Browsing Physics & Astronomy by Subject "Calibration"

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  • Marchili, N.; Hopwood, R.; Fulton, T.; Polehampton, E. T.; Valtchanov, I.; Zaretski, J.; Naylor, David A.; Griffin, M. J.; Imhof, P.; Lim, T.; Lu, N.; Makiwa, G.; Pearson, C.; Spencer, L. (Oxford University PressArts and ScienceDepartment of Physics and AstronomyIAPS-INAFImperial College LondonUniversity of LethbridgeBlue Sky SpectroscopyRutherford Appleton LaboratoryHerschel Science CentreCardiff UniversityChinese Academy of SciencesThe Open UniversityUniversity of Oxfordhttps://doi.org/10.1093/mnras/stw2600, 2017)
    The SPIRE Fourier Transform Spectrometer on-board the Herschel Space Observatory had two standard spectral resolution modes for science observations: high resolution (HR) and low resolution (LR), which could also be performed ...
  • Swinyard, B. M.; 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, M. J.; Lim, T. L.; Makiwa, G.; Naylor, David A.; Orton, G. S.; Papageorgiou, A.; Pearson, C. P.; Schulz, B.; Sidher, S. D.; Spencer, L. D.; van der Wiel, M. H. D.; Wu, R. (Oxford University PressArts and ScienceDepartment of Physics and AstronomyUniversity College LondonRutherford Appleton LaboratoryUniversity of LethbridgeImperial College LondonEuropean Space Astronomy Centre (Spain)California Institute of TechnologyBlue Sky SpectroscopyUniversité d'Aix-MarseilleCNRSUniversità di PadovaUniversity of ManchesterCardiff UniversityThe Open Universityhttps://doi.org/10.1093/mnras/stu409, 2014)
    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∼450–1550GHz. In this ...