The relative spectral response calibration of the ISO-SWS

B. Vandenbussche*, P. W. Morris, E. A. Valentijn, D. A. Beintema, D. R. Boxhoorn, L. Decin, T. De Graauw, H. Feuchtgruber, A. M. Heras, F. Lahuis, R. Lorente, D. Lutz, P. R. Roelfsema, A. Salama, R. F. Shipman, R. Van Malderen, E. Wieprecht

*Corresponding author voor dit werk

OnderzoeksoutputAcademicpeer review

Samenvatting

The Relative Spectral Response Function (RSRF) characterises the wavelength dependent response of a spectrometer. The wavelength range of the grating section of the ISO-SWS is covered in 15 spectral bands for each of which the RSRF has to be determined. We discuss how the RSRF was measured during the Instrument Level Tests before launch, and how it was corrected based on in-orbit measurements of stellar calibration sources. Uncertainties in synthetic spectra and noise in the calibration observations can result in the introduction of erroneous spectral features in the RSRF. We show how this can be avoided by a careful selection of calibration sources across different spectral types and the use of spline smoothed correction curves.

Originele taal-2English
TitelThe Calibration Legacy of the ISO Mission
Pagina's455-458
Aantal pagina's4
StatusPublished - mei-2003
EvenementThe Calibration Legacy of the ISO Mission - madrid, Spain
Duur: 5-feb.-20019-feb.-2001

Publicatie series

NaamEuropean Space Agency, (Special Publication) ESA SP
Volume481
ISSN van geprinte versie0379-6566

Conference

ConferenceThe Calibration Legacy of the ISO Mission
Land/RegioSpain
Stadmadrid
Periode05/02/200109/02/2001

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