Calibration of the Herschel SPIRE Fourier Transform Spectrometer

Article, Preprint English OPEN
Swinyard, Bruce; Polehampton, E. T.; Hopwood, R.; Valtchanov, I.; Lu, N.; Fulton, T.; Benielli, D.; Imhof, P.; Marchili, N.; Baluteau, J.- P.; Bendo, G. J.; Ferlet, M.; Griffin, Matthew Jason; Lim, T. L.; Makiwa, G.; Naylor, D. A.; Orton, G. S.; Papageorgiou, Andreas; Pearson, C. P.; Schulz, B.; Sidher, S. D.; Spencer, Locke; Van Der Wiel, M. H. D.; Wu, R.;
  • Publisher: Oxford University Press (OUP): Policy P - Oxford Open Option A
  • Related identifiers: doi: 10.1093/mnras/stu409
  • Subject: QC | Astrophysics - Instrumentation and Methods for Astrophysics | [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] | [ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Instrumentation and Methods for Astrophysics | Astrophysics::Solar and Stellar Astrophysics

International audience; The Herschel Spectral and Photometric REceiver (SPIRE) instrument consists of an imaging photometric camera and an imaging Fourier Transform Spectrometer (FTS), both operating over a frequency range of similar to 450-1550 GHz. In this paper, we b... View more
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