Powerful model for the point source sky: Far-ultraviolet and enhanced midinfrared performance

作者: M. Cohen

DOI: 10.1086/116878

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摘要: I report further developments of the Wainscoat et al. (1992) model originally created for point source infrared sky. The already detailed and realistic representation Galaxy (disk, spiral arms local spur, molecular ring, bulge, spheroid) has been improved, guided by CO surveys clouds, inclusion a component to represent Gould's Belt. newest version is very well validated Infrared Astronomy Satellite (IRAS) counts. A major new aspect extension same down far ultraviolet. compare predicted observed far-utraviolet counts from Apollo 16 'S201' experiment (1400 A) TD1 satellite (for 1565 band).

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