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Hiroshi Nishi, Akihiro Tojo, Maristela Lika Onozato, Rika Jimbo, Masaomi Nangaku, Hiroshi Uozaki, Kenji Hirano, Hiroyuki Isayama, Masao Omata and Shinya Kaname Nephrol Dial Transplant 2007; 22: 1273–1275; doi:10.1093/ndt/gfl672 In the above article, the name of the last author (Toshiro Fujita) was omitted. The correct author list should read as follows: Hiroshi Nishi, Akihiro Tojo, Maristela Li...
EXOMARS ROVER PANCAM PROTOTYPE. R. Li, D. Li, K. Di, G. Paar, A. Coates, J. P. Muller, A. Griffiths, J. Oberst, and D. P. Barnes. Mapping and GIS Laboratory, CEGE, The Ohio State University, 470 Hitchcock Hall, 2070 Neil Ave., Columbus, OH 43210-1275, USA, [email protected]; Institute for Information and Communication Technologies, Joanneum Research, Graz, Austria; Mullard Space Science Laboratory...
We report on the search for spectral irregularities induced by oscillations between photons and axionlike-particles (ALPs) in the γ-ray spectrum of NGC 1275, the central galaxy of the Perseus cluster. Using 6 years of Fermi Large Area Telescope data, we find no evidence for ALPs and exclude couplings above 5×10^{-12} GeV^{-1} for ALP masses 0.5≲m_{a}≲5 neV at 95% confidence. The limits are co...
The Great Recession of 2007-2009 is regarded as the most severe economic downturn since World War II. This study examined relationships between reported recession hardships and physical health in a national survey of American adults (N = 1275). Furthermore, education and psychological resources (perceived control, purpose in life, and conscientiousness) were tested as moderators of the health i...
Classical novae are potential gamma-ray emitters, both in lines and in a continuum. Continuum emission (at energies between 20-30 and 511 keV) and line emission at 511 keV are related to positron annihilation and its Comptonization in the expanding shell; 18 F is the main responsible of positron production. The lines at 478 and 1275 keV have their origin on the decay of the radioactive nuclei 7...
It is well known that standard estimators of an AR(p) model are biased in finite samples, yet little is done in practice to remove the bias. Apparently small biases have important implications for the estimation of the impulse response function, which is a nonlinear function of the original coefficients. This note shows how to obtain estimators adjusted for first order bias based on Stine and S...
We present Spitzer high-resolution spectra of off-nuclear regions in the central cluster galaxies NGC 1275 and NGC 4696 in the Perseus and Centaurus clusters, respectively. Both objects are surrounded by extensive optical emission-line filamentary nebulae, bright outer parts of which are the targets of our observations. The 10–37µm spectra show strong pure rotational lines from molecular hydrog...
1Weill Medical College of Cornell University, 1300 York Avenue, New York, NY 10021, USA 2Ludwig Institute for Cancer Research, New York Branch at Memorial Sloan-Kettering Cancer Center, 1275 York Avenue, New York, NY 10021, USA 3Escola Paulista de Medicina, Universidade Federal de Sao Paulo, Sao Paulo, SP, Brazil 4Ludwig Institute for Cancer Research, Sao Paulo Branch, Sao Paulo, SP, Brazil *Th...
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