Proceedings ArticleDOI
A SPECS update: engineering and technology requirements for a space-based far-IR imaging interferometer
David Leisawitz,Ronald J. Allen,Charles Baker,Dominic J. Benford,Claudio Bombardelli,Michael J. DiPirro,Pascale Ehrenfreund,Neal J. Evans,Martin Harwit,T. Tupper Hyde,Antoine Labeyrie,Jesse Leitner,Alice Liu,Enrico C. Lorenzini,Richard G. Lyon,Anthony J. Martino,John C. Mather,Karl M. Menten,S. Harvey Moseley,Lee G. Mundy,Takao Nakagawa,Stanford Ollendorf,John C. Pearson,Dave Quinn,Stephen A. Rinehart,Juan Roman,Shobita Satyapal,Robert F. Silverberg,H. Philip Stahl,Mark R. Swain,Theodore D. Swanson,Wesley A. Traub,Edward L. Wright,Harold W. Yorke +33 more
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TLDR
The Submillimeter Probe of the Evolution of Cosmic Structure (SPECS) is a space-based imaging and spectral interferometer with kilometer maximum baseline lengths for imaging as mentioned in this paper.Abstract:
The Submillimeter Probe of the Evolution of Cosmic Structure (SPECS) is a space-based imaging and spectral ("double Fourier") interferometer with kilometer maximum baseline lengths for imaging. This NASA "vision mission" will provide spatial resolution in the far-IR and submillimeter spectral range comparable to that of the Hubble Space Telescope, enabling astrophysicists to extend the legacy of current and planned far-IR observatories. The astrophysical information uniquely available with SPECS and its pathfinder mission SPIRIT will be briefly described, but that is more the focus of a companion paper in the Proceedings of the Optical, Infrared, and Millimeter Space Telescopes conference. Here we present an updated design concept for SPECS and for the pathfinder interferometer SPIRIT (Space Infrared Interferometric Telescope) and focus on the engineering and technology requirements for far-IR double Fourier interferometry. We compare the SPECS optical system requirements with those of existing ground-based and other planned space-based interferometers, such as SIM and TPF-I/Darwin.read more
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Proceedings ArticleDOI
A Contamination‐Free Ultrahigh Precision Formation Flying Method for Micro‐, Nano‐, and Pico‐Satellites with Nanometer Accuracy
TL;DR: In this paper, the authors proposed a propellant free, thus contamination free, method that enables ultra-high precision satellite formation flying with intersatellite distance accuracy of nm (10−9 m) at maximum estimated distances in the order of tens of km.
Journal ArticleDOI
Luciola hypertelescope space observatory: versatile, upgradable high-resolution imaging, from stars to deep-field cosmology
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Journal ArticleDOI
Self-stabilising attitude control for spinning tethered formations
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Proceedings ArticleDOI
Space-based far-infrared interferometry technology development through a laboratory-based spatial/spectral interferometry testbed instrument
TL;DR: In this article, the authors describe progress in the development of a lab-based spatial/spectral double Fourier interferometer within the Astronomical Instrumentation Group (AIG) laboratories at the University of Lethbridge, Canada (UL).
Proceedings ArticleDOI
The wide-field imaging interferometry testbed: I. progress, results, and future plans
Stephen A. Rinehart,J. T. Armstrong,Bradley J. Frey,Jeff Kirk,David Leisawitz,Douglas B. Leviton,Luke W. Lobsinger,Richard G. Lyon,Anthony J. Martino,Thomas A. Pauls,Lee G. Mundy,E. Sears +11 more
TL;DR: The Wide Field Imaging Interferometry Testbed (WIIT) as discussed by the authors uses a multi-pixel detector for spatial multiplexing and has demonstrated the ability to acquire wide-field imaging interferometry data.