here, we show that by allowing the phase in the image plane of a flat lens to be a free parameter, it is possible to correct chromatic…

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…

Astrophysics · Physics 2014-10-13 V. Yu. Terebizh

We present the design of an all-reflective, bi-folded Schmidt telescope aimed at surveys of extended astronomical objects with extremely-low surface brightness. The design leads to a high image quality without any diffracting spider, along…

Instrumentation and Methods for Astrophysics · Physics 2018-05-23 Eduard Muslimov , David Valls-Gabaud , Gérard Lemaître , Emmanuel Hugot , Wilfred Jahn , Simona Lombardo , Xin Wang , Pascal Vola , Marc Ferrari

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…

Astrophysics · Physics 2009-11-11 V. Yu. Terebizh

In this article we propose an original classification method for unobscured imaging systems unfolded in two dimensions. This classification is based on a study of off-axis properties, and relies on topology and algorithm of real algebraic…

Instrumentation and Methods for Astrophysics · Physics 2025-01-10 Benjamin Aymard , Andrea Delahaye , Audric Drogoul

Correcting astigmatism and ellipticity in laser beams is critical for improving performance in many applications like microscopy, atomic physics, quantum information processing, and advanced manufacturing. Passive correction methods based…

Optics · Physics 2025-06-30 Soroush Khoubyarian , Anastasiia Mashko , Alexandre Cooper

In the paper we present a low cost optical device which splits the light in the focal plane into two separate optical paths and collimates it back into a single image plane, and where a selective information processing ca be carried out.…

Instrumentation and Methods for Astrophysics · Physics 2016-08-24 Adam Popowicz , Tomasz Blachowicz
‹ Prev 1 2 3 10 Next ›