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...ata of the target source that degrade the image quality. Self-calibration (selfcal) is the process of using a model of the target source to reduce the phase a ...bration solutions we use interpolation to correct the target data, but for selfcal we apply the calibration solutions directly to the target field from which

...ata of the target source that degrade the image quality. Self-calibration (selfcal) is the process of using a model of the target source to reduce the phase a ...bration solutions we use interpolation to correct the target data, but for selfcal we apply the calibration solutions directly to the target field from which

...ata of the target source that degrade the image quality. Self-calibration (selfcal) is the process of using a model of the target source to reduce the phase a ...bration solutions we use interpolation to correct the target data, but for selfcal we apply the calibration solutions directly to the target field from which

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286, shown in black), which was also observed about a third of the way through | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|420px|left|thumb|Figure 3A: plotms view of amp vs. u

[[Image:plotms-3C286-UVDist_vs_Amp.png|200px|left|thumb|plotms view vs. uvdist of 3C 286]] ...picked by their names. We will be using the C-band EVLA standard model for 3C286 which is aptly named '3C286_C.im':

[[Image:plotms-3C286-UVDist_vs_Amp.png|200px|left|thumb|Figure 3A: plotms view vs. uvdist of 3C ...picked by their names. We will be using the C-band JVLA standard model for 3C286 which is aptly named '3C286_C.im':

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286), which was also observed about a third of the way through the scheduling b | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286), which was also observed about a third of the way through the scheduling b | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286), which was also observed about a third of the way through the scheduling b | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286), which was also observed about a third of the way through the scheduling b | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286), which was also observed about a third of the way through the scheduling b | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286, shown in black), which was also observed about a third of the way through | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286, shown in black), which was also observed about a third of the way through | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u

...tion. The next brightest is the first source observed (J1331+3030, a.k.a. 3C286, shown in black), which was also observed about a third of the way through | [[File:plotms-3C286-Amp vs UVdist 4.6.jpeg|200px|left|thumb|Figure 3A: plotms view of amp vs. u