Publication Details
| Title | 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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| Author(s) | Traficante, A. and Paladini, R. and Compiegne, M. and Alves, M. I. R. and Cambrésy, L. and Gibson, S. J. and Tibbs, C. T. and Noriega-Crespo, A. and Molinari, S. and Carey, S. J. and Ingalls, J. G. and Natoli, P. and Davies, R. D. and Davis, R. J. and Dickinson, C. and Fuller, G. A. |
| Journal | MNRAS , 2014, 440, 3588-3612 |
| ADS | 2014MNRAS.440.3588T |
| DOI | 10.1093/mnras/stu493 |
Data Sets Used
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from among: COSMOS, BLAST, BOLOCAM, IRTS, MSX, SWAS, BRAVA,
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A best-effort attempt was made to match publications with data sets actually used given available resources. It is possible that in some cases data sets were missed or the publication's use of the data set was indirect or incidental.
A best-effort attempt was made to match publications with data sets actually used given available resources. It is possible that in some cases data sets were missed or the publication's use of the data set was indirect or incidental.