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    <title>topic Re: Good introduction to serious astrophotography in General Discussion</title>
    <link>https://community.usa.canon.com/t5/General-Discussion/Good-introduction-to-serious-astrophotography/m-p/268367#M18781</link>
    <description>&lt;P&gt;Keep in mind the title is "getting started" ... there's quite a bit not included in this article.&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;Part of the challenge of astrophotography is "image data acquisition" ... and part of the problem is "image integration and processing". &amp;nbsp;&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;The author didn't mention a lot of the special types of exposures that are gathered (lights, darks, bias, &amp;amp; flats) as well as the image processing steps involved (special software that deals with image calibration, registration &amp;amp; integration ... this is fairly unique to astrophotography). &amp;nbsp;Ultimately you get a combined "master" integrated image ... but that's just the starting point for the rest of the image processing &amp;amp; adjustment steps.&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;The cameras tend to be specially modified for astrophotography. &amp;nbsp;You can use a normal camera, but the sensitivity will be weaker and the amount of exposure time will be increased. &amp;nbsp;The Canon 60Da (the "a" suffix is for "astrophotography) was pre-modded by Canon to remove the normal filter and replace it with a more permission filter. &amp;nbsp;Normal cameras are filtered so that the light collected will match the sensitivity of the human eye. &amp;nbsp;But human eyes aren't equally sensitive to all wavelengths across the visible spectrum. We are not especially sensitive to the "reds". &amp;nbsp;90% of the normal matter in the universe is Hydrogen. &amp;nbsp;The dominant emission wavelength for Hydrogen is mostly the Hydrogen alpha wavelength (656nm). &amp;nbsp;Human eyes are only about 20-25% sensitive to this. &amp;nbsp;Normal cameras gradually ramp up the blocking starting at around 550nm and increase it block 100% by the time they get to 700nm (the end of the visible spectrum on the IR end). &amp;nbsp;At 656nm, a normal camera blocks around 75-80% of the light. &amp;nbsp;But this means you have to run much longer exposures to collect this light. &amp;nbsp;Modded astrophotography cameras replace the factory filter with a much more permissive filter. &amp;nbsp;&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;</description>
    <pubDate>Tue, 26 Feb 2019 02:10:46 GMT</pubDate>
    <dc:creator>TCampbell</dc:creator>
    <dc:date>2019-02-26T02:10:46Z</dc:date>
    <item>
      <title>Good introduction to serious astrophotography</title>
      <link>https://community.usa.canon.com/t5/General-Discussion/Good-introduction-to-serious-astrophotography/m-p/268346#M18780</link>
      <description>&lt;P&gt;From lens rentals:&lt;/P&gt;&lt;P&gt;&lt;A href="https://www.lensrentals.com/blog/2019/02/getting-started-in-deep-space-and-astrophotography/" target="_self"&gt;https://www.lensrentals.com/blog/2019/02/getting-started-in-deep-space-and-astrophotography/&lt;/A&gt;&lt;/P&gt;</description>
      <pubDate>Mon, 25 Feb 2019 15:19:29 GMT</pubDate>
      <guid>https://community.usa.canon.com/t5/General-Discussion/Good-introduction-to-serious-astrophotography/m-p/268346#M18780</guid>
      <dc:creator>kvbarkley</dc:creator>
      <dc:date>2019-02-25T15:19:29Z</dc:date>
    </item>
    <item>
      <title>Re: Good introduction to serious astrophotography</title>
      <link>https://community.usa.canon.com/t5/General-Discussion/Good-introduction-to-serious-astrophotography/m-p/268367#M18781</link>
      <description>&lt;P&gt;Keep in mind the title is "getting started" ... there's quite a bit not included in this article.&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;Part of the challenge of astrophotography is "image data acquisition" ... and part of the problem is "image integration and processing". &amp;nbsp;&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;The author didn't mention a lot of the special types of exposures that are gathered (lights, darks, bias, &amp;amp; flats) as well as the image processing steps involved (special software that deals with image calibration, registration &amp;amp; integration ... this is fairly unique to astrophotography). &amp;nbsp;Ultimately you get a combined "master" integrated image ... but that's just the starting point for the rest of the image processing &amp;amp; adjustment steps.&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;The cameras tend to be specially modified for astrophotography. &amp;nbsp;You can use a normal camera, but the sensitivity will be weaker and the amount of exposure time will be increased. &amp;nbsp;The Canon 60Da (the "a" suffix is for "astrophotography) was pre-modded by Canon to remove the normal filter and replace it with a more permission filter. &amp;nbsp;Normal cameras are filtered so that the light collected will match the sensitivity of the human eye. &amp;nbsp;But human eyes aren't equally sensitive to all wavelengths across the visible spectrum. We are not especially sensitive to the "reds". &amp;nbsp;90% of the normal matter in the universe is Hydrogen. &amp;nbsp;The dominant emission wavelength for Hydrogen is mostly the Hydrogen alpha wavelength (656nm). &amp;nbsp;Human eyes are only about 20-25% sensitive to this. &amp;nbsp;Normal cameras gradually ramp up the blocking starting at around 550nm and increase it block 100% by the time they get to 700nm (the end of the visible spectrum on the IR end). &amp;nbsp;At 656nm, a normal camera blocks around 75-80% of the light. &amp;nbsp;But this means you have to run much longer exposures to collect this light. &amp;nbsp;Modded astrophotography cameras replace the factory filter with a much more permissive filter. &amp;nbsp;&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;&lt;P&gt;&amp;nbsp;&lt;/P&gt;</description>
      <pubDate>Tue, 26 Feb 2019 02:10:46 GMT</pubDate>
      <guid>https://community.usa.canon.com/t5/General-Discussion/Good-introduction-to-serious-astrophotography/m-p/268367#M18781</guid>
      <dc:creator>TCampbell</dc:creator>
      <dc:date>2019-02-26T02:10:46Z</dc:date>
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