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Authordc.contributor.authorRisacher, C. 
Authordc.contributor.authorGuesten, R. 
Authordc.contributor.authorStutzki, J. 
Authordc.contributor.authorHuebers, H. 
Authordc.contributor.authorBell, A. 
Authordc.contributor.authorBuchbender, C. 
Authordc.contributor.authorBuechel, D. 
Authordc.contributor.authorCsengeri, T. 
Authordc.contributor.authorGraf, U. 
Authordc.contributor.authorHeyminck, S. 
Authordc.contributor.authorHiggins, R. 
Authordc.contributor.authorHoningh, C. 
Authordc.contributor.authorJacobs, K. 
Authordc.contributor.authorKlein, B 
Authordc.contributor.authorOkada, D. 
Authordc.contributor.authorParikka, A. 
Authordc.contributor.authorPuetz, P. 
Authordc.contributor.authorReyes Guzmán, Nicolás Andrés 
Authordc.contributor.authorRicken, O. 
Authordc.contributor.authorRiquelme, D. 
Authordc.contributor.authorSimon, R. 
Authordc.contributor.authorWiesemeyer, H. 
Admission datedc.date.accessioned2017-12-12T21:16:51Z
Available datedc.date.available2017-12-12T21:16:51Z
Publication datedc.date.issued2016
Cita de ítemdc.identifier.citationA&A 595, A34 (2016)es_ES
Identifierdc.identifier.issn1432-0746
Identifierdc.identifier.other10.1051/0004-6361/201629045
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/146151
Abstractdc.description.abstractWe 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 4es_ES
Patrocinadordc.description.sponsorshipFederal 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)es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherEDP Scienceses_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceAstronomy & Astrophysicses_ES
Keywordsdc.subjectInstrumentation: spectrographses_ES
Keywordsdc.subjectTechniques: spectroscopices_ES
Títulodc.titleThe upGREAT 1.9 THz multi-pixel high resolution spectrometer for the SOFIA Observatoryes_ES
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorapces_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile