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	Comments on: Tulip Nebula Wide Field	</title>
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		<title>
		By: Ron Brecher		</title>
		<link>https://astrodoc.ca/tulip-nebula/#comment-9138</link>

		<dc:creator><![CDATA[Ron Brecher]]></dc:creator>
		<pubDate>Tue, 14 Aug 2018 19:20:27 +0000</pubDate>
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					<description><![CDATA[In reply to &lt;a href=&quot;https://astrodoc.ca/tulip-nebula/#comment-9021&quot;&gt;Steve&lt;/a&gt;.

I use the channel masters, not the individual files.]]></description>
			<content:encoded><![CDATA[<p>In reply to <a href="https://astrodoc.ca/tulip-nebula/#comment-9021">Steve</a>.</p>
<p>I use the channel masters, not the individual files.</p>
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		<title>
		By: Steve		</title>
		<link>https://astrodoc.ca/tulip-nebula/#comment-9021</link>

		<dc:creator><![CDATA[Steve]]></dc:creator>
		<pubDate>Fri, 20 Jul 2018 02:27:32 +0000</pubDate>
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					<description><![CDATA[Ron, When you are creating the SynthL channel data from the RGB are you using the individual subframe or the Master R G B?  I am guessing you are going back to the subs since they are noise weighted.  I have some nice Ha R G B data of the Cat&#039;s Paw and wondering how best to integrate the data.  Steve]]></description>
			<content:encoded><![CDATA[<p>Ron, When you are creating the SynthL channel data from the RGB are you using the individual subframe or the Master R G B?  I am guessing you are going back to the subs since they are noise weighted.  I have some nice Ha R G B data of the Cat&#8217;s Paw and wondering how best to integrate the data.  Steve</p>
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