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20022015
most citedThe Cosmic Evolution Survey (COSMOS) -- Overview

2k citations

Showing 2013Show all

19 papers · 1 filter

cs.IT20133 cited

Least Mean Square/Fourth Algorithm with Application to Sparse Channel Estimation

Guan Gui, Abolfazl Mehbodniya, Fumiyuki Adachi

Broadband signal transmission over frequency-selective fading channel often requires accurate channel state information at receiver. One of the most attracting adaptive channel est…

math.FA2013

Asymptotic Spectral Distributions of Distance -Graphs of Cartesian Product Graphs

Yuji Hibino, Hun Hee Lee, Nobuaki Obata

Let be a finite connected graph on two or more vertices and the distance -graph of the -fold Cartesian power of . For a fixed , we obtain explicitly…

physics.optics201314 cited

Assessment of some experimental and image analysis factors for background oriented schlieren measurements

Ardian B. Gojani, Shigeru Obayashi

Quantitative measurements of fluid flow properties can be achieved by background oriented schlieren. In this paper it is shown that this depends on several factors. Image quality i…

cs.IT20131 cited

Second Order Asymptotics for Random Number Generation

Wataru Kumagai, Masahito Hayashi

We treat a random number generation from an i.i.d. probability distribution of to that of . When or is a uniform distribution, the problems have been well-known as t…

cond-mat.supr-con20132 cited

Spin-Triplet Superconductivity Induced by Longitudinal Ferromagnetic Fluctuations in UCoGe: Theoretical Aspect

Y. Tada, S. Fujimoto, N. Kawakami +6

Identification of pairing mechanisms leading to the unconventional superconductivity realized in copper-oxide, heavy-fermions, and organic compounds is one of the most challenging…

cond-mat.supr-con2013

High critical current density and low anisotropy in textured Sr1-xKxFe2As2 tapes for high field applications

Zhaoshun Gao, Yanwei Ma, Chao Yao +5

From the application point of view, large critical current densities Jc (H) for superconducting wires are required, preferably for magnetic fields higher than 5 T. Here we show tha…