ESPRIT - A study concept for a far-infrared interferometer in space

被引:8
作者
Wild, W. [1 ,6 ]
de Graauw, Th. [1 ,5 ]
Helmich, F. [1 ,6 ]
Baryshev, A. [1 ,6 ]
Cernicharo, J. [2 ]
Gao, J. R. [1 ]
Gunst, A. [3 ]
Bos, A. [3 ]
den Herder, J. -W. [1 ]
Jackson, B. [1 ]
Koshelets, V. [1 ,7 ]
Langevelde, H-J [4 ]
Maat, P. [3 ]
Martin-Pintado, J. [2 ]
Noordam, J. [3 ]
Roelfsema, P. [1 ,6 ]
Venema, L.
Wesselius, P. [1 ,6 ]
Yagoubov, P. [1 ]
机构
[1] Univ Groningen, SRON Netherlands Inst Space Res, POB 800, NL-9700 AV Groningen, Netherlands
[2] CSIC, E-28006 Madrid, Spain
[3] ASTRON, NL-7990 AA Dwingeloo, Netherlands
[4] Joint Inst VLBI Europe, NL-7990 AA Dwingeloo, Netherlands
[5] Leiden Observ, NL-2300 RA Leiden, Netherlands
[6] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
[7] IREE, Moscow 125009, Russia
来源
OPTICAL AND INFRARED INTERFEROMETRY | 2008年 / 7013卷
关键词
FarInfrared; Submillimeter; Interferometry; Space mission; Space Instrumentation; Star Formation; Spectroscopy;
D O I
10.1117/12.789603
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the far-infrared (FIR) / THz regime the angular (and often spectral) resolution of observing facilities is still very restricted despite the fact that this frequency range has become of prime importance for modern astrophysics. ALMA (Atacama Large Millimeter Array) with its superb sensitivity and angular resolution will only cover frequencies up to about 1 THz, while the HIFI instrument for ESA'a Herschel Space Observatory will provide limited angular resolution (10 to 30 arcsec) up to 2 THz. Observations of regions with star and planet formation require extremely high angular resolution as well as frequency resolution in the full THz regime. In order to open these regions for high-resolution astrophysics we present a study concept for a heterodyne space interferometer, ESPRIT (Exploratory Submm Space Radio-Interferometric Telescope). This mission will cover the Terahertz regime inaccessible from the ground and outside the operating range of the James Webb Space Telescope (JWST).
引用
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页数:10
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