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Herschel SPIRE FTS spectral mapping calibration.

Authors :
Benielli, Dominique
Polehampton, Edward
Hopwood, Rosalind
Griñón Marín, Ana
Fulton, Trevor
Imhof, Peter
Lim, Tanya
Lu, Nanyao
Makiwa, Gibion
Marchili, Nicola
Naylor, David
Spencer, Locke
Swinyard, Bruce
Valtchanov, Ivan
Wiel, Matthijs
Source :
Experimental Astronomy. Jul2014, Vol. 37 Issue 2, p357-367. 11p.
Publication Year :
2014

Abstract

The Herschel SPIRE Fourier transform spectrometer (FTS) performs spectral imaging in the 447-1546 GHz band. It can observe in three spatial sampling modes: sparse mode, with a single pointing on sky, or intermediate or full modes with 1 and 1/2 beam spacing, respectively. In this paper, we investigate the uncertainty and repeatability for fully sampled FTS mapping observations. The repeatability is characterised using nine observations of the Orion Bar. Metrics are derived based on the ratio of the measured intensity in each observation compared to that in the combined spectral cube from all observations. The mean relative deviation is determined to be within 2 %, and the pixel-by-pixel scatter is ∼ 7 %. The scatter increases towards the edges of the maps. The uncertainty in the frequency scale is also studied, and the spread in the line centre velocity across the maps is found to be ∼ 15 km s . Other causes of uncertainty are also discussed including the effect of pointing and the additive uncertainty in the continuum. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
09226435
Volume :
37
Issue :
2
Database :
Academic Search Index
Journal :
Experimental Astronomy
Publication Type :
Academic Journal
Accession number :
97072527
Full Text :
https://doi.org/10.1007/s10686-013-9367-9