Authors
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Montenegro-Montes, Francisco Miguel
[European Southern Observatory (ESO)]
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Torstensson, Karl
[European Southern Observatory (ESO)]
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Parra, Rodrigo
[European Southern Observatory (ESO)]
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Pérez-Beaupuits, Juan Pablo
[European Southern Observatory (ESO)]
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Nyman, Lars-Åke
[European Southern Observatory (ESO)]
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Agurto, Claudio
[European Southern Observatory (ESO)]
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Azagra, Francisco
[European Southern Observatory (ESO)]
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Cárdenas, Mauricio
[European Southern Observatory (ESO)]
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González, Edouard
[European Southern Observatory (ESO)]
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MacAuliffe, Felipe
[European Southern Observatory (ESO)]
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Venegas, Paulina
[European Southern Observatory (ESO)]
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De Breuck, Carlos
[European Southern Observatory (ESO)]
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Bergman, Per
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Gunawan, Diah Setia
[IFA Universidad de Valparaíso, Chile]
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Wyrowski, Friedrich
[Max-Planck-Institut für Radiastronomie (MPIfR), Bonn, Germany]
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Stanke, Thomas
[European Southern Observatory (ESO)]
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Belitsky, Victor
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Fredrixon, Mathias
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Meledin, Denis
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Olberg, Michael
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Strandberg, Magnus
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Sundin, Erik
[Chalmers University of Technology, Onsala Space Observatory (OSO), Sweden]
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Adema, Joost
[NOVA Submillimetre Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, the Netherlands]
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Barkhof, Jan
[NOVA Submillimetre Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, the Netherlands]
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Baryshev, Andrey
[NOVA Submillimetre Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, the Netherlands]
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Hesper, Ronald
[NOVA Submillimetre Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, the Netherlands]
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Khudchenko, Andrey
[NOVA Submillimetre Instrumentation Group, Kapteyn Astronomical Institute, University of Groningen, the Netherlands]
Section
Telescopes and Instrumentation
Abstract
During Science Verification of the new SEPIA660 facility receiver at APEX, we carried out a shallow line survey of the archetypal Kleinmann-Low Nebula in the Orion star forming region (Orion-KL). These observations cover the tuning range towards the band edges, which has recently been extended beyond ALMA Band 9 specifications. At these frequencies, atmospheric transmission is very low but still sufficient to detect bright lines in Orion-KL. We present the collected spectra and compare with surveys from the literature, demonstrating the capabilities of the instrument.
Dates
Created: 2019-06-01/2019-06-30
Cite this article:
Montenegro-Montes, F., Torstensson, K., Parra, R., Pérez-Beaupuits, J., Nyman, L., Agurto, C., Azagra, F., Cárdenas, M., González, E., MacAuliffe, F., Venegas, P., De Breuck, C., Bergman, P., Gunawan, D., Wyrowski, F., Stanke, T., Belitsky, V., Fredrixon, M., Meledin, D., Olberg, M., Strandberg, M., Sundin, E., Adema, J., Barkhof, J., Baryshev, A., Hesper, R., Khudchenko, A.; Orion-KL Observations with the Extended Tuning Range of the New SEPIA660 APEX Facility Instrument. The Messenger 176 (June 2019): 20–24. https://doi.org/10.18727/0722-6691/5137