The upGREAT 1.9 THz multi-pixel high resolution spectrometer for the SOFIA Observatory
Author
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Risacher, C.
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Guesten, R.
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Stutzki, J.
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Huebers, H.
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Bell, A.
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Buchbender, C.
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Buechel, D.
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Csengeri, T.
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Graf, U.
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Heyminck, S.
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Higgins, R.
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Honingh, C.
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Jacobs, K.
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Klein, B
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Okada, D.
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Parikka, A.
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Puetz, P.
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Reyes Guzmán, Nicolás Andrés
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Ricken, O.
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Riquelme, D.
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Simon, R.
Author
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Wiesemeyer, H.
Admission date
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2017-12-12T21:16:51Z
Available date
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2017-12-12T21:16:51Z
Publication date
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2016
Cita de ítem
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A&A 595, A34 (2016)
es_ES
Identifier
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1432-0746
Identifier
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10.1051/0004-6361/201629045
Identifier
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https://repositorio.uchile.cl/handle/2250/146151
Abstract
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We present a new multi-pixel high resolution (R greater than or similar to 10(7)) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receiver uses 2 x 7-pixel subarrays in orthogonal polarization, each in an hexagonal array around a central pixel. We present the first results for this new instrument after commissioning campaigns in May and December 2015 and after science observations performed in May 2016. The receiver is designed to ultimately cover the full 1.8-2.5 THz frequency range but in its first implementation, the observing range was limited to observations of the [CII] line at 1.9 THz in 2015 and extended to 1.83-2.07 THz in 2016. The instrument sensitivities are state-of-the-art and the first scientific observations performed shortly after the commissioning confirm that the time efficiency for large scale imaging is improved by more than an order of magnitude as compared to single pixel receivers. An example of large scale mapping around the Horsehead Nebula is presented here illustrating this improvement. The array has been added to SOFIA's instrument suite already for ongoing observing cycle 4
es_ES
Patrocinador
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Federal Ministry of Economics and Technology via the German Space Agency (DLR)
50 OK 1102
50 OK 1103
50 OK 1104
Collaborative Research Centre 956 - Deutsche Forschungsgemeinschaft (DFG)