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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…

天体物理仪器与方法 · 物理学 2023-09-12 Daewook Kim , Heejoo Choi , Ewan S. Douglas

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,…

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…

天体物理仪器与方法 · 物理学 2015-06-19 Balasubramanian Singaravelu , Remi A. Cabanac

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…

This article presents research work on a spectroscopic survey telescope. Our idea is as follows: for such a telescope, a pure reflecting optical system is designed, which should have an aperture and a field of view (FOV) both as large as…

天体物理仪器与方法 · 物理学 2024-03-20 Ding-qiang Su , Hua Bai , Xiangyan Yuan , Xiangqun Cui

A new optical design concept of telescopes to provide an aberration-free, wide field, unvignetted flat focal plane is described. The system employs three aspheric mirrors to remove aberrations, and provides a semi-circular field of view…

天体物理学 · 物理学 2015-06-24 Kyoji Nariai , Masanori Iye

The SuperNova/Acceleration Probe (SNAP) mission will require a two-meter class telescope delivering diffraction limited images spanning a one degree field in the visible and near infrared wavelength regime. This requirement, equivalent to…

天体物理学 · 物理学 2007-05-23 M. Lampton , SNAP Collaboration

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…

天体物理仪器与方法 · 物理学 2019-01-23 Gerard Lemaitre , Pascal Vola , Eduard Muslimov

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…

天体物理仪器与方法 · 物理学 2016-11-23 L. Pasquini , B. Delabre , R. Ellis , T. de Zeeuw

Cubesats present unique opportunities for observational astronomy in the modern era. They are useful in observing difficult-to-access wavelength regions and long-term monitoring of interesting astronomical sources. However, conventional…

天体物理仪器与方法 · 物理学 2025-07-14 Anwesh Kumar Mishra , Gourav Banerjee , Rekhesh Mohan , Maheswar Gopinathan

We present a concept of the X-ray imaging system with high angular-resolution and moderate sensitivity. In this concept, a two-dimensional detector, i.e., imager, is put at a slightly out-of-focused position of the focusing mirror, rather…

The Atacama Large Aperture Submillimeter Telescope (AtLAST) aims to be the premier next generation large diameter (50-meter) single dish observatory capable of observations across the millimeter/sub-millimeter spectrum, from 30 to 950~GHz.…

We develop a proto-model of an off-axis reflective telescope for infrared wide-field observations based on the design of Schwarzschild-Chang type telescope. With only two mirrors, this design achieves an entrance pupil diameter of 50 mm and…

天体物理仪器与方法 · 物理学 2015-03-17 Sanghyuk Kim , Soojong Pak , Seunghyuk Chang , Geon Hee Kim , Sun Choel Yang , Myung Sang Kim , Sungho Lee , Hanshin Lee

Reliable, autonomously, deployment of telescopes enables a wide range of possible science cases. In this paper, we present a method for multi-stage telescope alignment with a simple commercial imaging sensor. For these studies, we use a…

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

We present a design for a wide-field spectroscopic telescope. The only large powered mirror is spherical, the resulting spherical aberration is corrected for each target separately, giving exceptional image quality. The telescope is a…

天体物理仪器与方法 · 物理学 2024-09-11 Will Saunders , Timothy Chin , Michael Goodwin

Recently, Su et al. (2016) propose a telescope design, referred as the "SYZ" design, for Chinese new project of a 12m optical-infrared telescope. The SYZ telescope design consists of three aspheric mirrors with non-zero power, including a…

天体物理仪器与方法 · 物理学 2017-12-27 Donglin Ma , Zheng Cai

We present a robust but still efficient simulation approach for high-resolution scanning tunneling microscopy with a flexible tip apex showing sharp submolecular features. The approach takes into account the electronic structure of sample…

介观与纳米尺度物理 · 物理学 2017-01-11 O. Krejci , P. Hapala , M. Ondracek , P. Jelinek

We report a computational 3D microscopy technique, termed Fourier ptychographic diffraction tomography (FPDT), that iteratively stitches together numerous variably illuminated, low-resolution images acquired with a low-numerical aperture…

光学 · 物理学 2020-02-19 Chao Zuo , Jiasong Sun , Jiaji Li , Anand Asundi , Qian Chen

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…

天体物理仪器与方法 · 物理学 2018-06-22 Eduard Muslimov , Emmanuel Hugot , Marc Ferrari , Thibault Behaghel , Gerard R. Lemaitre , Melanie Roulet , Simona Lombardo
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