
| Comparison of reconstruction methods for IRAS survey scans of the interacting galaxy pair, M51, The "Whirlpool Galaxy". Shown are reconstructions using the Pixon method, the Lucy-Richardson method, the IPAC Maximum Correlation Method (MCM), and MEM (MEMSYS 3). Panel (b) from Bontekoe et al. (1991, Astron & Astrophys, 248, 328), and panels (c) and (d) from Rice (1993, AJ, 105, 67). This figure first appeared in Puetter and Pina (1994, in "Science with high Spatial Resolution Far-Infrared Data", Pasadena: Jet Propulsion Laboratory, 95-4, 61) |