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The upGREAT Dual Frequency Heterodyne Arrays for SOFIA

2018; World Scientific; Volume: 07; Issue: 04 Linguagem: Inglês

10.1142/s2251171718400147

2251-1725

C. Risacher, R. Güsten, J. Stützki, Heinz‐Wilhelm Hübers, R. Aladro, Andreas Bell, C. Buchbender, Denis Buchel, T. Csengeri, C. Durán, U. U. Graf, R. Higgins, C. E. Honingh, K. Jacobs, M. Justen, Bernd Klein, Marc Mertens, Yoko Okada, A. Parikka, P. Pütz, Nicolás Reyes, Heiko Richter, Oliver Ricken, D. Riquelme, Nick Rothbart, N. Schneider, R. Simon, M. Wienold, H. Wiesemeyer, Monika Ziebart, Paul Fusco, S. J. Rosner, Bill Wohler,

Superconducting and THz Device Technology

We present the performance of the upGREAT heterodyne array receivers on the SOFIA telescope after several years of operations. This instrument is a multi-pixel high resolution (R > 10^7) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receivers use 7-pixel subarrays configured in a hexagonal layout around a central pixel. The low frequency array receiver (LFA) has 2x7 pixels (dual polarization), and presently covers the 1.83-2.06 THz frequency range, which allows to observe the [CII] and [OI] lines at 158 um and 145 um wavelengths. The high frequency array (HFA) covers the [OI] line at 63 um and is equipped with one polarization at the moment (7 pixels, which can be upgraded in the near future with a second polarization array). The 4.7 THz array has successfully flown using two separate quantum-cascade laser local oscillators from two different groups. NASA completed the development, integration and testing of a dual-channel closed-cycle cryocooler system, with two independently operable He compressors, aboard SOFIA in early 2017 and since then, both arrays can be operated in parallel using a frequency separating dichroic mirror. This configuration is now the prime GREAT configuration and has been added to SOFIA's instrument suite since observing cycle 6.