Detection of cosmic magnification via galaxy shear-galaxy number density correlation from HSC survey data

Xiangkun Liu; Dezi Liu; Zucheng Gao; Chengliang Wei; Guoliang Li; Liping Fu; Toshifumi Futamase; Zuhui Fan

doi:10.1103/physrevd.103.123504

Detection of cosmic magnification via galaxy shear-galaxy number density correlation from HSC survey data

Physical Review D ◽

10.1103/physrevd.103.123504 ◽

2021 ◽

Vol 103 (12) ◽

Author(s):

Xiangkun Liu ◽

Dezi Liu ◽

Zucheng Gao ◽

Chengliang Wei ◽

Guoliang Li ◽

...

Keyword(s):

Survey Data ◽

Number Density ◽

Density Correlation

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A Trickiness of the High-Temperature Limit for Number Density Correlation Functions in Classical Coulomb Fluids

Journal of Statistical Physics ◽

10.1007/s10955-007-9337-6 ◽

2007 ◽

Vol 128 (3) ◽

pp. 569-586

Author(s):

Ladislav Šamaj

Keyword(s):

High Temperature ◽

Correlation Functions ◽

Temperature Limit ◽

Number Density ◽

Density Correlation ◽

High Temperature Limit ◽

Coulomb Fluids

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Mass Determination by Direct Measurement of Electron Scattering

Proceedings, annual meeting, Electron Microscopy Society of America ◽

10.1017/s0424820100114827 ◽

1975 ◽

Vol 33 ◽

pp. 240-241

Author(s):

M. K. Lamvik ◽

A. V. Crewe

Keyword(s):

Cross Section ◽

Electron Scattering ◽

Mass Density ◽

Variable Mass ◽

Scattering Cross Section ◽

Mass Determination ◽

Number Density ◽

Cross Sectional ◽

Thin Slice ◽

Scattering Cross

If a molecule or atom of material has molecular weight A, the number density of such units is given by n=Nρ/A, where N is Avogadro's number and ρ is the mass density of the material. The amount of scattering from each unit can be written by assigning an imaginary cross-sectional area σ to each unit. If the current I0 is incident on a thin slice of material of thickness z and the current I remains unscattered, then the scattering cross-section σ is defined by I=IOnσz. For a specimen that is not thin, the definition must be applied to each imaginary thin slice and the result I/I0 =exp(-nσz) is obtained by integrating over the whole thickness. It is useful to separate the variable mass-thickness w=ρz from the other factors to yield I/I0 =exp(-sw), where s=Nσ/A is the scattering cross-section per unit mass.

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Is the Personal Always Political?

Journal of Individual Differences ◽

10.1027/1614-0001/a000230 ◽

2017 ◽

Vol 38 (3) ◽

pp. 133-143 ◽

Cited By ~ 4

Author(s):

Danny Osborne ◽

Yannick Dufresne ◽

Gregory Eady ◽

Jennifer Lees-Marshment ◽

Cliff van der Linden

Keyword(s):

Survey Data ◽

National Survey ◽

Negative Relationship ◽

Openness To Experience ◽

Political Sophistication ◽

Knowledge Based

Abstract. Research demonstrates that the negative relationship between Openness to Experience and conservatism is heightened among the informed. We extend this literature using national survey data (Study 1; N = 13,203) and data from students (Study 2; N = 311). As predicted, education – a correlate of political sophistication – strengthened the negative relationship between Openness and conservatism (Study 1). Study 2 employed a knowledge-based measure of political sophistication to show that the Openness × Political Sophistication interaction was restricted to the Openness aspect of Openness. These studies demonstrate that knowledge helps people align their ideology with their personality, but that the Openness × Political Sophistication interaction is specific to one aspect of Openness – nuances that are overlooked in the literature.

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