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Wikipedia:Featured picture candidates/delist/Keplers supernova.jpg

In this article, the topic of Wikipedia:Featured picture candidates/delist/Keplers supernova.jpg will be addressed from different perspectives, with the purpose of exploring its implications, applications and relevance today. Its historical context, its possible impacts in various areas and its relevance in the current panorama will be analyzed in detail. Likewise, its possible future implications will be delved into and various points of view on Wikipedia:Featured picture candidates/delist/Keplers supernova.jpg will be discussed. Through a journey through different approaches and opinions, the aim is to provide the reader with a comprehensive and detailed vision of this topic, with the aim of encouraging debate and reflection.
Keplers supernova.jpg
Reason
Originally nom'ed in 2004 (then, weirdly, renom'ed in 2006). Low quality for what we expect out of NASA these days, and considerably under the 1000px×1000 size requirement. Suggest delisting of this image.
Previous nomination/s
Wikipedia:Featured pictures candidates/October-2004#Kepler.27s Supernova (2004) and then Wikipedia:Featured picture candidates/Supernova (2006)
Nominator
ωαdεstεr16♣TC♣

STOP THE PRESSES - I've uploaded a higher-res version over it. It should be more-or-less identical otherwise, save maybe a slightly different crop of the black space around it. It shows some graininess from some of the instruments used to investigate it (also visible in the old one), but I think it's fine, and well over size requirements now. (In other words, keep) Shoemaker's Holiday (talk) 17:05, 10 March 2009 (UTC)

Thanks for the replacement image! Very cool astrophoto. Best, Pete Tillman (talk) 17:45, 10 March 2009 (UTC)

Unfortunately the replacement is one of the images I commented about earlier on. The funkiness in the red channel strongly suggests it is upsampled. Comments? MER-C 03:34, 15 March 2009 (UTC)

My presumption - perhaps wrong - is that this is because the composite mixes several images from different sources, and, for whatever reason, the Spitzer Space telescope's image was lower resolution compared to the others. Shoemaker's Holiday (talk) 04:23, 15 March 2009 (UTC)
A back of the envelope calculation based on telescope diameter and wavelength gives angular resolution as follows: red: 730 - 4400 milliarcseconds, yellow: 3 - 60 milliarcseconds, green ~0.3 milliarcseconds and blue: ~0.01 milliarcseconds. These probably aren't the real resolutions of the scopes. MER-C 05:51, 15 March 2009 (UTC)
Then I honestly don't know, ut the graininess is isible in all versions of this image I can find - look at the upper left of te 700px version and it's clearly visible. Maybe the person who assembled the images messed up. Shoemaker's Holiday (talk) 13:08, 15 March 2009 (UTC)
I've since found out that this image has a FOV of 300 arcseconds and (from an above nom) Chandra has a resolution of 0.5 arcseconds (this image represents the limit of the scope) and the various Spitzer resolutions are here. The reds are definitely upsampled by a factor of at least 4.5. MER-C 11:21, 25 March 2009 (UTC)
Well, if that's the limit of the ability of this to be photographed at this time, and the better resolution of the other things justifies upscaling that in a composite, I think it's best to just accept this as the best currently possible image of this remnant at these wavelengths. Shoemaker's Holiday (talk) 12:44, 25 March 2009 (UTC)

Delisted MER-C 08:22, 5 May 2009 (UTC)