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	<title>QHY183M Archives - Modern Astronomy</title>
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		<title>QHY183M</title>
		<link>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy183m/</link>
					<comments>https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy183m/#respond</comments>
		
		<dc:creator><![CDATA[Bernard Karpinski]]></dc:creator>
		<pubDate>Fri, 02 Feb 2018 10:35:05 +0000</pubDate>
				<guid isPermaLink="false">https://www.modernastronomy.com/?post_type=product&#038;p=76431</guid>

					<description><![CDATA[<p><span class="ws12" style="color: #3c3c3c;">QHY183M is a one-inch, 20 Megapixel back-illuminated COLDMOS camera with 2.4um pixels. The camera is capable of producing 15FPS @ 20 Mpxs.  The two-stage TEC cools the sensor to 40C to 45C below ambient.  ADC is 10/12-bit and output is 8/12-bit with 1e- read noise!  </span></p>
<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy183m/">QHY183M</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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										<content:encoded><![CDATA[<div align="justify"><span class="ws12" style="color: #3c3c3c;">The QHY183M is a one-inch, 20 Megapixel back-illuminated COLDMOS camera.  Pixel size is 2.4um for high-resolution. The camera is capable of producing 15FPS @ 20 Megapixels.  It has a two-stage TEC that cools the sensor to -40C to -45C below ambient.  ADC is 10/12-bit and 8/12-bit output with 1e- read noise!  Computer interface is USB 3.0 and exposure times can be set from 50us to 3600 sec.  </span></div>
<div><span class="ws12" style="color: #3c3c3c;"> </span></div>
<div><span class="ws12" style="color: #3c3c3c;"><b>128MB DDR Buffer</b></span></div>
<div><span class="ws12" style="color: #3c3c3c;">The QHY183M has a built-in 128MB DDRII image buffer. The benefit of the image buffer is that the memory will cache the image and transfer it to the computer when the USB interface is not busy or being interrupted, and the frame will not be lost or corrupted.  This buffer also allows a slower computer with USB 2.0 socket to capture every frame without loss even if the USB socket is occasionally busy with other peripherals.  This buffer also helps multiple camera applications and avoids USB transfer problems.  For example, it is possible to operate four QHY183M cameras on the same computer to create an LRGB imaging array.</span></div>
<div><span class="ws12" style="color: #3c3c3c;"> </span></div>
<div><span class="ws12" style="color: #3c3c3c;"><b>Full Anti-Dew Solution</b></span></div>
<div><span class="ws12" style="color: #3c3c3c;">With more than a decade of experience designing cooled cameras, QHYCCD has applied this knowledge to the QHY183M camera.  The full anti-dew technology includes a sealed CMOS chamber with silicon gel tube socket and a heated chamber optical window.  This technology prevents dew from forming on the sensor itself, or on the chamber window, even in a high humidity environment.</span></div>
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<div>
<div align="justify"><span class="ws12" style="color: #3c3c3c;"><i>Sony&#8217;s Image Sensor </i></span><span class="ws12" style="color: #3c3c3c;"><b><i>Exmor R</i></b></span><span class="ws12" style="color: #3c3c3c;"><i> is a back-illuminated CMOS image sensor with improved sensitivity and noise reduction &#8211; the key factors to enhancing image quality, while radically realigning their fundamental pixel structure from front-illumination to back-illumination. It retains the advantages of CMOS image sensors such as low power consumption and high-speed operation while dramatically improving sensitivity.  With a conventional front-illumination structure, the metal wiring and transistors on the surface of the silicon substrate that form the sensor&#8217;s light-sensitive area (photo-diode) impede photon gathering carried out by the on-chip lens, and this has also been an important issue in the miniaturization of pixels and widening optical angle response.</i></span></div>
<div align="justify"><span class="ws12" style="color: #3c3c3c;"><i> </i></span></div>
<div align="justify"><span class="ws12" style="color: #3c3c3c;"><i>A back-illuminated structure minimizes the degradation of sensitivity to optical angle response, while also increasing the amount of light that enters each pixel due to the lack of obstacles such as metal wiring and transistors that have been moved to the reverse of the silicon substrate.  However, compared to conventional front-illuminated structures, back-illuminated structures have historically caused problems such as noise, dark current, defective pixels and color mixture that lead to image degradation and also cause a decrease in the signal-to-noise ratio  To overcome this Sony newly developed a unique photo-diode structure and on-chip lens optimized for back-illuminated structures that achieves a higher sensitivity and a lower random noise without light by reducing noise, dark current and defect pixels compared to the conventional front-illuminated structure.  Additionally, Sony&#8217;s advanced technologies such as high-precision alignment have addressed any color mixture problems.</i></span></div>
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<p>The post <a href="https://modernastronomy.com/shop/cameras/cooled-ccd/qhy-cooled-ccd-cameras/qhy183m/">QHY183M</a> appeared first on <a href="https://modernastronomy.com">Modern Astronomy</a>.</p>
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