Field of View and Stellar Density Function
Virtual Egocenters as a Function of Display Geometric Field of View and Eye Station Point
... This experiment was conducted to investigate the role of field of view (FOV) and observer station points in the perception of the location of one's egocenter (the personal viewpoint) in [r] ...
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The LAMOST spectroscopic survey of stars in the Kepler field of view: Activity indicators and stellar parameters
... of view of the Kepler space telescope covered with the LAMOST observations acquired in the second round of the LAMOST–Kepler project (in order to reduce the size of the figure, only every 15th target has been ...
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Electronic reconstruction of hexagonal FeS: a view from density functional dynamical mean-field theory
... insulating-metallic-insulating phases of FeS without leaving the strongly correlated picture, and derive the trans- itions by searching for the correlated solution of the DMFT equations under pressure. To justify our ...
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Field research: The animal welfare view
... & Fuller M.R., A Critical Review of the Effects of Marking on the Biology of Vertebrates, In Research Techniques in Animal Ecology , Columbia University Press, 2000. & Barber S.[r] ...
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The Economics of the Cloud: A View from the Field
... The Economics of the Cloud authors view Cloud computing as a new paradigm that is creating a transformative impact, but one that is not yet fully understood or leveraged. This, they argue, is analogous to another ...
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The CALIFA view on stellar angular momentum across the Hubble sequence
... of stellar kinematic maps is rapidly increas- ing with ongoing and upcoming integral-field spectroscopic in- struments and ...the stellar kinematic data at higher redshift will remain based on ...
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An Error Controlled Method to Determine the Stellar Density Function in a Region of the Sky
... the stellar density function in a region of the sky with complete error controlled esti- ...the density stellar function due to the variance of the least squares solutions ...
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Stellar population effects on the inferred photon density at reionization
... from stellar mergers (Eldridge et ...mass function for the stellar population, as well as creating more massive stars at later ages than would be expected for a single-star popula- ...
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The environmental dependence of the stellar mass function at z ~ 1. Comparing cluster and field between the GCLASS and UltraVISTA surveys
... The structure of the paper is as follows. In Sect. 2 we give an overview of GCLASS, and the spectroscopic and photometric data that have been taken for this cluster sample. We also de- scribe the data from the reference ...
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The environmental dependence of the stellar mass function at z ~ 1: Comparing cluster and field between the GCLASS and UltraVISTA surveys
... UltraVISTA field pop- ...the stellar mass range we study, so we take the shape of this SMF for the mass-quenched popu- lation and allow the normalisation to be adjusted by the ...
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Hyper Suprime-Cam view of the CMASS galaxy sample. Halo mass as a function of stellar mass, size, and Sérsic index
... fixed stellar mass ξ h , the inferred value depends in a non- negligible way on the surface brightness profile used to fit the photometric data, on which the stellar mass and size measure- ments are ...the ...
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Binaries in star clusters and the origin of the field stellar population
... 2. What is the origin of the field binary population? As we have seen, the properties of binaries in different environments are different. In particular, dense clusters have fewer binaries and those that they have ...
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Mapping the core mass function on to the stellar initial mass function: multiplicity matters
... the field statistics are probably not the only ones that form in a core cluster, but simply the ones that survive its dissolution and subsequent tidal perturbations ...the field, and also includes a ...
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The COSMOS2015 galaxy stellar mass function: Thirteen billion years of stellar mass assembly in ten snapshots
... The same properties are observed in (NUV − r) versus (r − K) and (U − V) versus (V − J), as demonstrated in Arnouts et al. ( 2013 ) and Forrest et al. ( 2016 ). Rest-frame colour selections have been successfully used up ...
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Evolution of the stellar mass function and infrared luminosity function of galaxies since z = 1.2
... luminosity function and stellar mass function (SMF) for red and blue galaxies at z ...luminosity density for both red and blue galaxies increased by a factor of ...a function of (B−V ) ...
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The connection between stellar activity cycles and magnetic field topology
... Donati & Landstreet, 2009; Morin et al., 2010; Vidotto et al., 2016; Folsom et al., 2016). Usually, the symbol size scales with log⟨B 2 ⟩ on this type of plot. However, due to the density of points in this plot, ...
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The connection between stellar activity cycles and magnetic field topology
... unresolved stellar discs making the determination of stellar activity cycle periods a non-trivial ...a function of ...of stellar cycles via ...
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The connection between stellar activity cycles and magnetic field topology
... Landstreet 2009; Morin et al. 2010; Vidotto et al. 2016; Folsom et al. 2016). Usually, the symbol size scales with loghB 2 i on this type of plot. However, due to the density of points in this plot, we have chosen ...
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Low Surface Brightness Galaxies and the Galaxy Stellar Mass Function
... for field galaxies Field galaxies are considered to be central in the modern parlance of halo occupation ...history, field galaxies form and evolve in a relatively isolated environment, and are ...
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Theoretical and experimental considerations of the critical current density of DI-BiSCCO superconducting tapes as a function of magnetic field, field orientation, temperature and strain
... Chapter 8 Future work In this chapter, we will consider the possible directions of some future work. The probe designed for comprehensive J c (B,T,θ,) measurements presented in Chapter 5 has incorporated a ...
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