信噪比 - 版本历史

2016年2月18日 (四) 08:21 Shen

2016-02-18T08:21:29Z

←上一版本		2016年2月18日 (四) 08:21的版本
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	*常见[http://www.ucolick.org/~bolte/AY257/s_n.pdf]		*参见[http://www.ucolick.org/~bolte/AY257/s_n.pdf]
	*The signal-to-noise ratio of an observation is:		*The signal-to-noise ratio of an observation is:
	s/n = Ct/[sqrt(sigma^2n+t(C-A*S))]		s/n = Ct/[sqrt(sigma^2n+t(C-A*S))]

2016年2月18日 (四) 08:21 Shen

2016-02-18T08:21:05Z

←上一版本		2016年2月18日 (四) 08:21的版本
第1行：		第1行：
			*常见[http://www.ucolick.org/~bolte/AY257/s_n.pdf]
	*The signal-to-noise ratio of an observation is:		*The signal-to-noise ratio of an observation is:
	s/n = Ct/[sqrt(sigma^2n+t(C-A*S))]		s/n = Ct/[sqrt(sigma^2n+t(C-A*S))]

2013年12月18日 (三) 12:08 Shen

2013-12-18T12:08:28Z

←上一版本		2013年12月18日 (三) 12:08的版本
第1行：		第1行：
	The signal-to-noise ratio of an observation is:		*The signal-to-noise ratio of an observation is:
	s/n = Ct/[sqrt(sigma^2n+t(C-A*S))]		s/n = Ct/[sqrt(sigma^2n+t(C-A*S))]
	where C is the count rate from the object (photons per second), t the exposure time, sigma the read-out noise of each pixel, n the number of pixels on which the image falls, S the number of photons from the sky per unit solid angle, and A the solid angle subtended by the image.		where C is the count rate from the object (photons per second), t the exposure time, sigma the read-out noise of each pixel, n the number of pixels on which the image falls, S the number of photons from the sky per unit solid angle, and A the solid angle subtended by the image.

	Through-put Measurements and SNR[http://www.noao.edu/kpno/manuals/l2mspect/node12.html]		*Through-put Measurements and SNR[http://www.noao.edu/kpno/manuals/l2mspect/node12.html]

			*[http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand/HTML/W2_61.html]

Shen：以“The signal-to-noise ratio of an observation is: s/n = Ct/[sqrt(sigma^2n+t(C-A*S))] where C is the count rate from the object (photons per second), t the exposure ...”为内容创建页面

2013-12-18T11:35:59Z

以“The signal-to-noise ratio of an observation is: s/n = Ct/[sqrt(sigma^2*n+t*(C-A*S))] where C is the count rate from the object (photons per second), t the exposure ...”为内容创建页面

新页面

The signal-to-noise ratio of an observation is:
s/n = Ct/[sqrt(sigma^2*n+t*(C-A*S))]
where C is the count rate from the object (photons per second), t the exposure time, sigma the read-out noise of each pixel, n the number of pixels on which the image falls, S the number of photons from the sky per unit solid angle, and A the solid angle subtended by the image.

Through-put Measurements and SNR[http://www.noao.edu/kpno/manuals/l2mspect/node12.html]

信噪比 - 版本历史

2016年2月18日 (四) 08:21 Shen

2016年2月18日 (四) 08:21 Shen

2013年12月18日 (三) 12:08 Shen

Shen：​以“The signal-to-noise ratio of an observation is: s/n = Ct/[sqrt(sigma^2*n+t*(C-A*S))] where C is the count rate from the object (photons per second), t the exposure ...”为内容创建页面

Shen：以“The signal-to-noise ratio of an observation is: s/n = Ct/[sqrt(sigma^2n+t(C-A*S))] where C is the count rate from the object (photons per second), t the exposure ...”为内容创建页面