The pros and cons of the inversion method approach to derive 3D dust emission properties in the ISM: the Hi-GAL field centred on (l, b) = (30°, 0°)
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G. Fuller | S. Molinari | M. Compiègne | R. Davies | C. Dickinson | J. Ingalls | S. Carey | P. Natoli | R. Paladini | S. Gibson | A. Noriega-Crespo | A. Traficante | M. Alves | C. Tibbs | R. Davis | L. Cambrésy | R. Davis