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As discussed, we need to image a facet with a user defined model (but where no DDE selfcal is used). For example to deal with 3C295 in the field center (for which we already have a good model and no D…
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This is not related in specific to the reimage branch but a more general problem. It seems that the solutions it finds during peeling are wrong for some reason (I noticed it before but thought my 3C29…
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Hello,
I have a 2048 X 30000 science image. The image contains few saturated objects (one of them is shown in the link below).
![ds9](https://cloud.githubusercontent.com/assets/16637195/12223363/5bdc…
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Is there a lens galaxy or the smoothed profile of the dark matter that creates the arcs?
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@linan7788626, Scott Daniel and @drphilmarshall are going to try and PhoSim a 10 arcsec sky patch containing a massive elliptical galaxy in front of two distant galaxies at different redshifts, to mak…
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I noticed clear aliasing in the facet images (and final mosaic), see examples.
There are at least a few dozen(!) of these in the mosaic. Note that I used the latest WSClean v1.11. I think we need to i…
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```
Change median sky check to a lower percentile.
```
Original issue reported on code.google.com by `robbarns...@gmail.com` on 15 Mar 2013 at 11:35
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Is it reasonable to add the best-fit synthetic template as a fits extension, in addition to its ccf? This would be useful information in early days, but I'm not sure it would continue to be.
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work with Tommaso and Xiao-Lei
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Dear colleagues
I have a first version of the long2pos reduction. I managed to finish a reduction and the reduced spectrum is attached. The code lives in a special and separate branch called Longslit…