<?xml version="1.0" encoding="UTF-8"?><rss xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:content="http://purl.org/rss/1.0/modules/content/" xmlns:atom="http://www.w3.org/2005/Atom" version="2.0"><channel><title><![CDATA[This is my attempt at processing James Webb Space Telescope (JWST) data of Sh 2-305.]]></title><description><![CDATA[This is my attempt at processing James Webb Space Telescope (JWST) data of Sh 2-305. It is an emission nebula usually visible in red (H II emission), but it is displayed here in false-color infrared. Blue areas emit higher-energy photons than red regions. This area is a stellar nursery where gas and dust remnants from supernovae or collisions form new stars. The three versions show the nebula only, with galaxies only, and with everything else.<br />
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A great deal of work went into creating a clean nebula image with as few artifacts as possible. After data extraction and initial stretching with <a href="https://pixelfed.de/discover/tags/Siril?src=hash" rel="external nofollow noopener">#Siril</a>, the single monochrome filter images were combined, processed, and cropped in <a href="https://pixelfed.de/discover/tags/GIMP?src=hash" rel="external nofollow noopener">#GIMP</a>. The combined image was then run through <a href="https://pixelfed.de/discover/tags/StarNet?src=hash" rel="external nofollow noopener">#StarNet</a>++ to remove most of the stars. Since StarNet++ does not work well with JWST data, it leaves artifacts for every star, especially the brighter ones, whose long spikes typical of JWST overlay large parts of the image. I therefore had to remove each star artifact manually using the clone and healing tools in GIMP. This took tens of hours to complete. <a href="https://pixelfed.de/discover/tags/GMIC?src=hash" rel="external nofollow noopener">#GMIC</a> additionally helped reduce banding. As such, this is an artistic interpretation by me and is not scientifically accurate. The full resolution versions can be downloaded from <a href="https://www.picturavis.com/index?/tags/1204-jwst" rel="external nofollow noopener">https://www.picturavis.com/index?/tags/1204-jwst</a> (these JWST images are crazily detailed).<br />
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The person responsible for this JWST proposal is Mark McCaughrean of the Max-Planck-Institut für Astronomie in Heidelberg. He also shared an initial version of the uncropped processed image: <a href="https://www.flickr.com/photos/markmccaughrean/55209728128/" rel="external nofollow noopener">https://www.flickr.com/photos/markmccaughrean/55209728128/</a><br />
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Attribution: NASA/ESA/CSA<br />
Telescope: JWST/NIRCam<br />
Proposal ID: 4547<br />
Observation description: The stellar &amp; sub-stellar initial mass function in Sharpless 305: imaging<br />
Release date: 02.04.2026<br />
Filters (mapping): F140M (blue), F150W+162M (light blue), F182M (blue-green), F212N (green), F300M (light green), F335M (yellow), F360M (orange), F444W (red)<br />
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<a href="https://pixelfed.de/discover/tags/Sharpless305?src=hash" rel="external nofollow noopener">#Sharpless305</a> <a href="https://pixelfed.de/discover/tags/Sh2305?src=hash" rel="external nofollow noopener">#Sh2305</a> <a href="https://pixelfed.de/discover/tags/JWST?src=hash" rel="external nofollow noopener">#JWST</a> <a href="https://pixelfed.de/discover/tags/JamesWebb?src=hash" rel="external nofollow noopener">#JamesWebb</a> <a href="https://pixelfed.de/discover/tags/NIRCam?src=hash" rel="external nofollow noopener">#NIRCam</a> <a href="https://pixelfed.de/discover/tags/Nebula?src=hash" rel="external nofollow noopener">#Nebula</a> <a href="https://pixelfed.de/discover/tags/SpaceTelescope?src=hash" rel="external nofollow noopener">#SpaceTelescope</a> <a href="https://pixelfed.de/discover/tags/astrophotography?src=hash" rel="external nofollow noopener">#astrophotography</a> <a href="https://pixelfed.de/discover/tags/DeepSky?src=hash" rel="external nofollow noopener">#DeepSky</a> <a href="https://pixelfed.de/discover/tags/DigiKam?src=hash" rel="external nofollow noopener">#DigiKam</a>

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