CLEAN results for CCYGSN+25 simulations

CLEAN results for xCCYGSN+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.

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

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

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

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

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

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

Image= KCCYGSN+25B7.DIFF . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean=-1.4235E-02 Rms= 4.4322E-02 JY/BEAM over 66049. pixels Minimum=-1.2283E+00 at 14 84 1 1 Maximum= 1.2164E+00 at 14 81 1 1

Image= CCCYGSN+25B7.DIFF . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean=-9.1407E-03 Rms= 5.4464E-02 JY/BEAM over 66049. pixels Minimum=-1.1027E+00 at 14 78 1 1 Maximum= 1.5468E+00 at 14 81 1 1

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

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

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

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

Image= KCCYGSN+25B7.FID . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean= 4.8392E+00 Rms= 1.9226E+01 RATIO over 66049. pixels Minimum=-2.8729E-06 at 6 38 1 1 Maximum= 1.0497E+03 at 15 79 1 1

Image= CCCYGSN+25B7.FID . 1 5 xywind= 1 1 257 257 Mean and rms found by including all data: Mean= 3.7391E+00 Rms= 1.5197E+01 RATIO over 66049. pixels Minimum=-2.3379E-06 at 6 38 1 1 Maximum= 7.4110E+02 at 243 173 1 1

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

2001-02-15