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Related papers: Large-area Reflective Infrared Filters for Millime…

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Fundamentally new technology is described for constructing low areal mass density (1kg/m^2), high precision (< 10micron RMS) reflectors scalable to large apertures (10 to 20 meters) for use as the primary element of a telescope system. A…

Astrophysics · Physics 2009-09-25 Mark Dragovan

Since the start of full science operations from 2004, the Submillimeter Array has been implementing plans to expand IF bandwidths and upgrade receivers and cryostats. Metal mesh low-pass filters were designed to block infrared (IR)…

Instrumentation and Methods for Astrophysics · Physics 2022-08-09 Chao-Te Li , C. -Y. E. Tong , Ming-Jye Wang , Tse-Jun Chen , Yen-Pin Chang , Sheng-Feng Yen , Jen-Chieh Cheng , Wei-Chun Lu , Yen-Ru Huang

Infrared (IR) blocking filters are crucial for controlling the radiative loading on cryogenic systems and for optimizing the sensitivity of bolometric detectors in the far-IR. We present a new IR filter approach based on a combination of…

Instrumentation and Methods for Astrophysics · Physics 2018-05-23 C. D. Munson , S. K. Choi , K. P. Coughlin , J. J. McMahon , K. H. Miller , L. A. Page , E. J. Wollack

We present the design and performance of broadband and tunable infrared-blocking filters for millimeter and sub-millimeter astronomy composed of small scattering particles embedded in an aerogel substrate. The ultra-low-density (typically <…

Instrumentation and Methods for Astrophysics · Physics 2021-11-03 Thomas Essinger-Hileman , Charles L. Bennett , Lance Corbett , Haiquan Guo , Kyle Helson , Tobias Marriage , Mary Ann B. Meador , Karwan Rostem , Edward J. Wollack

As telescopes get larger, the size of a seeing-limited spectrograph for a given resolving power becomes larger also, and for ELTs the size will be so great that high resolution instruments of simple design will be infeasible. Solutions…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 J. Gordon Robertson , Joss Bland-Hawthorn

Future far-infrared astrophysics observatories will require focal plane arrays containing thousands of ultra-sensitive, superconducting detectors, each of which needs to be optically coupled to the telescope. At longer wavelengths, many…

Instrumentation and Methods for Astrophysics · Physics 2024-06-05 Nicholas F. Cothard , Thomas Stevenson , Jennette Mateo , Nicholas Costen , Kevin Denis , Joanna Perido , Ian Schrock , Frederick Wang , Jason Glenn

Microscopes and various forms of interferometers have been used for decades in optical metrology of objects that are typically larger than the wavelength of light {\lambda}. However, metrology of subwavelength objects was deemed impossible…

Gratings enable dispersive spectroscopy from the X-ray to the optical, and feature prominently in proposed flagships and SmallSats alike. The exacting performance requirements of these future missions necessitate assessing whether the…

Instrumentation and Methods for Astrophysics · Physics 2020-12-09 Casey T. DeRoo , Jared Termini , Fabien Grise , Randall L. McEntaffer , Benjamin D. Donovan , Chad Eichfeld

We propose a high thermal conductivity infrared (IR) filter using alumina for use in millimeter wave detection systems. We constructed a prototype two-layer anti-reflection (AR) coated alumina filter with a diameter of 100mm and a thickness…

Instrumentation and Methods for Astrophysics · Physics 2015-06-18 Yuki Inoue , Tomotake Matsumura , Masashi Hazumi , Adrian T. Lee , Takahiro Okamura , Aritoki Suzuki , Takayuki Tomaru , Hiroshi Yamaguchi

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

One of the problems of producing spectrographs for Extremely Large Telescopes (ELTs) is that the beam size is required to scale with telescope aperture if all other parameters are held constant, leading to enormous size and implied cost.…

Instrumentation and Methods for Astrophysics · Physics 2009-08-12 J. R. Allington-Smith

In traditional seeing-limited observations the spectrograph aperture scales with telescope aperture, driving sizes and costs to enormous proportions. We propose a new solution to the seeing-limited spectrograph problem. A massively…

Astrophysics · Physics 2009-11-13 Nicholas Konidaris , Joel Kubby , Andrew Sheinis

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…

Instrumentation and Methods for Astrophysics · Physics 2015-06-04 Yong Zhang , Jie Zhang , Dehua Yang , Guohua Zhou , Aihua Li , Guoping Li

Optical interferometry has been successful at achieving milliarcsecond resolution on bright stars. Imaging performance can improve greatly by increasing the number of baselines, which has motivated proposals to build large (~ 100 m) optical…

Instrumentation and Methods for Astrophysics · Physics 2015-06-18 Paul D. Nuñez , Antoine Labeyrie , Pierre Riaud

The increasing scale of cryogenic detector arrays for sub-millimeter and millimeter wavelength astrophysics has led to the need for large aperture, high index of refraction, low loss, cryogenic refracting optics. Silicon with n = 3.4, low…

The emerging technology of large (~ 10,000 pixel) submillimeter-wave bolometer arrays presents a novel optical design problem---how can such arrays be fed by diffraction-limited telescope optics where the primary mirror is less than 100,000…

Astrophysics · Physics 2015-06-24 Antony A. Stark

Optical metasurfaces, comprised of subwavelength nanostructures, hold a great promise to high-power laser optics but also a limited pertinence due to their currently limited aperture size, throughput and durability. Here, an alternative…

We present two prescriptions for broadband (~77 - 252 GHz), millimeter-wave antireflection coatings for cryogenic, sintered polycrystalline aluminum oxide optics: one for large-format (700 mm diameter) planar and plano-convex elements, the…

Infrared-blocking scattering aerogel filters have a broad range of potential applications in astrophysics and planetary science observations in the far-infrared, sub-millimeter, and microwave regimes. Successful dielectric modeling of…

MIDIR is the proposed thermal/mid-IR imager and spectrograph for the European Extremely Large Telescope (E-ELT). It will cover the wavelength range of 3 to at least 20 microns. Designed for diffraction-limited performance over the entire…

Astrophysics · Physics 2009-11-13 S. Kendrew , B. Brandl , R. Lenzen , L. Venema , H. U. Käufl , G. Finger , A. Glasse , R. Stuik
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