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Calibration and performance of the ISO Long-Wavelength Spectrometer

Swinyard, B. M., Clegg, P. E., Ade, Peter A. R., Armand, C., Baluteau, J. P., Barlow, M. J., Berges, J. C., Burgdorf, M., Caux, E., Ceccarelli, C., Cerulli, R., Church, S. E., Colgan, S., Cotin, F., Cox, P., Cruvellier, P., Davis, G. R., Digiorgio, A., Emery, R. J., Ewart, D., Fischer, J., Furniss, I., Glencross, W. M., Greenhouse, M., Griffin, Matthew J., Gry, M. R., Haas, C., Joubert, M., King, K. J., Lim, T., Liseau, R., Lord, S., Lorenzetti, D., Molinari, S., Naylor, D. A., Nisini, B., Omont, A., Orfei, R., Patrick, T., Pequignot, D., Pouliquen, D., Price, M. C., Nguyen, Q. Rieu, Robinson, F. D., Saisse, M., Saraceno, P., Serra,, G., Sidher, S. D., Smith, H. A., Spinoglio, L., Texier, D., Towlson, W. A., Trams, N., Unger, S. J. and White, G. J. 1996. Calibration and performance of the ISO Long-Wavelength Spectrometer. Astronomy and Astrophysics 315 , pp. 43-48.

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Abstract

The wavelength and flux calibration, and the in-orbit performance of the Infrared Space Observatory Long-Wavelength Spectrometer (LWS) are described. The LWS calibration is mostly complete and the instrument's performance in orbit is largely as expected before launch. The effects of ionising radiation on the detectors, and the techniques used to minimise them are outlined. The overall sensitivity figures achieved in practice are summarised. The standard processing of LWS data is described.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Uncontrolled Keywords: artificial satellites, instrumentation: spectrographs, infrared: general
Publisher: EDP Sciences
ISSN: 0004-6361
Last Modified: 10 Jan 2018 14:46
URI: http://orca.cf.ac.uk/id/eprint/75889

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