CLEAN results for CSDCSN+25 simulations

CLEAN results for xCSDCSN+25B7 simulations

Naming convention
-----------------
First character: 	K = (Kogan) ring type array
			C = (Conway) spiral type array
Second character:  	A, C 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)

Images CLEANed for 10,000 iterations.

Note also that the fidelity image is the ratio of (convolved model image) and (absolute value of the difference image truncated at 0.7 x rms of difference image). Importantly, in the figures below this latter rms value is different for each of the K and C array cases, resulting in the C array Fidelity image showing more structure despite (or as a consequence of) having half the rms value for its difference image.

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...} \par\parbox[t]{578pt}{~~~~~~a) contour plots of CLEAN image.} \par\end{figure}$

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...par\parbox[t]{578pt}{~~~~~~b) grey scale plots of CLEAN image.} \par\end{figure}$

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...r\parbox[t]{578pt}{~~~~~~c) contour plots of difference image.} \par\end{figure}$

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...arbox[t]{578pt}{~~~~~~d) grey scale plots of difference image.} \par\end{figure}$

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...8pt}{~~~~~~e) histograms of pixel values for difference image.} \par\end{figure}$

f) Listing of max, min, mean and rms for difference images

Image= KCSDCSN+25B7.DIFF . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean=-2.5247E-02 Rms= 4.5944E-02 JY/BEAM over 66049. pixels Minimum=-1.0602E+00 at 135 171 1 1 Maximum= 7.9254E-01 at 135 168 1 1

Image= CCSDCSN+25B7.DIFF . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean=-6.9361E-03 Rms= 4.1725E-02 JY/BEAM over 66049. pixels Minimum=-1.0203E+00 at 135 171 1 1 Maximum= 1.2256E+00 at 135 168 1 1

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...ar\parbox[t]{578pt}{~~~~~~g) contour plots of Fidelity images.} \par\end{figure}$

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KCSDCSN+25B7... ...parbox[t]{578pt}{~~~~~~h) grey scale plots of Fidelity images.} \par\end{figure}$

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KandCCSDCSN+... ...n bins with 0 pixels and 1 pixel\\ in the graph on the left.} \par\end{figure}$

j) Listing of max, min, mean and rms for fidelity images

Image= KCSDCSN+25B7.FID . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean= 4.9383E+00 Rms= 1.9461E+01 RATIO over 66049. pixels Minimum=-6.6946E-06 at 5 164 1 Maximum= 1.0103E+03 at 136 166 1

Image= CCSDCSN+25B7.FID . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean= 6.5388E+00 Rms= 2.2396E+01 RATIO over 66049. pixels Minimum=-7.3714E-06 at 5 164 1 Maximum= 1.0053E+03 at 131 167 1

$\begin{figure} \par\vspace{3.6in} \special{psfile=/wine/alma/myarea/KandCCSDCSN+... ...s is the\\ arithmetic mean of the intensity range of the bin. \par\end{figure}$

2001-02-15