The Spectral and Photometric Imaging REceiver (SPIRE; Griffin et al. ), is one of the three instruments on the Herschel Space Observatory (Pilbratt et al. ). It has separate photo-metric and spectroscopic imaging subinstruments that take advan-tage of Herschel’s capabilities for submillimetre observations. The. The Herschel-SPIRE instrument and its in-flight performance () SPIRE Quick-Start Guide () Instrument and systems: SPIRE fact sheet () SPIRE Fourier Transform Spectrometer fact sheet () SPIRE Data Products Overview. SPIRE Products Explained () SPIRE Highly Processed Data Products [HPDPs] () SPIRE Ancillary Data Products. The Herschel -SPIRE instrument and its in-flight performance. Download. The Herschel -SPIRE instrument and its in-flight performance. N. Schneider. Luca Conversi + 23 More. N. Schneider. Luca Conversi. Mattia Vaccari. Mattia Vaccari. Mattia Vaccari. George Bendo. Dominique Benielli. Matt Griffin. Steve Guest. Nanyao Lu.
ESA Herschel Space Observatory (Herschel; Pilbratt et al. ) between May and April. It contains an imaging pho- (SPIRE Observer's Manual ). Note that in general (except for very bright sources), the fringing shown in the top plot of Fig. 2 is successfully removed by the calibration scheme as it is. 04 Herschel DPU/ICU Subsystem Development Plan 05 DPU/ICU www.doorway.ru 06 DPU/ICU OBS Product Assurance Plan 07 DPU/ICU Switch-ON Procedure 08 SPIRE DPU Interface Control Document 09 Herschel PS-ICD 10 SPIRE DPU OBS URD 11 SPIRE DPU OBS User Manual 12 Herschel DPU/ICU Spacecraft Interface Acceptance Test Plan Reference Documents. The Herschel SPIRE Fourier transform spectrometer (FTS) performs spectral imaging in the GHz band. It can observe in three spatial sampling modes: sparse mode, with a single pointing on.
SPIRE instrument overview The Spectral and Photometric Imaging Receiver (SPIRE; Griffin et al. ) consists of a three-band imaging photometer and a two-band imaging Fourier-Transform Spectrometer (FTS). This sub-mm instrument operated on board the Herschel Space Observatory (Pilbratt et al., ) between May and April The Spectral and Photometric Imaging REceiver (SPIRE; Griffin et al. ), is one of the three instruments on the Herschel Space Observatory (Pilbratt et al. ). It has separate photo-metric and spectroscopic imaging subinstruments that take advan-tage of Herschel’s capabilities for submillimetre observations. The. A combined Herschel and XMM-Newton (x-ray) image of M31 showing dusty star-forming regions (Herschel) and the point-sources that represent highly evolved stars (XMM-Newton). The Herschel data were taken at microns with SPIRE between 17 and 21 December
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