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	<title>Specials Archives - Modern Astronomy</title>
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	<description>Visual and Electronic Astronomy...</description>
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		<title>TeleVue Paracorr Type 2</title>
		<link>https://modernastronomy.com/shop/accessories/focal-reducers-correctors/televue-paracorr-type-2/</link>
					<comments>https://modernastronomy.com/shop/accessories/focal-reducers-correctors/televue-paracorr-type-2/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Mon, 18 Mar 2024 20:04:26 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=94483</guid>

					<description><![CDATA[<p>TeleVue Paracorr Type 2 is a universal corrector that tightens and intensifies stars on all F ratios down to f/3, without adding any colour or aberration!<br />
Price includes delivery!</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/focal-reducers-correctors/televue-paracorr-type-2/">TeleVue Paracorr Type 2</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<p><strong>TeleVue Paracorr Type 2</strong></p>
<div class="img_break">An optical chain is only as good as its weakest link. With the development of 82 degree Nagler and 100+ degree Ethos eyepieces, Tele Vue offers the largest, flattest and best corrected visual fields in the industry. Combine the Nagler/Ethos revolution, Dobsonian revolution and Paracorr for the ideal mating for spectacular wide and sharp &#8220;spacewalk&#8221; observing.</div>
<div></div>
<div>
<div class="pageSectionTitle"><strong>Life without the TeleVue Paracorr Type 2</strong></div>
<p>Coma makes stars look like blurry comets whose tails point out radially from the center of the field. The faster your scope&#8217;s speed, the worse the effect. All parabolic mirrors used in Newtonian reflecting telescopes are limited in field sharpness due to coma. Even a perfectly made 13&#8243; f/4.5 parabola has only about 0.1 degree diffraction limited field.</p>
<p>Previous attempts to correct for coma have been limited in usefulness. Some correctors were designed mainly for astrophotography, some required difficult installation in the focuser&#8217;s draw tube. Dedicated coma correcting eyepieces were another approach. However, these were limited to 50 degree apparent fields and would orphan your existing eyepiece collection.</p>
<div class="pageSectionTitle"><strong>Life with the TeleVue Paracorr Type 2</strong></div>
<p>Paracorr is a universal corrector that tightens and intensifies star images on all f-ratios down to f/3! (see spot size graphs: <a href="https://www.televue.com/pdf/Paracorr_T2_spotsizes.pdf" target="_blank" rel="noopener">PDF</a> or <a href="https://www.televue.com/images/TV3_Images/Images_in_articles/Paracorr_2_chart.jpg" target="_blank" rel="noopener">JPG</a>) without adding any false color or spherical aberration! You no longer have to constantly shift a Dobsonian to keep objects centered for sharp viewing. Using a Tele Vue eyepiece, put M-13 at the edge of the field and enjoy fully resolving its beauty as it drifts across your view.</p>
<p>Paracorr is easy to use. It slips into your focuser, just like a Barlow. To minimize focuser in-travel, due to additional length, a mild 15% Barlow effect was designed into Paracorr to effectively push the focus out. Paracorr is recommended for use with all Tele Vue eyepieces because our Plössls, Delites, Panoptics, Naglers, Ethos and Delos eyepieces achieve higher levels of aberration correction than competitive models. However, Paracorr is also compatible with other eyepiece makes.</p>
<p>Try Paracorr on your &#8220;DobNewt.&#8221; We think you&#8217;ll agree that the revolution is complete.</p>
<div class="pageSectionTitle"><strong>Paracorr Eats Coma</strong></div>
<p>Paracorr can be used with both 2&#8243; and 1¼&#8221; eyepieces. For visual use, slip Paracorr Type-2 into your focuser like a Barlow lens, and your eyepiece into Paracorr. 1¼&#8221; eyepieces will make use of Paracorr&#8217;s special low profile 1¼&#8221; reducing adapter. Paracorr is threaded for 2&#8243; filters.</p>
<div class="pageSectionTitle"><strong>SIPS</strong></div>
<p>Note: The Paracorr Type 2 optical assembly is also available in a special adapter housing made by Starlight Instruments for their Feather Touch focusers. This unit avoids the need for a tunable top to optimize eyepiece position. Some Dobsonian manufacturers may also offer the Feather Touch focuser with integrated Paracorr type 2 as standard. <a href="https://www.starlightinstruments.com/?s=paracorr" target="_blank" rel="noopener">Starlight Instruments</a> offers Paracorr Type 2 integrated with Feather Touch focuser or as an add-on if you already have a Feather Touch focuser.</p>
<div class="pageSectionTitle"><strong>Astrophotography</strong></div>
<p>Paracorr also works with DSLR and CCD cameras. Just unscrew the lens assembly from the Tunable Top and attach appropriate threaded accessory tubes and camera mounts. See <a href="https://www.televue.com/engine/TV3b_page.asp?id=61&amp;Tab=_phot">2&#8243; Imaging</a> (Paracorr Type-2), <a href="https://www.televue.com/engine/TV3b_page.asp?id=61&amp;Tab=_phot3">3&#8243; Imaging</a> (3&#8243; BIG Paracorr Type-2), and <a href="https://www.televue.com/engine/TV3b_page.asp?id=61&amp;Tab=_back">&#8220;is&#8221; adapter for 3&#8243;</a> (3&#8243; BIG Paracorr Type-2) sections for more on Paracorr imaging.</p>
<div class="pageSectionTitle">
<p><strong>History and How to Choose</strong></p>
</div>
<div>Tele Vue&#8217;s two-part blog post on the Paracorr Type-2 is a must-read for any Dobsonian / Newtonian user!</div>
<ul>
<li>In <a href="https://televue.com/televueopticstalk/2021/06/25/paracorr-newtonian-for-visual-and-imaging-to-f-3-part-1/">Part 1</a> they cover the history of the Newtonian reflector, its inherent aberrations, and how Tele Vue&#8217;s Paracorr enlarged the &#8220;sweet spot&#8221; of fast Newtonian / Dobsonians to cover the entire field. We also pitted the Paracorr — Newtonian combination against more &#8220;exotic&#8221; telescope designs for imaging.</li>
<li>The <a href="https://televue.com/televueopticstalk/2021/07/12/paracorr-newtonian-for-visual-and-imaging-to-f-3-part-2/">Part 2</a> post answers the follow-up question: Which Paracorr to Use? We focus on the three currently available versions of the Type-2 Paracorr: 2&#8243; Photo/Visual, 2&#8243; Starlight Instruments SIPS, and 3&#8243; Paracorr Type-2 for imaging. They all have their own strengths. This post also has links to many sources to help you decide what Paracorr is best for your usage.</li>
</ul>
</div>
<p>The post <a href="https://modernastronomy.com/shop/accessories/focal-reducers-correctors/televue-paracorr-type-2/">TeleVue Paracorr Type 2</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<item>
		<title>StarSense Autoalign for SkyWatcher Mounts</title>
		<link>https://modernastronomy.com/shop/accessories/mount-accessories/starsense-autoalign-for-skywatcher-mounts/</link>
					<comments>https://modernastronomy.com/shop/accessories/mount-accessories/starsense-autoalign-for-skywatcher-mounts/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Tue, 12 Mar 2024 18:26:05 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=94462</guid>

					<description><![CDATA[<p>The Celestron StarSense Autoalign for SkyWatcher Mounts can be used on Celestron and SkyWatcher mounts, to automatically align your telescope so you can begin observing in minutes!<br />
Price includes delivery!</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/mount-accessories/starsense-autoalign-for-skywatcher-mounts/">StarSense Autoalign for SkyWatcher Mounts</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<h3>StarSense Autoalign for SkyWatcher Mounts</h3>
<p>The StarSense AutoAlign for SkyWatcher Mounts also works with Celestron goto systems, StarSense technology was developed by Celestron’s engineers, allowing a Celestron computerized telescope to automatically align itself with the night sky. It’s never been easier to locate celestial objects. Now, this technology can be connected to a computerized SkyWatcher synscan mount with the included Interface Box, further expanding the number of scopes that can take advantage of StarSense’s revolutionary auto alignment!</p>
<p><strong>Please note StarSense Autoalign for SkyWatcher Mounts</strong> works with Celestron <strong>and</strong> SkyWatcher Goto telescopes and mounts, the interface box is included for use on SkyWatcher models and is not used on Celestron models.</p>
<p><strong>Automatically align a Celestron or SkyWatcher mount with StarSense</strong><br />
No need to identify or locate any star in the sky StarSense will automatically align your telescope, so you can begin observing in minutes. Plug and play compatibility</p>
<p><strong>Celestron Compatability</strong><br />
NexStar SE Series<br />
CPC, CPC DX<br />
NexStar GT (with Aux. splitter)<br />
CGE Pro<br />
Advanced VX<br />
CG-5 (with Aux. splitter)<br />
CGEM, CGEM DX, CGEMII<br />
CGE<br />
CGX, CGX-L<br />
NexStar SLT<br />
NexStar Evolution<br />
LCM (with Aux. splitter)</p>
<p><strong>SkyWatcher Compatability</strong><br />
HEQ5<br />
EQ6 / EQ6R<br />
AZ-EQ5<br />
AZ-EQ6<br />
CQ350<br />
EQ8<br />
AZ SynScan compatible mounts</p>
<p><strong>Included Items </strong><br />
StarSense Hand Control<br />
StarSense Camera with large and small mounting brackets<br />
Cable, camera to mount<br />
Interface Box (for SkyWatcher)</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/mount-accessories/starsense-autoalign-for-skywatcher-mounts/">StarSense Autoalign for SkyWatcher Mounts</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<item>
		<title>QHY533M CMOS Camera</title>
		<link>https://modernastronomy.com/shop/cameras/astro-video/qhy/qhy533m-cmos-camera/</link>
					<comments>https://modernastronomy.com/shop/cameras/astro-video/qhy/qhy533m-cmos-camera/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Sat, 06 Aug 2022 09:44:29 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=93370</guid>

					<description><![CDATA[<p><span class="ql-author-8876147">The QHY533M CMOS camera is part of a new generation of back-illuminated CMOS cameras with 3.76um pixels featuring low noise and improved full well capacity. Price includes delivery.<br />
</span></p>
<p>Perfect for Deep Sky <a href="https://astrobiscuit.com/lucky-imaging-theory/">"Lucky Imaging"</a> - <a href="https://www.youtube.com/watch?v=5s9xbZ5G-wk">BAT project on M82</a></p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/astro-video/qhy/qhy533m-cmos-camera/">QHY533M CMOS Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<h1>QHY533M CMOS Camera</h1>
<div class="block lv1 on">
<h3 id="a1" class="tit">Overview</h3>
<p>With the advantage of low readout noise and high-speed readout, CMOS technology has revolutionized astronomical imaging.  The QHY533M CMOS Camera is part of a new generation of back-illuminated CMOS cameras with 3.76um pixels.  <span class="ql-author-8876147">The QHY533M uses a similar series of sensors to the flagship models <a href="https://www.modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy600-mono-full-frame-cooled-cmos-camera/">QHY600</a> and <a href="https://www.modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy268m-mono-cmos-camera/">QHY268</a>, featuring low noise and improved full well capacity.</span></p>
<div class="child">
<div class="block lv2 on">
<h3 id="b10" class="tit">Features</h3>
<div class="cnt">
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20210602659.png"><img decoding="async" class="wp-image-1586 alignleft" src="https://www.qhyccd.com/wp-content/uploads/20210602659.png" alt="" width="100" height="100" /></a><strong>BSI</strong></p>
<p>One benefit of the back-illuminated CMOS structure is improved full well capacity. This is particularly helpful for sensors with small pixels. In a typical front-illuminated sensor, photons from the target entering the photosensitive layer of the sensor must first pass through the metal wiring that is embedded just above the photosensitive layer. The wiring structure reflects some of the photons and reduces the efficiency of the sensor.</p>
<p>In the back- illuminated sensor the light is allowed to enter the photosensitive surface from the reverse side. In this case the sensor’s embedded wiring structure is below the photosensitive layer. As a result, more incoming photons strike the photosensitive layer and more electrons are generated and captured in the pixel well. This ratio of photon to electron production is called quantum efficiency. The higher the quantum efficiency the more efficient the sensor is at converting photons to electrons and hence the more sensitive the sensor is to capturing an image of something dim.</p>
<p>&nbsp;</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20210602542.png"><img decoding="async" class="wp-image-1573 alignleft" src="https://www.qhyccd.com/wp-content/uploads/20210602542.png" alt="" width="100" height="100" /></a><strong>TRUE RAW Data</strong></p>
<p>In the DSLR implementation there is a RAW image output, but typically it is not completely RAW.  Some evidence of noise reduction and hot pixel removal is still visible on close inspection.  This can have a negative effect on the image for astronomy such as the “star eater” effect.  However,  QHY Cameras offer TRUE RAW IMAGE OUTPUT and produces an image comprised of the original signal only, thereby maintaining the maximum flexibility for post-acquisition astronomical image processing programs and other scientific imaging applications.</p>
<p>&nbsp;</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20210602234.png"><img decoding="async" class="wp-image-1604 alignleft" src="https://www.qhyccd.com/wp-content/uploads/20210602234.png" alt="" width="100" height="100" /></a><strong>Anti-Dew Technology</strong></p>
<p>Based on almost 20-year cooled camera design experience, The QHY cooled camera has implemented the fully dew control solutions. The optic window has built-in dew heater and the chamber is protected from internal humidity condensation. An electric heating board for the chamber window can prevent the formation of dew and the sensor itself is kept dry with our silicon gel tube socket design for control of humidity within the sensor chamber.</p>
<p>&nbsp;</p>
<p><img decoding="async" class="wp-image-1585 alignleft" src="https://www.qhyccd.com/wp-content/uploads/20210602302.png" alt="" width="100" height="100" /><strong>Cooling</strong></p>
<p>In addition to dual stage TE cooling, QHYCCD implements proprietary technology in hardware to control the dark current noise.</p>
</div>
</div>
<div class="block lv2 on">
<div id="b11" class="tit">Amplify Control</div>
<div class="cnt">
<p>Compare to the last generation’s astrocam for beginners, like QHY183 or QHY 163, the QHY533M CMOS Camera has much better amplifier control.</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220428929-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2397" src="https://www.qhyccd.com/wp-content/uploads/20220428929-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220428929-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220428929-768x768.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220428929-1536x1536.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220428929-2048x2048.jpg 2048w" alt="" width="800" height="800" /></a></p>
<p>QHY533M Dark Frame, 300s</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220428442-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2396" src="https://www.qhyccd.com/wp-content/uploads/20220428442-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220428442-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220428442-768x510.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220428442-1536x1021.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220428442-2048x1361.jpg 2048w" alt="" width="800" height="532" /></a></p>
<p>QHY183M Dark Frame, 300s</p>
<p>&nbsp;</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220429950-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2399" src="https://www.qhyccd.com/wp-content/uploads/20220429950-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220429950-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220429950-768x768.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220429950-1536x1536.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220429950-2048x2048.jpg 2048w" alt="" width="800" height="800" /></a></p>
<p>QHY533M Dark frame, 600s, with highest gain (170) and strech–only very slight amplify can be detected at the corner.</p>
</div>
</div>
</div>
</div>
<div class="block lv1 on">
<h3 id="a2" class="tit">Design</h3>
<p class="ql-long-8876147"><span class="ql-author-8876147">QHY533M (mono) and 533C (color) have different interface designs to be more flexible to deal with different applications.</span></p>
<p class="ql-long-8876147"><span class="ql-author-8876147">QHY533M can be directly connected to the QHYCFW3S-SR without removing <strong>any part of the filter wheel </strong>(like the filter container). This provides a very short back focal length and that’s easy to fix! Besides, QHY533M + QHYCFW3S-SR combination can be easily connected to a DSLR lens, with only one additional adapter (sold separately).  </span></p>
<p class="ql-long-8876147"><span class="ql-author-8876147">Both QHY533M/C comes with an additional adapter for tripod interface. This makes it easier to shoot with DSLR lens.</span></p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220711590.jpg"><img decoding="async" class="aligncenter wp-image-2550" src="https://www.qhyccd.com/wp-content/uploads/20220711590.jpg" sizes="(max-width: 850px) 100vw, 850px" srcset="https://www.qhyccd.com/wp-content/uploads/20220711590.jpg 920w, https://www.qhyccd.com/wp-content/uploads/20220711590-768x389.jpg 768w" alt="" width="850" height="431" /></a></p>
<div class="child">
<div class="block lv2 on">
<h3 id="b20" class="tit">QHYCFW3S Adjustment for QHY533M</h3>
<div class="cnt">
<p><span class="ql-author-8876147">In order to let all astrophotographers easily use 533M’s threaded interface to connect filter wheel without removing <strong>any part of the filter wheel </strong>(like the filter container), s</span><span class="ql-author-8876147">ince 2022, QHYCFW3-SR won’t be loaded with this adapter (below).  This adapter is used to connect QHY163 or QHY183 while QHY533M doesn’t need it. Therefore, if you want to get a QHY533M, we recommend you choose QHYCFW3S-SR for the best experience.</span></p>
<p>By the way, this adapter is still contained in CFW3S-SR’s package. You can still use CFW3S-SR with QHY183 or QHY163.</p>
<p>&nbsp;</p>
<p><span class="ql-author-8876147"><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220705345.png"><img decoding="async" class="aligncenter wp-image-2540" src="https://www.qhyccd.com/wp-content/uploads/20220705345.png" alt="" width="247" height="236" /></a></span></p>
</div>
</div>
<div class="block lv2 on">
<h3 id="b21" class="tit">QHY533M parallel position adjustment</h3>
<div class="cnt">
<p class="ql-long-8876147"><span class="ql-author-8876147">The QHY533M CMOS Camera is connected to the QHYCFW3S by using threads， so the sensor may not parallel to the filter wheel when the threads are fully rotated. In this case you can adjust the front part of the 533M to the right angle of the sensor.</span></p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106896-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2275" src="https://www.qhyccd.com/wp-content/uploads/20220106896-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106896-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106896-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106896-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106896-2048x1365.jpg 2048w" alt="" width="800" height="533" /></a></p>
</div>
</div>
<div class="block lv2 on">
<h3 id="b22" class="tit">QHY533C Design</h3>
<div class="cnt">
<p><span class="ql-author-8876147">A free <strong>Adapter Kit E </strong>will be provided with QHY533C. The adapters can be directly connected to the 55mm BFL M48 interface MPCC, or Nikon / Canon DSLR lens (need to purchase another DSLR lens adapter). At the same time, the C-port thread can be provided with the QHY533C and you can directly mount the C-port lens.</span><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106761-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2270" src="https://www.qhyccd.com/wp-content/uploads/20220106761-scaled.jpg" sizes="(max-width: 500px) 100vw, 500px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106761-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106761-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106761-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106761-2048x1365.jpg 2048w" alt="" width="500" height="333" /></a></p>
</div>
</div>
</div>
</div>
<div class="block lv1 on">
<div id="a3" class="tit">Specifications</div>
<table width="100%">
<tbody>
<tr>
<td width="18%"><strong>Model</strong></td>
<td width="41%"><strong>QHY533M</strong></td>
<td width="39%"><strong>QHY533C</strong></td>
</tr>
<tr>
<td width="18%">COMS Sensor</td>
<td width="41%">SONY IMX533 M</td>
<td width="39%">SONY IMX533 C</td>
</tr>
<tr>
<td width="18%">Mono/Color</td>
<td width="41%">Mono</td>
<td width="39%">Color</td>
</tr>
<tr>
<td width="18%">FSI/BSI</td>
<td colspan="2" width="81%">BSI</td>
</tr>
<tr>
<td width="18%">Pixel Size</td>
<td colspan="2" width="81%">3.76um x 3.76um</td>
</tr>
<tr>
<td width="18%">Effective Pixel Area</td>
<td colspan="2" width="81%">3008*3028 (includes the optically black area and overscan area)</td>
</tr>
<tr>
<td width="18%">Effective Pixels</td>
<td colspan="2" width="81%">9MP</td>
</tr>
<tr>
<td width="18%">Sensor Size</td>
<td colspan="2" width="81%">1 inch</td>
</tr>
<tr>
<td width="18%">A/D Sample Depth</p>
<p>&nbsp;</td>
<td colspan="2" width="81%">Native 14-bit A/D</td>
</tr>
<tr>
<td width="18%">Full Well Capacity (1×1, 2×2, 3×3)</td>
<td colspan="2" width="81%">58ke-</td>
</tr>
<tr>
<td width="18%">Full Frame Rate</td>
<td colspan="2" width="81%">USB3.0 Port:<br />
Full Resolution  26.5FPS  @8BIT         20FPS @16BIT2160Lines          37FPS     @8BIT          28.5FPS@16BIT1080Lines          71.5FPS   @8BIT          55FPS @16BIT768Lines             97FPS      @8BIT          76FPS @16BIT480Lines             152FPS    @8BIT          117FPS @16BIT240Lines             280FPS    @8BIT         215FPS@16BIT</td>
</tr>
<tr>
<td width="18%">Readout Noise</td>
<td colspan="2" width="81%">1.3 to 3.4e-</td>
</tr>
<tr>
<td width="18%">Dark Current</td>
<td colspan="2" width="81%">-20C，0.0005e- /pixel/sec</td>
</tr>
<tr>
<td width="18%">Exposure Time Range</td>
<td colspan="2" width="81%">30us-3600sec</td>
</tr>
<tr>
<td width="18%">Unity Gain</td>
<td colspan="2" width="81%">68</td>
</tr>
<tr>
<td width="18%"></td>
<td colspan="2" width="81%"></td>
</tr>
<tr>
<td width="18%">Shutter Type</td>
<td colspan="2" width="81%">Electronic Shutter</td>
</tr>
<tr>
<td width="18%">Computer Interface</td>
<td colspan="2" width="81%">USB3.0</td>
</tr>
<tr>
<td width="18%">Built-in Image Buffer</td>
<td colspan="2" width="81%">1GByte DDR3 Memory</td>
</tr>
<tr>
<td width="18%">Cooling System</td>
<td colspan="2" width="81%">Two-stage TEC cooler</p>
<p>Less than 1S lower than ambient temperature -30C in continuous mode</p>
<p>More than 1S continuous mode or lower than ambient temperature -35C in single frame mode</p>
<p>（Test temperature +20°）</td>
</tr>
<tr>
<td width="18%">Optic Window Type</td>
<td colspan="2" width="81%">AR+AR High Quality Multi-Layer Anti-Reflection Coating</td>
</tr>
<tr>
<td width="18%">Anti-Dew Heater</td>
<td colspan="2" width="81%">Yes</td>
</tr>
<tr>
<td width="18%"></td>
<td width="41%"></td>
<td width="39%"></td>
</tr>
<tr>
<td width="18%">Telescope Interface</td>
<td width="41%">–</td>
<td width="39%">Support M48 (with adapter)</td>
</tr>
<tr>
<td width="18%">Back Focal Length</td>
<td width="41%">Actual Back Focal Consumed: 14 mm (Combined with CFW)</p>
<p>Standard BFL: 17.5mm（±0.5）</td>
<td width="39%">17mm</td>
</tr>
<tr>
<td width="18%">Weight</td>
<td width="41%">845g</td>
<td width="39%">845g</td>
</tr>
</tbody>
</table>
<div class="child">
<div class="block lv2 on">
<div id="b30" class="tit">Curves</div>
<div class="cnt">
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106495.png"><img decoding="async" class="aligncenter size-full wp-image-2263" src="https://www.qhyccd.com/wp-content/uploads/20220106495.png" sizes="(max-width: 2289px) 100vw, 2289px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106495.png 2289w, https://www.qhyccd.com/wp-content/uploads/20220106495-768x383.png 768w, https://www.qhyccd.com/wp-content/uploads/20220106495-1536x766.png 1536w, https://www.qhyccd.com/wp-content/uploads/20220106495-2048x1022.png 2048w" alt="" width="2289" height="1142" /></a><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106205.png"><img decoding="async" class="aligncenter size-full wp-image-2264" src="https://www.qhyccd.com/wp-content/uploads/20220106205.png" sizes="(max-width: 2335px) 100vw, 2335px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106205.png 2335w, https://www.qhyccd.com/wp-content/uploads/20220106205-768x360.png 768w, https://www.qhyccd.com/wp-content/uploads/20220106205-1536x720.png 1536w, https://www.qhyccd.com/wp-content/uploads/20220106205-2048x960.png 2048w" alt="" width="2335" height="1095" /></a><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/2022010616.png"><img decoding="async" class="aligncenter size-full wp-image-2265" src="https://www.qhyccd.com/wp-content/uploads/2022010616.png" sizes="(max-width: 2294px) 100vw, 2294px" srcset="https://www.qhyccd.com/wp-content/uploads/2022010616.png 2294w, https://www.qhyccd.com/wp-content/uploads/2022010616-768x383.png 768w, https://www.qhyccd.com/wp-content/uploads/2022010616-1536x767.png 1536w, https://www.qhyccd.com/wp-content/uploads/2022010616-2048x1022.png 2048w" alt="" width="2294" height="1145" /></a></p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220411218.jpg"><img decoding="async" class="aligncenter size-full wp-image-2371" src="https://www.qhyccd.com/wp-content/uploads/20220411218.jpg" sizes="(max-width: 2560px) 100vw, 2560px" srcset="https://www.qhyccd.com/wp-content/uploads/20220411218.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220411218-768x375.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220411218-1536x750.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220411218-2048x1000.jpg 2048w" alt="" width="2560" height="1250" /></a></p>
</div>
</div>
<div class="block lv2 on">
<h3 id="b31" class="tit">Mechanical Dimensions</h3>
<div class="cnt">
<p>&nbsp;</p>
<p>QHY533M CMOS Camera</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220407216.jpg"><img decoding="async" class="aligncenter wp-image-2362" src="https://www.qhyccd.com/wp-content/uploads/20220407216.jpg" sizes="(max-width: 900px) 100vw, 900px" srcset="https://www.qhyccd.com/wp-content/uploads/20220407216.jpg 1182w, https://www.qhyccd.com/wp-content/uploads/20220407216-768x767.jpg 768w" alt="" width="900" height="898" /></a></p>
<p>QHY533C</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220407696.jpg"><img decoding="async" class="aligncenter wp-image-2363" src="https://www.qhyccd.com/wp-content/uploads/20220407696.jpg" sizes="(max-width: 900px) 100vw, 900px" srcset="https://www.qhyccd.com/wp-content/uploads/20220407696.jpg 1198w, https://www.qhyccd.com/wp-content/uploads/20220407696-768x769.jpg 768w" alt="" width="900" height="902" /></a></p>
<p>&nbsp;</p>
</div>
</div>
</div>
</div>
<div class="block lv1 on">
<h3 id="a4" class="tit">Matching Accessories</h3>
<div></div>
<div class="child">
<div class="block lv2 on">
<div id="b40" class="tit">QHY533M CMOS Camera</div>
<div class="child">
<div class="block lv3 on">
<div class="cnt">
<p class="ql-long-8876147"><span class="ql-author-8876147">QHY533M external use of threaded interface can be directly connected to the small filter wheel. This time we will launch a special standard small filter wheel version together with the 533M, which can be assembled directly by the user externally without removing the disc. When the QHY533M + filter wheel combination is connected to a DSLR lens, only an additional DSLR lens adapter ring (sold separately) is required to complete the focus. </span></p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220414894.png"><img decoding="async" class="aligncenter size-full wp-image-2374" src="https://www.qhyccd.com/wp-content/uploads/20220414894.png" sizes="(max-width: 1920px) 100vw, 1920px" srcset="https://www.qhyccd.com/wp-content/uploads/20220414894.png 1920w, https://www.qhyccd.com/wp-content/uploads/20220414894-768x1440.png 768w, https://www.qhyccd.com/wp-content/uploads/20220414894-819x1536.png 819w, https://www.qhyccd.com/wp-content/uploads/20220414894-1092x2048.png 1092w" alt="" width="1920" height="3600" /></a></p>
</div>
</div>
</div>
</div>
<div class="block lv2 on">
<div id="b41" class="tit">QHY533C</div>
<div class="cnt"></div>
<div class="child">
<div class="block lv3 on">
<div id="c410" class="tit"></div>
<div class="cnt">
<p class="ql-long-8876147"><span class="ql-author-8876147">Adapter Kit E1 can be directly connected to the 55mm BFL M48 interface MPCC, or Nikon / Canon DSLR lens (need to purchase another DSLR lens adapter). </span></p>
<p>E1 is designed for QHY533C, 294C, 163C, 183C, 174C. Of course, if you use 163M/294M/183M/174M while a filter wheel or OAG is not needed, you can use E1 as well.</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220414219.png"><img decoding="async" class="aligncenter size-full wp-image-2372" src="https://www.qhyccd.com/wp-content/uploads/20220414219.png" sizes="(max-width: 1930px) 100vw, 1930px" srcset="https://www.qhyccd.com/wp-content/uploads/20220414219.png 1930w, https://www.qhyccd.com/wp-content/uploads/20220414219-768x938.png 768w, https://www.qhyccd.com/wp-content/uploads/20220414219-1258x1536.png 1258w, https://www.qhyccd.com/wp-content/uploads/20220414219-1678x2048.png 1678w" alt="" width="1930" height="2356" /></a></p>
<p>&nbsp;</p>
</div>
</div>
</div>
</div>
</div>
</div>
<div class="block lv1 on">
<div id="a5" class="tit">Reviews</div>
<p>&nbsp;</p>
<div class="fluid-width-video-wrapper"><iframe title="New QHY533M - Best BEGINNER Mono Camera for Astrophotography? (Raw Data Included!)" src="https://www.youtube.com/embed/cxGpYN4c0o8?feature=oembed" name="fitvid0" frameborder="0" allowfullscreen="allowfullscreen" data-mce-fragment="1"></iframe></div>
<p><a href="https://www.galactic-hunter.com/post/qhy533m-review">https://www.galactic-hunter.com/post/qhy533m-review</a></p>
<p>&nbsp;</p>
<div class="fluid-width-video-wrapper"><iframe title="Narrowband in the City: Should You Go MONO?" src="https://www.youtube.com/embed/kJptGyDVCZ0?feature=oembed" name="fitvid1" frameborder="0" allowfullscreen="allowfullscreen" data-mce-fragment="1"></iframe></div>
<div class="fluid-width-video-wrapper"><iframe title="QHY533M - Everything You Need to Know, Hands On Review of the new Square Mono Sensor" src="https://www.youtube.com/embed/2t5MPUHCe0k?feature=oembed" name="fitvid2" frameborder="0" allowfullscreen="allowfullscreen" data-mce-fragment="1"></iframe></div>
<p>&nbsp;</p>
</div>
<div class="block lv1 ">
<div id="a6" class="tit">User Guide: Start the Camera</div>
</div>
<div class="block lv1 ">
<div id="a7" class="tit">Camera Maintenance</div>
</div>
<div class="block lv1 ">
<div id="a8" class="tit">FAQs</div>
</div>
<div class="block lv1 ">
<div id="a9" class="tit">Appendix 1: How to Set Gain and Offset</div>
</div>
<div class="block lv1 ">
<div id="a10" class="tit">Appendix 2: Bayer Sequences of Some Colored Cameras</div>
</div>
<div class="block lv1 ">
<div id="a11" class="tit">Appendix 3: White Balance Adjustment</div>
</div>
<div class="block lv1 on">
<div id="a12" class="tit">Appendix 4: QHY533M Parallel Position Adjustment</div>
<p class="ql-long-8876147"><span class="ql-author-8876147">The QHY533M is connected to the QHYCFW3S by using threads. So there might be a small problem that the sensor may not remain parallel to the filter wheel when the threads are fully rotated. In this case you can adjust the front part of the 533M to the angle of sensor correct.</span></p>
<p class="ql-long-8876147"><strong class="ql-author-8876147">Steps</strong></p>
<ul>
<li class=""><span class="ql-author-8876147">Remove the front part of the camera.</span><span class="ql-author-8876147"> Rotate the front part onto the filter wheel.</span></li>
<li class=""><span class="ql-author-8876147">Position the camera so that the sensor is parallel to the filter wheel. Then use one screw to fix it.</span></li>
<li class=""><span class="ql-author-8876147">Remove the filter wheel and fix the other two screws. Finally install the filter wheel.</span></li>
</ul>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106457-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2279" src="https://www.qhyccd.com/wp-content/uploads/20220106457-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106457-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106457-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106457-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106457-2048x1365.jpg 2048w" alt="" width="800" height="533" /></a><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106309-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2280" src="https://www.qhyccd.com/wp-content/uploads/20220106309-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106309-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106309-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106309-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106309-2048x1365.jpg 2048w" alt="" width="800" height="533" /></a><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106433-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2281" src="https://www.qhyccd.com/wp-content/uploads/20220106433-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106433-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106433-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106433-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106433-2048x1365.jpg 2048w" alt="" width="800" height="533" /></a><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106524-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2282" src="https://www.qhyccd.com/wp-content/uploads/20220106524-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106524-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106524-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106524-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106524-2048x1365.jpg 2048w" alt="" width="800" height="533" /></a><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20220106417-scaled.jpg"><img decoding="async" class="aligncenter wp-image-2283" src="https://www.qhyccd.com/wp-content/uploads/20220106417-scaled.jpg" sizes="(max-width: 800px) 100vw, 800px" srcset="https://www.qhyccd.com/wp-content/uploads/20220106417-scaled.jpg 2560w, https://www.qhyccd.com/wp-content/uploads/20220106417-768x512.jpg 768w, https://www.qhyccd.com/wp-content/uploads/20220106417-1536x1024.jpg 1536w, https://www.qhyccd.com/wp-content/uploads/20220106417-2048x1365.jpg 2048w" alt="" width="800" height="533" /></a></p>
</div>
<div class="block lv1 on">
<div id="a13" class="tit">Appendix: UVLO Function</div>
<div class="child">
<div class="block lv2 on">
<div id="b130" class="tit"></div>
<div class="cnt">
<p><strong>Note: Now only QHY600, QHY268, QHY410, QHY411, QHY461, QHY533 cameras have UVLO function.</strong></p>
<p><strong>What is UVLO?</strong></p>
<p>UVLO（Under Voltage Locking), is primarily intended to protect the electronic device from damage caused by abnormally low voltages.</p>
<p>Our daily life experience tells us that the actual operational voltage of an electrical device must not significantly exceed the rated voltage, otherwise it will be damaged. For such precision equipment as cameras, long-term work at too low input voltage can also be detrimental to the working life of the camera, and may even make some devices, such as power manager, burn up due to long-term overload. In the all-in-one driver and SDK after 2021.10.23 stable version, the camera will give a warning when the input voltage of the camera is below 11V.</p>
<p><strong>UVLO warning execution</strong></p>
<p>After a warning is given, the camera firmware will automatically turn off the cooler and will turn on the camera’s TEC protection mode. After the camera is reconnected, it will always work in TEC protection mode (maximum power cooler power will be limited to 70%). Since many times the voltage shortage is caused by the high resistance of the power supply cable itself, resulting in a large voltage drop at high currents, the voltage will usually rise after the power is limited. But limiting the power will affect the cooling temperature difference. Therefore, it is recommended that users first check the power supply cable to solve the problem of excessive resistance of the power supply cable.</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20211112177.png"><img decoding="async" class="aligncenter size-full wp-image-2188" src="https://www.qhyccd.com/wp-content/uploads/20211112177.png" alt="" width="747" height="302" /></a></p>
<p>If the user has solved the problem of insufficient supply voltage, the TEC protection mode can be removed through the menu of EZCAP_QT.</p>
<p><strong>How to improve the power supply?</strong></p>
<ol>
<li>Make sure the output voltage of the AC adapter is not less than 12V and the maximum output current can reach 4A or more. Otherwise, the AC adapter itself will not meet the power demand of the camera and it may cause a low voltage problem.</li>
<li> Make sure that the 12V power supply cable connecting the AC adapter to the camera has a low impedance. The impedance of the positive and negative paths should not exceed 0.1 ohms each. Or the total impedance (positive + negative) should not exceed 0.2 ohms. Otherwise, the power supply cable should be thickened.</li>
<li>When using battery power, it is recommended to add a 12V output voltage regulator. If the battery is connected directly, usually the battery voltage reaches 13.8V when fully charged, and will gradually drop during use. It is easy to cause the camera to reach the low-voltage detection threshold.</li>
</ol>
<p>&nbsp;</p>
<p><strong>How to clear the TEC protection status triggered by UVLO?</strong></p>
<p>Once a UVLO event occurs, the camera will automatically memorize it and will work in a protected mode at a maximum of 70% power after reconnection. This memory can be erased as follows:</p>
<p>After you find the system error, you need to turn off the device and check the power supply. After inspecting the problem, open the ezcap software and select “Camera Settings” – “Preferences” – “Reset Flash Code” to reset the error status.</p>
<p><a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20211112353.png"><img decoding="async" class="aligncenter wp-image-2189 size-full" src="https://www.qhyccd.com/wp-content/uploads/20211112353.png" sizes="(max-width: 1017px) 100vw, 1017px" srcset="https://www.qhyccd.com/wp-content/uploads/20211112353.png 1017w, https://www.qhyccd.com/wp-content/uploads/20211112353-768x427.png 768w" alt="" width="1017" height="565" /></a></p>
<p>&nbsp;</p>
<p><strong>Why does the warning appear even though the power supply voltage is 12 V?</strong></p>
<ol>
<li>The voltage measured inside the camera is the voltage reaching the camera, not the voltage at the power adapter end. Therefore, the voltage measured at the power adapter end does not reflect the voltage received at the camera end. This is because the power cable has its own resistance. If the resistance is large, it will cause a large voltage drop. The voltage drop can be calculated by U = I * R. So if the power cable has a resistance of 0.2 ohms, it will produce a voltage drop of 3.3 * 0.2 = 0.66V. If the power adapter output is 12 V, the voltage reaching the camera is 12 – 0.66 = 11.34 V. To actually measure the input voltage at the camera end, you can refer to the photo below.<a class="oceanwp-lightbox" href="https://www.qhyccd.com/wp-content/uploads/20211112482.jpg"><img decoding="async" class="aligncenter size-full wp-image-2190" src="https://www.qhyccd.com/wp-content/uploads/20211112482.jpg" alt="" width="553" height="415" /></a></li>
<li>For cameras produced after September 2021, the UVLO is detected by communicating directly with the power manager, and the UVLO code that appears is 9, while for cameras produced before, the indirect detection method is used, and the UVLO code that appears is 3. The indirect detection method will detect UVLO except for the low voltage problem, and any other accident that causes CMOS not to work will also trigger the UVLO=3 alarm, for example, the camera is subject to severe electromagnetic interference, causing registers inside the CMOS not to work. Therefore, if UVLO=3 occurs, it is recommended to contact QHYCCD technical support for further judgment.</li>
<li> Using older versions of drivers and firmware may cause false positives (UVLO=9). Please make sure that ALL-in-one SDK version is out of stable version 2021.10.23 or higher. Please disconnect the 12V power supply during the driver installation.</li>
</ol>
<p>&nbsp;</p>
</div>
</div>
</div>
</div>
<p>The post <a href="https://modernastronomy.com/shop/cameras/astro-video/qhy/qhy533m-cmos-camera/">QHY533M CMOS Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></content:encoded>
					
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			</item>
		<item>
		<title>Omegon Mount MiniTrack LX Quattro NS</title>
		<link>https://modernastronomy.com/shop/mounts/omegon/omegon-mount-minitrack-lx-quattro-ns/</link>
					<comments>https://modernastronomy.com/shop/mounts/omegon/omegon-mount-minitrack-lx-quattro-ns/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Thu, 02 Dec 2021 11:10:31 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=92764</guid>

					<description><![CDATA[<p>The Omegon Mount MiniTrack LX Quattro NS is a portable mini-mount for astrophotography with wide-angle and lightweight telephoto lenses, which doesn't require a power supply. It allows you to capture great images of the night sky - even if you haven't tried before. Price includes UK delivery!</p>
<p>The post <a href="https://modernastronomy.com/shop/mounts/omegon/omegon-mount-minitrack-lx-quattro-ns/">Omegon Mount MiniTrack LX Quattro NS</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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<p>The Omegon Mount MiniTrack LX Quattro NS is a re-design of the popular <a href="https://www.modernastronomy.com/shop/mounts/omegon/omegon-mount-mini-track-lx3/">LX3 mini-mount</a> for better astrophotography using wide-angle and lightweight telephoto lenses. It will allow you to capture fascinating images of the night sky &#8211; even if you haven&#8217;t done any astrophotography until now.</p>
<p>The Omegon Mount MiniTrack LX Quattro NS is purely mechanical, without batteries &#8211; and now also takes heavy cameras and lenses weighing up to 4 kilograms. But there&#8217;s even more to it: the MiniTrack Quattro has been redesigned from scratch and is now better than ever. For successful astrophotography that&#8217;s addictive.</p>
<p>&nbsp;</p>
<p><b>The highlights at a glance:</b></p>
<ul>
<li>Successfully and effortlessly capturing the night sky</li>
<li>No need to recharge: functions using a mechanical system, independent of battery and power cables</li>
<li>Wind up the mechanism and get going immediately</li>
<li>Perfect for wide shots of the starry sky and telephoto lenses</li>
<li>Fits in every backpack: the perfect mount for travelling &#8211; wherever the road takes you.</li>
</ul>
<p>&nbsp;</p>
<p>&nbsp;</p>
<p><b>The special advantages of the MiniTrack LX Quattro:</b></p>
<ul>
<li>Even stronger: the new MiniTrack now takes even heavy cameras up to 4 kg</li>
<li>A needle roller bearing ensures smooth running &#8211; for better-tracked images</li>
<li>Newly developed spring system: the stronger spring system replaces a counterweight and reliably guides cameras even with heavy one-sided loads</li>
<li>CNC body: the MiniTrack consists of a piece of machined aluminium &#8211; high quality, stable, the perfect companion on every trip</li>
<li>Optical polar finder for exact alignment to the celestial pole</li>
<li>Simple conversion for astrophotography in the southern hemisphere</li>
<li>Simple to assemble: built-in Vixen GP-style plate &#8211; no additional rail needed</li>
</ul>
<p>&nbsp;</p>
<p>&nbsp;</p>
<p><b>Better astronomy photos when travelling or at home</b></p>
<p>Now bring home not only holiday snaps but also impressive astronomy photos from your travels. It&#8217;s easier than you might think. All you need: a tripod, the MiniTrack, a ball head and your camera. Reduced to the essentials, it has just one mission: good astrophotography that everyone can manage. Here&#8217;s how it&#8217;s done&#8230;</p>
<p>&nbsp;</p>
<p><b>60 minutes of mechanical tracking</b></p>
<p>The MiniTrack has a mechanical heart &#8211; there&#8217;s no place for electronics here. The accurate clockwork precisely guides your camera. Wind up the MiniTrack like an analogue clock and the tracking is activated. This mount never fails, even at sub-zero temperatures. Your new mount keeps a cool head, even with telephoto lenses. It is not without reason that this wide-field photography expert has conquered the hearts of amateur astronomers.</p>
<p>&nbsp;</p>
<p><b>The smallest counterweight in the world?</b></p>
<p>The MiniTrack Quattro has a completely new spring system. It&#8217;s not a counterweight, but it works like one. It ensures that the LX Quattro remains as compact and travel-ready as ever. It&#8217;s simply got better and stronger. The spring directly drives the axle and guides your camera like a strong and precise arm.</p>
<p>Tip: an ideal tracking speed is reached when the mechanism ticks at 130-135 times per minute. You may need to adjust the spring tension, depending on the weight of your camera. We recommend that you measure the ticks per minute with a TapTempo BPM app for smartphones. These apps are created for the music industry and are supposed to automatically measure the tempo of a song. But you can use such an app to measure the MiniTrack&#8217;s speed.</p>
<p>&nbsp;</p>
<p><b>Needle roller bearing: track the stars precisely</b></p>
<p>The MiniTrack&#8217;s integrated needle roller bearing performs the same role as power-steering in a car: It runs as smooth as silk. This is exactly what is needed, because the MiniTrack tracks the stars smoothly and precisely even when carrying heavier loads.</p>
<p>&nbsp;</p>
<p><b>Looks great, inside and out: CNC housing made completely of aluminium</b></p>
<p>A real eye-catcher: The body of the MiniTrack Quattro now consists of a single piece of aluminium. No corners have been cut here, which makes this model even more stable. Whatever you demand from your MiniTrack, it will accompany you up mountains or on your travels and will succeed in every astronomy adventure with a smile.</p>
<p>&nbsp;</p>
<p><b>High load-bearing capacity of 4 kilogrammes</b></p>
<p>The MiniTrack has now become fitter and can carry cameras weighing up to 4 kilogrammes. At the same time, our developers have kept the old and proven form. So the MiniTrack Quattro still fits in any bag. Have you always wanted to use a large and particularly fast lens? Until now, unfortunately it was always too big &#8211; but now it&#8217;s possible.</p>
<p>&nbsp;</p>
<p><b>Find the celestial pole more precisely</b></p>
<p>Simply use the optical polar finder to find the celestial pole. The MiniTrack comes with a holder and a polar finder, as also seen on large mounts. This makes it even easier to align the MiniTrack for images with point-shaped stars.</p>
<p>&nbsp;</p>
<p><b>Fits on every photographic tripod</b></p>
<p>The MiniTrack has two connectors: for the tripod and for your camera or a ball head. Attach the mount to your photographic tripod as usual using a 1/4&#8243; thread, and align the MiniTrack as required. On the other side, attach a ball head using a 3/8&#8243; thread.</p>
<p>&nbsp;</p>
<p><b>GP plate for mounting</b></p>
<p>Simply attach the MiniTrack to a polar wedge. You don&#8217;t need a prism rail. A GP Vixen-style plate has been incorporated into the body. Here everything is fully integrated and you no longer need to waste time on screws or spanners.</p>
<p>And if you want to mount the MiniTrack onto a tilt head? There is an integrated 1/4&#8243; and 3/8&#8243; thread for this purpose.</p>
<p>&nbsp;</p>
<p><b>Invented by Cristian Fattinnanzi, further developed by Omegon</b></p>
<p>The MiniTrack was developed by Christian Fattinnanzi from Italy. Together with the inventor, Omegon has further developed the MiniTrack and realised it technically. It is now a perennial favourite and is used by thousands of astrophotographers all over the world. To ensure consistently high quality, we manufacture the MiniTrack exclusively in Portugal, where it is assembled and tested by our specialists.</p>
<p>With this fully mechanical mini-mount, you can take astronomy photos in no time at all. No power. No charging. No batteries. Just take photographs. Anytime, anywhere.</p>
<p>Tags: MiniTrack, Mini Track, LX2, LX3, LX4, Lx Quattro</p>
<p>Scope of delivery:</p>
<ul>
<li>MiniTrack LX Quattro</li>
<li>Optical polar finder</li>
<li>Polar finder holder</li>
<li>Insert for the southern hemisphere</li>
</ul>
</div>
</div>
</div>
<p>The post <a href="https://modernastronomy.com/shop/mounts/omegon/omegon-mount-minitrack-lx-quattro-ns/">Omegon Mount MiniTrack LX Quattro NS</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<title>QHY5III462C Expansion Kit</title>
		<link>https://modernastronomy.com/shop/accessories/qhy-accessories/qhy5iii462c-expansion-kit/</link>
					<comments>https://modernastronomy.com/shop/accessories/qhy-accessories/qhy5iii462c-expansion-kit/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Thu, 03 Sep 2020 12:51:34 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=90991</guid>

					<description><![CDATA[<p>The QHY5III462C Expansion Kit Contains:</p>
<ul>
<li>1.25″ 10nm Methane Filter (890nm) – <a href="https://www.planetary-astronomy-and-imaging.com/en/making-methane-images-jupiter/" target="_blank" rel="noopener noreferrer">info</a> – <a href="https://britastro.org/journal_item/8975" target="_blank" rel="noopener noreferrer">more info</a></li>
</ul>
<ul>
<li>Wide Angle All-Sky CS Lens (2.5mm F1.2)</li>
</ul>
<ul>
<li>CS Mount Lens Adapter</li>
</ul>
<p>This kit can also be used as a cost effective upgrade for CS / Mini cameras from ZWO, Altair and others</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/qhy-accessories/qhy5iii462c-expansion-kit/">QHY5III462C Expansion Kit</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<p>The QHY5III462C Expansion Kit Contains:</p>
<ul>
<li>1.25″ 10nm Methane Filter (890nm) – <a href="https://www.planetary-astronomy-and-imaging.com/en/making-methane-images-jupiter/" target="_blank" rel="noopener noreferrer">info</a> – <a href="https://britastro.org/journal_item/8975" target="_blank" rel="noopener noreferrer">more info</a></li>
</ul>
<ul>
<li>Wide Angle All-Sky CS Lens (2.5mm F1.2)</li>
</ul>
<ul>
<li>CS Mount Lens Adapter</li>
</ul>
<p>This kit can also be used as a cost effective upgrade for CS / Mini cameras from ZWO, Altair and others.</p>
<p>If unsure please email for advice.</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/qhy-accessories/qhy5iii462c-expansion-kit/">QHY5III462C Expansion Kit</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<title>QHY5III462C Camera and Expansion Kit</title>
		<link>https://modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-camera-and-expansion-kit/</link>
					<comments>https://modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-camera-and-expansion-kit/#comments</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Sun, 16 Aug 2020 20:14:30 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=90893</guid>

					<description><![CDATA[<p>The QHY5III462C Camera and <a href="https://www.modernastronomy.com/shop/accessories/lenses/qhy5iii462c-expansion-kit-only/" target="_blank" rel="noopener noreferrer">Expansion Kit</a> contains all the items in the <a href="https://www.modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-planetary-and-nir-imaging-camera/" target="_blank" rel="noopener noreferrer">standard kit</a> plus a quality Methane (CH4) filter and All Sky Lens.<br />
The most useful and exciting new camera in years and the perfect "All in One Camera" for Planetary, Guiding, Near IR and basic Deep Sky use.<br />
Uses the IMX462 sensor in the <a href="https://www.modernastronomy.com/shop/telescopes/smart-telescopes/zwo-seestar-s50-all-in-one-smart-apo-refractor/" target="_blank" rel="noopener">SeeStar S50 All-in-One Smart APO Refractor</a>!</p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-camera-and-expansion-kit/">QHY5III462C Camera and Expansion Kit</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<p>The QHY5III462C Camera and <a href="https://www.modernastronomy.com/shop/accessories/lenses/qhy5iii462c-expansion-kit-only/" target="_blank" rel="noopener noreferrer">Expansion Kit</a> contains all the items in the <a href="https://www.modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-planetary-and-nir-imaging-camera/" target="_blank" rel="noopener noreferrer">standard kit</a> plus a quality Methane (CH4) filter and All Sky Lens.</p>
<p>List of contents:</p>
<ul>
<li>QHY QHY5III462 USB 3.0 CMOS Colour Imaging Camera in storage tin</li>
</ul>
<ul>
<li>1.25&#8243; UV/IR Cut Filter</li>
</ul>
<ul>
<li>1.25&#8243; IR850 Filter</li>
</ul>
<ul>
<li>USB Cable</li>
</ul>
<ul>
<li>Guide Cable</li>
</ul>
<ul>
<li>Focus Locking Ring</li>
</ul>
<ul>
<li>C-Mount Adapter</li>
</ul>
<ul>
<li>1.25&#8243; 10nm Methane Filter (890nm) &#8211; <a href="https://www.planetary-astronomy-and-imaging.com/en/making-methane-images-jupiter/" target="_blank" rel="noopener noreferrer">info</a> &#8211; <a href="https://britastro.org/journal_item/8975" target="_blank" rel="noopener noreferrer">more info</a></li>
</ul>
<ul>
<li>Wide Angle All-Sky Lens</li>
</ul>
<ul>
<li>CS Mount Lens Adapter</li>
</ul>
<h3></h3>
<h3>Superb NIR response &#8211; High QE 800-1000nm</h3>
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<h3 class="revealOnScroll animated fadeInUp" data-animation="fadeInUp">Monochrome at NIR</h3>
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<p>The QHY5III462C Camera and <a href="https://www.modernastronomy.com/shop/accessories/lenses/qhy5iii462c-expansion-kit-only/" target="_blank" rel="noopener noreferrer">Expansion Kit</a> uses Sony&#8217;s latest generation IMX462 back-illuminated sensor with extended red and near infrared response. It has nearly double the red and NIR sensitivity as previous generation BSI sensors and even greater sensitivity compared to front illuminated sensors. Because the RGB filters become transparent at NIR wavelengths, the camera captures RGB colour images in visible light and monochrome images in NIR.</p>
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<h3 class="revealOnScroll animated fadeInUp" data-animation="fadeInUp">Super High Conversion Gain &#8211; Boosts Low Light Sensitivity</h3>
<h3 class="revealOnScroll animated fadeInUp" data-animation="fadeInUp">0.5e- Read Noise!</h3>
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<p>Sony&#8217;s new sHCG (Super High Conversion Gain) technology produces a higher voltage from fewer photons resulting in greater sensitivity even at very low levels of light. With sHCG technology, even in visible light, the QHY5III462C has higher sensitivity than the back-illuminated IMX290 based cameras.</p>
</div>
</div>
</div>
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<h3 class="revealOnScroll animated fadeInUp" data-animation="fadeInUp">High Frame Rate &#8211; 135FPS</h3>
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<p>To produce the highest detail with the greatest dynamic range, many planetary imagers prefer to capture hundreds or thousands of images in as short a time as possible and then process the results into one final combined image. This requires high sensitivity for short exposures and low read noise for combining multiple images. The QHY5III462C will output 135 frames per second at full resolution. With its exceptionally high QE and extraordinarily low (0.5e-) read noise, it is the perfect camera for planetary imaging.</p>
</div>
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<h3 class="revealOnScroll animated fadeInUp" data-animation="fadeInUp">Filters for Visible and IR Imaging &#8211; IR850 for NIR, UV-IR for Colour</h3>
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<p>The QHY5III462C comes with two free 1.25-inch filters. The IR850 filter is a long wavelength pass filter that allows wavelengths &gt; 850nm to pass through. The UV/IR filter passes visible light and blocks the NIR. With these two filters you can capture both RGB colour images and NIR monochrome images with the same camera. At NIR wavelengths, the RGB filters become transparent and the camera behaves like a monochrome IR camera.</p>
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<h3>Best for Beginners &#8211; Reasonable price, Multiple functions</h3>
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<dl>
<dt><img decoding="async" src="https://www.qhyccd.com/uploadfile/2020/0730/20200730032023776.png" /></dt>
<dd>
<h2>IR850 Filter</h2>
<p>Special for NIR photography or monochrome shots</dd>
</dl>
<dl>
<dt><img decoding="async" src="https://www.qhyccd.com/uploadfile/2020/0730/20200730032220272.png" /></dt>
<dd>
<h2>IR/Cut Filter</h2>
<p>For normal astrophotography when using 462C as colour camera.</dd>
</dl>
<dl>
<dt><img decoding="async" src="https://www.qhyccd.com/uploadfile/2020/0730/20200730032339300.png" /></dt>
<dd>
<h2>IR890 CH4 filter</h2>
<p>In Expansion Kit&#8211;CH4 filter is useful for Saturn and Jupiter imaging.</dd>
</dl>
</div>
</div>
</div>
<p>The post <a href="https://modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-camera-and-expansion-kit/">QHY5III462C Camera and Expansion Kit</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<title>QHY600 Mono Full Frame Cooled CMOS Camera</title>
		<link>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy600-mono-full-frame-cooled-cmos-camera/</link>
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		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Fri, 19 Jun 2020 22:31:57 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=90578</guid>

					<description><![CDATA[<p>The QHY600 Mono Full Frame Cooled CMOS Camera uses the latest SONY IMX455 back-illuminated sensor, a full frame (35mm format) sensor with 3.76um pixels and native 16-bit A/D. This listing is for the latest short back focus version.</p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy600-mono-full-frame-cooled-cmos-camera/">QHY600 Mono Full Frame Cooled CMOS Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<p>The QHY600 Mono Full Frame Cooled CMOS Camera uses the latest SONY IMX455 back-illuminated sensor, a full frame (35mm format) sensor with 3.76um pixels and native 16-bit A/D. This sensor is available in both monochrome and color versions. The sensor size is 36mm x 24mm. With the round body design, the QHY600 is an ideal camera to match the image circle of the new generation of RASA telescopes.</p>
<p><span style="font-family: arial, verdana, helvetica;">The new Sony sensor used in the QHY600 has native 16-bit A/D on-chip. The output is real 16 bit with 65536 levels. Compared to 12-bit and 14-bit A/D, a 16-bit A/D yields higher sample resolution and the system gain will be less than 1e-/ADU with no sample error noise and very low read noise. This leads to the possibility of images with superb dynamic range.</span></p>
<p><span style="font-family: arial, verdana, helvetica;">One benefit of the back-illuminated CMOS structure is improved full well capacity. This is particularly helpful for sensors with small pixels. Even unbinned, the QHY600 has a full well capacity of more than 51ke-. When binned 2&#215;2 to 7.5um the full well is 196ke- and when binned 3&#215;3 to 11um the full well is 441ke-</span></p>
<p><span style="font-family: arial, verdana, helvetica;">The QHY600 has only one electron of read noise at high gain / full resolution and a 4FPS readout speed. One electron of read noise means the camera can achieve a SNR&gt;3dB at only 4 to 6 photons. This is perfect performance when conditions are photon limited, i.e., short exposures, narrow band imaging, etc. This makes the sensor ideal for sky surveys, time domain astronomy, fluorescence imaging, DNA sequencing and microscopy.</span></p>
<p>In order to provide smooth uninterrupted data transfer of the entire 60MP sensor at high speed, the QHY600 has <strong>2GB</strong> DDR3 image buffer. In addition the camera features a USB3.0 interface for transmission of data at high speed.</p>
<p><strong>Specifications</strong></p>
<p><strong>Model</strong> QHY600 PH (QHY600U3G20M) Mono</p>
<p><strong>Image Sensor</strong> SONY Full Frame BSI CMOS Sensor IMX455</p>
<p><strong>Pixel Size</strong> 3.76µm x 3.76µm Mono</p>
<p><strong>Sensor Surface Glass</strong> AR+AR Multi-Coated</p>
<p><strong>Sensor Type</strong> Back-Illuminated (BSI)</p>
<p><strong>Effective Pixels</strong> 61.17 Megapixels 9576 x 6388 effective area (9600 x 6422 with overscan and optically black area)</p>
<p><strong>Effective Image Area</strong> 36mm x 24mm</p>
<p><strong>Full Well Capacity</strong> (1&#215;1, 2&#215;2, 3&#215;3) Standard Mode &gt;51ke- / &gt;204ke- / &gt;408ke- Extend Full Well Mode &gt;80ke- / &gt;320ke- / &gt;720ke-</p>
<p><strong>A/D 16-bit</strong> (0-65535 levels) at 1&#215;1 binning 18-bit at 2&#215;2, 19-bit at 3&#215;3, 20-bit at 4&#215;4 software binning *QHY600 uses software digital binning for 2x2binning. With digital sum, 2x2binning will be four 16-bit summed then it is 18-bit.</p>
<p><strong>Sensor Size</strong> Full Frame Format (36mm x 24mm)</p>
<p><strong>Image Transfer Speed</strong></p>
<p>Full Frame Size: 4.0FPS (8-bit output)</p>
<p>Full Frame Size: 2.5FPS (16-bit output)</p>
<p>7.2FPS at 9600 x 3194</p>
<p>22.5FPS at 9600 x 1080</p>
<p>28FPS at 9600 x 768</p>
<p>47FPS at 9600 x 480</p>
<p>160FPS at 9600 x 100,</p>
<p><strong>Read Noise</strong> 1.0e- to 3.7e- (Standard Mode)</p>
<p><strong>Dark Current</strong> 0.0032e-/p/s @ -20C 0.0056e-/p/s @ -10C</p>
<p><strong>Exposure Time Range</strong> 40µs &#8211; 3600sec</p>
<p><strong>Firmware/FPGA remote Upgrade Supported</strong>. Via Camera USB Port</p>
<p><strong>Shutter Type</strong> Electric Rolling Shutter</p>
<p><strong>Computer Interface</strong> USB3.0</p>
<p><strong>Built-in Image Buffer </strong>1GBytes（8Gbit）/ 2GBytes（16Gbit）DDR3 memory Non-volatile memory / On camera storage Build-in total 64MByte Flash Memory. 10MBytes user-accessible space for stellar ROI frames for analysis of exoplanet investigation, occultations, atmospheric seeing measurement, focus, optical analysis, etc. Supports 100*100 image x 500 frames, 50*50 image x 4000 frames, 25*25 image x16000 frames, 10*10 image x 250000 frames</p>
<p><strong>Cooling System</strong> Dual Stage TEC cooler: &#8211; Long exposures (&gt; 1 second) typically -35C° below ambient &#8211; Short exposure (&lt; 1second) high FPS, typically -30C° below ambient</p>
<p><strong>Water Cooling Version</strong> Available optionally. QHYCCD can offer this version. Contact us for more details</p>
<p><strong>Anti-Dew Heater</strong> Yes</p>
<p><strong>Telescope Interface</strong> M54/0.75</p>
<p><strong>Optic Window Type</strong> AR+AR High Quality Multi-Layer Anti-Reflection Coating</p>
<p><strong>Power</strong> 40W/100% 20W/50% 13.8W/0%</p>
<p><strong>Back Focal Length</strong> 12.5mm (±0.2mm).</p>
<p><strong>Weight</strong> (net) Photographic Version: 837g (not including the M54/0.75mm center/tilt adjust ring)</p>
<p>NB. This listing is for the latest short back focus version.</p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy600-mono-full-frame-cooled-cmos-camera/">QHY600 Mono Full Frame Cooled CMOS Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<title>Revolution Imager All Sky Lens</title>
		<link>https://modernastronomy.com/shop/accessories/lenses/revolution-imager-all-sky-lens/</link>
					<comments>https://modernastronomy.com/shop/accessories/lenses/revolution-imager-all-sky-lens/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Sat, 02 Nov 2019 14:10:04 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=83836</guid>

					<description><![CDATA[<p>The Revolution Imager All Sky lens allows you to image wide areas (150°) of sky. Perfect for capturing images of the milky way. Combined with a <a title="USB Capture Device" href="https://www.modernastronomy.com/shop/accessories/astro-video-accessories/revolution-imager-usb-video-capture-adapter/">USB Capture Device</a> and powerful software like <a href="http://www.sharpcap.co.uk/">SharpCap</a> or <a href="https://www.azcendant.com/HandyAviOverview.html">HandyAvi</a> you can easily setup a time-lapse for meteors and satellites.</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/lenses/revolution-imager-all-sky-lens/">Revolution Imager All Sky Lens</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<p>The Revolution Imager All Sky lens allows you to image wide areas of the sky (150 degrees) using the powerful sensitivity of the Revolution Imager. Perfect for capturing images of the milky way, constellations, meteors and satellites! When combined with a <a title="USB Capture Device" href="https://www.modernastronomy.com/shop/accessories/astro-video-accessories/revolution-imager-usb-video-capture-adapter/">USB Capture Device</a> and powerful software like <a href="http://www.sharpcap.co.uk/">SharpCap</a> you can easily setup a time-lapse for meteors and satellites or see the constellations move across the night sky! Software such as <a href="https://www.azcendant.com/HandyAviOverview.html">HandyAvi</a> can be used for motion detection, surveillance and animation.</p>
<p>Specifications:</p>
<ul>
<li>Focal Length: 2.1mm</li>
<li>Focal Ratio: f/1.2</li>
<li>Field-of-View (with Revolution Imager R2) =150 degrees</li>
</ul>
<p>Field of view is less than 180 degrees with this lens, as few of us enjoy a complete view of the sky. Moreover light pollution and haze are often visible near the horizon. However if you&#8217;d like a lens that gives a full 180 degree view (in fish eye format) with the Revolution Imager R2 and other 1/3&#8243; format cameras please choose the <a href="https://www.modernastronomy.com/shop/accessories/qhy-accessories/all-sky-lens-for-qhy5l-ii-cameras/">All Sky Lens for QHY5L-II Cameras</a>.</p>
<p>The post <a href="https://modernastronomy.com/shop/accessories/lenses/revolution-imager-all-sky-lens/">Revolution Imager All Sky Lens</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<title>QHY247C APS-C Camera</title>
		<link>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy247-aps-c-camera/</link>
					<comments>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy247-aps-c-camera/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Tue, 17 Sep 2019 12:34:25 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=81937</guid>

					<description><![CDATA[<p>The QHY247C APS-C Camera uses a SONY IMX193 APS size color CMOS sensor. Pixel size is 3.91um and it has a 14-bit A/D with a full well capacity of 36ke-. The read noise is 1e- to 2.7e-, the lowest tested noise at the lowest gain in the entire QHYCCD COLDMOS product line making it ideal for stacking many short exposures.</p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy247-aps-c-camera/">QHY247C APS-C Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<p><strong>Ultra High Performance</strong><br />
QHY247C APS-C Camera has a APC-S 24mega pixels, 14bit CMOS sensor IMX193. This sensor is also used in the D5300 and D5500 camera. It has 2.7e low readout noise at lowest gain and 2.2e low readout noise at unity gain(system gain = 1e/adu), and 1.0e at high gain. QHY247C is camera with lowest readout noise and thermal noise in the QHY165C/168C/247C/367C production line.</p>
<p><strong>True RAW Image Output</strong><br />
QHY247C APS-C Camera has the same CMOS sensor like D5300/D5500.But D5300 only offer 13bit and both D5300 and D5500 is not really RAW output even it is &#8220;RAW&#8221; format. You will find the de-noise sign on the raw images from the hot pixel styles in the DSLR dark frames. While the QHY247C offers the TRUE RAW IMAGE OUTPUT and it gives original signal and keep the max flexibility of astronomy image process.</p>
<p><strong>Unique Thermal Noise Reduction Technology</strong><br />
Besides the 2-stage TEC, QHYCCD has an unique thermal noise control technology to get the cmos sensor very low thermal noise and make whole 165/168/247/367 product line has much better thermal noise performance than competitors.</p>
<p><strong>128MB DDRII Image Buffer</strong><br />
QHY247C has 128MB DDRII image buffer to help the image cache to avoid the risk of frame lost. The data will store in the DDR for first then transfer to computer. It will avoid the USB port too busy when there is more USB3.0 camera connected.</p>
<p><strong>Anti-Dew Technology</strong><br />
With the long time experience on the cooled CCD camera design. QHYCCD has the fully anti-dew technology for both CCD sensor surface glass and the optic window glass. QHY247C has the electric heating board for the CCD glass windows to prevent the window get dew and the silicon gel tube socket design for control the humidity within CMOS chamber.</p>
<p><strong>AR+AR optic window</strong><br />
In order to avoid the halo around the bright star. The QHY247C has a AR+AR coating optic window rather than the common IR cut window for OSC color cameras. So you need to use your own IR cut filter (most L filter can do that) on front of the camera. You can install the 2inch filter on the M48 thread of the 2inch T ring. Or  QHYCCD supplies an optional 2inch filter holder for QHY247C to allow you put this filter when connecting with a flat field</p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy247-aps-c-camera/">QHY247C APS-C Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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		<title>QHY367C Full Frame Camera</title>
		<link>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy367c-full-frame-camera/</link>
					<comments>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy367c-full-frame-camera/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Wed, 23 Aug 2017 13:56:00 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=73043</guid>

					<description><![CDATA[<div align="justify">
<p align="justify">The QHY367C full frame cooled CMOS camera uses the Sony IMX094 36 megapixel, 14bit sensor. This sensor is also used in the Nikon D810A camera. Readout noise is 3.2e at lowest gain and 2.4e at unity gain. Dynamic range is &#62; 14 Stops.</p>
<div align="justify">
<h4><a href="http://www.skyatnightmagazine.com/review/camera/qhyccd-qhy367c-cmos-colour-camera">Sky at Night review</a></h4>
</div>
</div>
<div align="justify"></div>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy367c-full-frame-camera/">QHY367C Full Frame Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
]]></description>
										<content:encoded><![CDATA[<div align="justify"><strong>The QHY367C full frame cooled CMOS camera</strong> uses the Sony IMX094 36 megapixel, 14bit sensor. This sensor is also used in the Nikon D810A camera. Readout noise is 3.2e at lowest gain and 2.4e at unity gain. Dynamic range is &gt; 14 Stops.</div>
<div align="justify"><span class="ws12" style="color: #535353;"> </span></div>
<div align="justify"><span class="ws16" style="color: #333399;"><b>True RAW Image Output</b></span></div>
<div align="justify"><span class="ws12" style="color: #535353;">Although many DSLRs claim RAW image output, often it is not true. You will find signs of denoising in the images from removal of hot pixels. However the QHY367C offers TRUE RAW IMAGE OUTPUT and preserves the original signal to retain maximum flexibility for image processing.</span></div>
<div align="justify"><span class="ws12" style="color: #535353;"> </span></div>
<div align="justify"><span class="ws16" style="color: #333399;"><b>Unique Thermal Noise Reduction Technology</b></span></div>
<div align="justify"><span class="ws12" style="color: #535353;">Besides the 2-stage TEC, QHYCCD has unique thermal noise control technology to achieve very low noise to make the whole 165/168/247/367 product line have much better thermal noise performance than any other competitor.</span></div>
<div align="justify"><span class="ws12" style="color: #535353;"> </span></div>
<div align="justify"><span class="ws16" style="color: #333399;"><b>128MB DDRII Image Buffer</b></span></div>
<div align="justify"><span class="ws12" style="color: #535353;">QHY367C has a 128MB DDRII image buffer to avoid the risk of frame loss. Data is stored in the buffer first then transferred to the PC. This avoids issues when the USB port is busy when other USB3.0 cameras are connected.</span></div>
<div align="justify"><span class="ws12" style="color: #535353;"> </span></div>
<div align="justify"><span class="ws16" style="color: #333399;"><b>Anti-Dew Technology</b></span></div>
<div align="justify"><span class="ws12" style="color: #535353;">With long time experience of cooled CCD camera design. QHYCCD has full anti-dew technology for both the CCD sensor surface and the optical window. QHY367C has an electric heating board for the glass windows, to prevent misting, and a silica gel system to control humidity within the CMOS chamber.</span></div>
<div align="justify"><span class="ws12" style="color: #535353;"> </span></div>
<div align="justify"><span class="ws16" style="color: #333399;"><b>AR+AR optic window</b></span></div>
<div align="justify"><span class="ws12" style="color: #535353;">In order to avoid halos around bright stars, the QHY367C Full Frame Camera has a AR+AR coating optic window rather than the common IR cut window for colour cameras. You will need to use your own IR cut filter on front of the camera. A 2 inch filter holder is available for installing the IR-cut filter. </span></div>
<div align="justify"></div>
<div align="justify"></div>
<div align="justify">
<table border="0" cellspacing="0" cellpadding="5" bgcolor="#EBEBEB">
<tbody>
<tr valign="top">
<td colspan="2" bgcolor="#000000">
<div class="wpmd">
<div><span class="ws11" style="color: #ffffff;"><b>QHY367C Specification</b></span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11" style="color: #000000;">CMOS Sensor</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11" style="color: #000000;">SONY IMX094 COLOUR CMOS</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">CMOS Size</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">36mm x 24mm full frame</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Effective Pixel</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">7376*4938    36.4 megapixel</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Photosensitive Area</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">36.0 x 24.1mm</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Pixel Size</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">4.88um x 4.88um</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Full Well</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">56ke-</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Readout Type</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">Progressive Scan</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Shutter</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">Electric rolling shutter</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Exposure Time</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">60us-3600 sec</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Max Frame Rate</span></div>
<div><span class="ws11">(for both 8bit and 14bit)</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">3.2FPS@Full Resolution</span></div>
<div><span class="ws11">7FPS@2160 LINES  (eg. 7400*2160, 4096*2160 etc)</span></div>
<div><span class="ws11">14</span><span class="ws11">FPS@1080 LINES (eg. 7400*1080,1920*1080 etc)</span></div>
<div><span class="ws11">19FPS@768 LINES</span></div>
<div><span class="ws11">30FPS@480 LINES</span></div>
<div><span class="ws11">40FPS@320 LINES</span></div>
<div><span class="ws11">83FPS@100 LINES (eg.7400*100)</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Pixel Binning</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">1*1</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Peak QE</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">TBD</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">AD Converter</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">14BIT</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Readout Noise</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">3.2e @ Low gain. 2.4e @ unity gain</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div>Maximum Dynamic Range</div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">More than 17000. &gt;14 Stops</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Mechanical Interface</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">M54/0.75 female thread  see mechanical drawing</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Optical window heater</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">Yes</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">TEC</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">2-stage TEC. -35C below ambient</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Optical Glass Window</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">AR+AR Clear glass</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200" height="15">
<div class="wpmd">
<div><span class="ws11">Silicon gel socket</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424" height="15">
<div class="wpmd">
<div><span class="ws11">Yes</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Weight(Camera only)</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">788g</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td bgcolor="#FFFFFF" width="200">
<div class="wpmd">
<div><span class="ws11">Power Consumption</span></div>
</div>
</td>
<td bgcolor="#FFFFFF" width="424">
<div class="wpmd">
<div><span class="ws11">About 30 Watts @ 100% Cooling and 13 Watts @ 50%</span></div>
</div>
</td>
</tr>
<tr valign="top">
<td width="200">
<div class="wpmd">
<div><span class="ws11">Electric interface</span></div>
</div>
</td>
<td width="424">
<div class="wpmd">
<div><span class="ws11">USB3 12V DC Power socket with lock (2.1 mm)</span></div>
</div>
</td>
</tr>
</tbody>
</table>
</div>
<div align="justify"></div>
<div align="justify"><a href="http://www.skyatnightmagazine.com/review/camera/qhyccd-qhy367c-cmos-colour-camera">Sky at Night review</a></div>
<div align="justify"></div>
<div align="justify"><a href="http://www.qhyccd.com/index.php?m=content&amp;c=index&amp;a=show&amp;catid=94&amp;id=10">Manufacturers website presentation</a></div>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy367c-full-frame-camera/">QHY367C Full Frame Camera</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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