Abstract
The ISO Long Wavelength Spectrometer (LWS) parallel mode allowed LWS data to be taken at all times when the LWS was not the prime ISO insrument. Although the data is of a lower quality than that of the prime mode, large regions of the sky have been probed with 10 narrow band photometry points between 46 and 178μm. Detailed below is a description of the current state of the processing, interactive analysis and calibration with estimates of the accuracies obtainable.
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Lim, T., Vivares, F., Caux, E. (2000). The ISO LWS Parallel Mode. In: Lemke, D., Stickel, M., Wilke, K. (eds) ISO Surveys of a Dusty Universe. Lecture Notes in Physics, vol 548. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-45553-1_37
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DOI: https://doi.org/10.1007/3-540-45553-1_37
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