نتایج جستجو برای: rx detector

تعداد نتایج: 62020  

Journal: :وقایع علوم کاربردی ورزش 0
korkut ulucan üsküdar univerity, haluk turksoy sok. no:14, altunizade, üsküdar, i̇stanbul, turkey. marmara university, basibuyuk yolu 9/3 maltepe saglık yerleşkesi, maltepe, istanbul, turkey betul biyik üsküdar univerity, haluk turksoy sok. no:14, altunizade, üsküdar, i̇stanbul, turkey sezgin kapici üsküdar univerity, haluk turksoy sok. no:14, altunizade, üsküdar, i̇stanbul, turkey canan sercan marmara university, basibuyuk yolu 9/3 maltepe saglık yerleşkesi, maltepe, istanbul, turkey oznur yilmaz üsküdar univerity, haluk turksoy sok. no:14, altunizade, üsküdar, i̇stanbul, turkey tunc catal üsküdar univerity, haluk turksoy sok. no:14, altunizade, üsküdar, i̇stanbul, turkey

actins are small globular filaments functioning in cell processes like muscle contraction, and stabilized to the sarcomeric z- discs by actin binding proteins (actinins). one of the important gene coding for actin binding proteins in fast twitch fibers is alpha- actinin- 3 (actn3). in this research, we have conducted a gene profile study investigating the genotype and allele distributions of ac...

2010
J. P. EVANS J. L. WALSH

and let the function f(z) be analytic in these points. To study the convergence to f(z) of the sequence of functions gn(z); here gn(z) is analytic throughout Rx, coincides with f(z) in the points 0nl, 0n2, • • • , 0nn, and among all functions with these two properties has the least norm in Rx. This problem has been previously studied [6; 7] where norm is [lub |g„(z)|, z in A\], and is now to be...

2002
C. Mei L. Zhang Z. J. Jiang B. Z. Dai

Using the sample of radio selected BL Lacer-tae objects (RBLs) and X-ray selected BL Lacertae objects (XBLs) presented by Sambruna et al. (1996), we calculated the luminosities of radio, optical and X-ray of each source and made the statistical analysis among the luminosities at different wave-bands, broad-band spectral indices from radio to X-ray (α rx) and peak frequencies (ν p). Our results ...

2014
Feng Gu Yun Yin Yisheng Song

and Applied Analysis 3 Moreover, if the pairs (f, R), (g, S), and (h, T) are weakly compatible, then f, g, h, R, S, and T have a unique common fixed point in X. Proof. First, we suppose that the subspace RX is closed inX, fX ⊆ SX, gX ⊆ TX, and two pairs of (f, R) and (g, S) satisfy common (E.A) property.Then by Definition 11 we know that, there exist two sequences {x n } and {y n } inX such tha...

Journal: :Family medicine 2011
Katherine Hurst

Journal: :IEEE Access 2021

In this letter, a wireless power transfer (WPT) system based on two high-impedance coil (HIC) - cable loop antennas with modified shield as transmitters (Tx)s and spiral receiver (Rx) is proposed discussed. Utilizing features of HIC at its parallel-circuit resonance frequency, we design the Tx in way that absence Rx, input impedance very high compared to case when Rx near Tx. This feature offer...

Journal: :Optometry 2000
P F Vinger T A Woods

OBJECTIVES To determine if a plano lens could be the test lens for all prescription (Rx) lenses and to investigate why Rx lenses pop out of safety eyewear. DESIGN Plano and Rx polycarbonate lenses (n = 641) with varying thickness and edge geometry, mounted on steel lens holders, and Rx safety eyewear (n = 128) placed on headforms were impacted with test objects of varying diameter and hardnes...

2001
G. P. Garmire M. W. Bautz

The mini Broad Absorption Line (BAL) quasar RX J0911.4+0551 was observed with the Advanced CCD Imaging Spectrometer (ACIS) of the Chandra X-ray Observatory for ∼ 29 ks as part of a gravitational lens (GL) survey aimed at measuring time-delays. Timing analysis of the light-curve of the lensed image A2 shows a rapid flux variation with a duration of about 2000s. A Kolmogorov-Smirnov test shows th...

2008
MARCEL BERGMANN

We present the Fundamental Plane (FP) in the z = 0.28 cluster of galaxies RX J0142.0+2131. There is no evidence for a difference in the slope of the FP when compared with the Coma cluster, although the internal scatter is larger. On average, stellar populations in RX J0142.0+2131 have rest-frame V -band mass-to-light ratios (M/LV ) 0.29± 0.03 dex lower than in Coma. This is significantly lower ...

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