127,014 research outputs found
Weak lensing power spectrum reconstruction by counting galaxies.-- I: the ABS method
We propose an Analytical method of Blind Separation (ABS) of cosmic
magnification from the intrinsic fluctuations of galaxy number density in the
observed galaxy number density distribution. The ABS method utilizes the
different dependences of the signal (cosmic magnification) and contamination
(galaxy intrinsic clustering) on galaxy flux, to separate the two. It works
directly on the measured cross galaxy angular power spectra between different
flux bins. It determines/reconstructs the lensing power spectrum analytically,
without assumptions of galaxy intrinsic clustering and cosmology. It is
unbiased in the limit of infinite number of galaxies. In reality the lensing
reconstruction accuracy depends on survey configurations, galaxy biases, and
other complexities, due to finite number of galaxies and the resulting shot
noise fluctuations in the cross galaxy power spectra. We estimate its
performance (systematic and statistical errors) in various cases. We find that,
stage IV dark energy surveys such as SKA and LSST are capable of reconstructing
the lensing power spectrum at and \ell\la 5000 accurately. This
lensing reconstruction only requires counting galaxies, and is therefore highly
complementary to the cosmic shear measurement by the same surveys.Comment: v1: 13 pages, 10 figures. v2: minor revisions. ApJ in pres
Electron correlation and spin-orbit coupling effects in US3 and USe3
A systematic density functional theory (DFT)+U study is conducted to
investigate the electron correlation and spin-orbit coupling (SOC) effects in
US3 and USe3. Our calculations reveal that inclusion of the U term is essential
to get energy band gaps for them, indicating the strong correlation effects for
uranium 5f electrons. Taking consideration of the SOC effect results in small
reduction on the electronic band gaps of US3 and USe3, but largely changes the
energy band shapes around the Fermi energy. As a result, US3 has a direct band
gap while USe3 has an indirect one. Our calculations predict that both US3 and
USe3 are antiferromagnetic insulators, in agreement with corresponding
experimental results. Based on our DFT+U calculations, we systematically
present the ground-state electronic, mechanical, and Raman properties for US3
and USe3.Comment: 6 pages, 6 figure
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