预报:索菲亚将有一台中红外照相机

IF 1.5 Q3 ASTRONOMY & ASTROPHYSICS Journal of Astronomical Instrumentation Pub Date : 2018-12-01 DOI:10.1142/S2251171718400056
T. Herter, J. Adams, G. Gull, J. Schoenwald, L. Keller, B. Pirger, C. Henderson, G. Stacey, T. Nikola, J. D. De Buizer, W. Vacca, K. Ennico
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引用次数: 14

摘要

我们描述了SOFIA望远镜(FORCAST)的微弱物体红外相机,该望远镜目前作为红外天文平流层天文台(SOFIA)的设施仪器运行。FORCAST在5–40[公式:见正文][公式:见文本]m波长范围内提供成像和中等分辨率光谱功能。在成像模式下,FORCAST有一个3.4[公式:见文本]的视场,像素为0.768[公式:见图文本]。FORCAST使用灰度,在选定的波长上提供长缝低分辨率([公式:见正文]–300)和短缝交叉分散中等分辨率光谱模式([公式,见正文]-1200)。在Spitzer和Herschel之前,FORCAST的发现阶段空间在于提供独特的光度带和/或光谱覆盖范围、更高的空间分辨率以及探索通常使空间天文台饱和的最亮光源。
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FORCAST: A Mid-Infrared Camera for SOFIA
We describe the Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST) which is presently operating as a facility instrument on the Stratospheric Observatory For Infrared Astronomy (SOFIA). FORCAST provides imaging and moderate resolution spectroscopy capability over the 5–40[Formula: see text][Formula: see text]m wavelength range. In imaging mode, FORCAST has a 3.4[Formula: see text] field-of-view with 0.768[Formula: see text] pixels. Using grisms, FORCAST provides long-slit low-resolution ([Formula: see text]–300) and short-slit, cross-dispersed medium-resolution spectroscopic modes ([Formula: see text]–1200) over select wavelengths. Preceded by both Spitzer and Herschel, the discovery phase space for FORCAST lies in providing unique photometric bands and/or spectroscopic coverage, higher spatial resolution and exploration of the brightest sources which typically saturate space observatories.
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来源期刊
Journal of Astronomical Instrumentation
Journal of Astronomical Instrumentation ASTRONOMY & ASTROPHYSICS-
CiteScore
2.30
自引率
7.70%
发文量
19
期刊介绍: The Journal of Astronomical Instrumentation (JAI) publishes papers describing instruments and components being proposed, developed, under construction and in use. JAI also publishes papers that describe facility operations, lessons learned in design, construction, and operation, algorithms and their implementations, and techniques, including calibration, that are fundamental elements of instrumentation. The journal focuses on astronomical instrumentation topics in all wavebands (Radio to Gamma-Ray) and includes the disciplines of Heliophysics, Space Weather, Lunar and Planetary Science, Exoplanet Exploration, and Astroparticle Observation (cosmic rays, cosmic neutrinos, etc.). Concepts, designs, components, algorithms, integrated systems, operations, data archiving techniques and lessons learned applicable but not limited to the following platforms are pertinent to this journal. Example topics are listed below each platform, and it is recognized that many of these topics are relevant to multiple platforms. Relevant platforms include: Ground-based observatories[...] Stratospheric aircraft[...] Balloons and suborbital rockets[...] Space-based observatories and systems[...] Landers and rovers, and other planetary-based instrument concepts[...]
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