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We consider a dynamic panel AR(1) model with Öxed e§ects when both n and T are large. It is shown that the MLE motivated by the random e§ects assumption is asymptotically unbiased even when the ...
We consider a dynamic panel AR(1) model with fixed effects when both n and T are large. Under the “T fixed n large” asymptotic approximation, the ordinary least squares (OLS) or Gau...
Wind buffeting of large telescopes     Wind buffeting  large telescopes       font style='font-size:12px;'> 2015/5/13
Wind buffeting of large telescopes.
Analysis of normalized point source sensitivity as a performance metric for large telescopes.
A wide-band current preamplifier based on a composite operational amplifier is proposed. It has been shown that the bandwidth of the preamplifier can be significantly increased by enhancing the effect...
Abstract: We have built a RICH detector prototype consisting of a liquid C6F14 radiator and six triple Thick Gaseous Electron Multipliers (TGEMs), each of them having an active area of 10x10 cm2. One ...
Abstract: We present results on quasidiffusion studies in large, 3 inch diameter, 1 inch thick [100] high purity germanium crystals, cooled to 50 mK in the vacuum of a dilution refrigerator, and expos...
Large Scales - Long Times: Adding High Energy Resolution to SANS     MIEZE  NSE  Resolution function  ESS       font style='font-size:12px;'> 2011/8/3
Abstract: The Neutron Spin Echo (NSE) variant MIEZE (Modulation of IntEnsity by Zero Effort), where all beam manipulations are performed before the sample position, offers the possibility to perform l...

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