Clegg, P. E., Ade, Peter A. R., Armand, C., Baluteau, J. P., Barlow, M. J., Buckley, M. A., Berges, J. C., Burgdorf, M., Caux, E., Ceccarelli, C., Cerulli, R., Church, S. E., Cotin, F., Cox, P., Cruvellier, P., Culhane, J. L., Davis, G. R., di Giorgio, A., Diplock, B. R., Drummond, D. L., Emery, R. J., Ewart, J. D., Fischer, J., Furniss, I., Glencross, W. M., Greenhouse, M. A., Griffin, Matthew J., Gry, C., Harwood, A. S., Hazell, A. S., Joubert, M., King, K. J., Lim, T., Liseau, R., Long, J. A., Lorenzetti, D., Molinari, S., Murray, A. G., Naylor, D. A., Nisini, B., Norman, K., Omont, A., Orfei, R., Patrick, T. J., Pequignot, D., Pouliquen, D., Price, M. C., Nguyen, Q. Rieu, Rogers, A. J., Robinson, F. D., Saisse, M., Saraceno, P., Serra, G., Sidher, S. D., Smith, A. F., Smith, H. A., Spinoglio, L., Swinyard, B. M., Texier, D., Towlson, W. A., Trams, N. R., Unger, S. J. and White, G. J. 1996. The ISO Long-Wavelength Spectrometer. Astronomy and Astrophysics 315 , pp. 38-42. |
Abstract
The Long-Wavelength Spectrometer (LWS) is one of two complementary spectrometers aboard the European Space Agency's Infrared Space Observatory (ISO) (Kessler et al., 1996A&A...315L..49D). It operates over the wavelength range 43-196.9μm at either medium (about 150 to 200) or high (6800 to 9700) spectral resolving power. This Letter describes the instrument and its modes of operation; a companion paper (Swinyard et al, 1996) describes its performance and calibration.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy Neuroscience and Mental Health Research Institute (NMHRI) |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | artificial satellites, space probes, instrumentation: spectrographs, infrared: general |
Additional Information: | http://adsabs.harvard.edu/abs/1996A%26A...315L..38C |
Publisher: | EDP Sciences |
ISSN: | 0004-6361 |
Last Modified: | 10 Jan 2018 14:48 |
URI: | http://orca.cf.ac.uk/id/eprint/75944 |
Citation Data
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