![\begin{figure}
\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7.UV....
...offset=0 hscale=38
vscale=38}
\par\parbox[t]{578pt}{a) uv coverage}
\end{figure}](img1.gif)
(Results identical for simulations using other test images)
Naming convention ----------------- First character: K = (Kogan) ring type array C = (Conway) spiral type array Second character: A, B, C, D or E, denoting resolution of array Characters 3-5: Member of SIL- M51, CYG, MAR, SDC or MPD Characters 6 and 7: SN (snapshot) or track, e.g. _4 for 4hr track Characters 8-10: signed declination Characters 11 and 12: Wavelength, e.g. _1 or _3 for 1 and 3mm respectively or b7 corresponding to ALMA band 7 frequency (345GHz)
K array shown on left, C array shown on right for comparison
![\begin{figure}
\par\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7...
...ox[t]{578pt}{b) distribution of baselines\\ (Note axes may differ)}
\end{figure}](img2.gif)
![\begin{figure}
\par\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7...
...parbox[t]{578pt}{d) grey scale plot of dirty beam (-3\% to +10\%) }
\end{figure}](img4.gif)
![\begin{figure}
\par\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7...
...38}
\par\parbox[t]{578pt}{e) slice through dirty beam at 0 degrees}
\end{figure}](img5.gif)
![\begin{figure}
\par\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7...
...8}
\par parbox[t]{578pt}{f) slice through dirty beam at 45 degrees}
\end{figure}](img6.gif)
![\begin{figure}
\par\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7...
...8}
\par\parbox[t]{578pt}{g) slice through dirty beam at 90 degrees}
\end{figure}](img7.gif)
![\begin{figure}
\par\vspace{3.6in}
\special{psfile=/wine/alma/myarea/KCM51SN-70b7...
...}
\par\parbox[t]{578pt}{h) slice through dirty beam at 135 degrees}
\end{figure}](img8.gif)