An empirical investigation of the role of camaraderie, cause, competency, and participation motives in the development of attachment to a charity sport event

This paper examines the factors that contribute to the meaning participants hold for charity sport events. Specifically, the paper investigates the role of three value-laden constructs; along with participation motives, to understand participant attachment to a charity sport event. An online questionnaire was given to participants in the Lance Armstrong Foundation (LAF) LIVESTRONG Challenge (n=568) following the event. Data analysis revealed two recreational event motives, three motives for charitable giving, and three value-laden constructs contribute to attachment to the charity sport event. In addition, the results revealed the value-laden constructs make a stronger contribution to event attachment than the participation motives. Suggestions are made for increasing the meaning held for the event through community building, calls to action, and customization.Griffith Business School, Department of Tourism, Sport and Hotel ManagementFull Tex

Dark matter annihilation and decay in dwarf spheroidal galaxies: The classical and ultrafaint dSphs

Dwarf spheroidal (dSph) galaxies are prime targets for present and future gamma-ray telescopes hunting for indirect signals of particle dark matter. The interpretation of the data requires careful assessment of their dark matter content in order to derive robust constraints on candidate relic particles. Here, we use an optimised spherical Jeans analysis to reconstruct the `astrophysical factor' for both annihilating and decaying dark matter in 21 known dSphs. Improvements with respect to previous works are: (i) the use of more flexible luminosity and anisotropy profiles to minimise biases, (ii) the use of weak priors tailored on extensive sets of contamination-free mock data to improve the confidence intervals, (iii) systematic cross-checks of binned and unbinned analyses on mock and real data, and (iv) the use of mock data including stellar contamination to test the impact on reconstructed signals. Our analysis provides updated values for the dark matter content of 8 `classical' and 13 `ultrafaint' dSphs, with the quoted uncertainties directly linked to the sample size; the more flexible parametrisation we use results in changes compared to previous calculations. This translates into our ranking of potentially-brightest and most robust targets---viz., Ursa Minor, Draco, Sculptor---, and of the more promising, but uncertain targets---viz., Ursa Major 2, Coma---for annihilating dark matter. Our analysis of Segue 1 is extremely sensitive to whether we include or exclude a few marginal member stars, making this target one of the most uncertain. Our analysis illustrates challenges that will need to be addressed when inferring the dark matter content of new `ultrafaint' satellites that are beginning to be discovered in southern sky surveys.Comment: 19 pages, 14 figures, submitted to MNRAS. Supplementary material available on reques

Dark matter profiles and annihilation in dwarf spheroidal galaxies: prospectives for present and future γ-ray observatories - I. The classical dwarf spheroidal galaxies

Due to their large dynamical mass-to-light ratios, dwarf spheroidal galaxies (dSphs) are promising targets for the indirect detection of dark matter (DM) in γ-rays. We examine their detectability by present and future γ-ray observatories. The key innovative features of our analysis are as follows: (i) we take into account the angular size of the dSphs; while nearby objects have higher γ-ray flux, their larger angular extent can make them less attractive targets for background-dominated instruments; (ii) we derive DM profiles and the astrophysical J-factor (which parametrizes the expected γ-ray flux, independently of the choice of DM particle model) for the classical dSphs directly from photometric and kinematic data. We assume very little about the DM profile, modelling this as a smooth split-power-law distribution, with and without subclumps; (iii) we use a Markov chain Monte Carlo technique to marginalize over unknown parameters and determine the sensitivity of our derived J-factors to both model and measurement uncertainties; and (iv) we use simulated DM profiles to demonstrate that our J-factor determinations recover the correct solution within our quoted uncertainties. Our key findings are as follows: (i) subclumps in the dSphs do not usefully boost the signal; (ii) the sensitivity of atmospheric Cherenkov telescopes to dSphs within ∼20 kpc with cored haloes can be up to ∼50 times worse than when estimated assuming them to be point-like. Even for the satellite-borne Fermi-Large Area Telescope (Fermi-LAT), the sensitivity is significantly degraded on the relevant angular scales for long exposures; hence, it is vital to consider the angular extent of the dSphs when selecting targets; (iii) no DM profile has been ruled out by current data, but using a prior on the inner DM cusp slope 0 ≤γprior≤ 1 provides J-factor estimates accurate to a factor of a few if an appropriate angular scale is chosen; (iv) the J-factor is best constrained at a critical integration angle αc= 2rh/d (where rh is the half-light radius and d is the distance from the dwarf) and we estimate the corresponding sensitivity of γ-ray observatories; (v) the ‘classical' dSphs can be grouped into three categories: well constrained and promising (Ursa Minor, Sculptor and Draco), well constrained but less promising (Carina, Fornax and Leo I), and poorly constrained (Sextans and Leo II); and (vi) observations of classical dSphs with the Fermi-LAT integrated over the mission lifetime are more promising than observations with the planned Cherenkov Telescope Array for DM particle mass ≲ 700 GeV. However, even the Fermi-LAT will not have sufficient integrated signal from the classical dwarfs to detect DM in the ‘vanilla' Minimal Supersymmetric Standard Model. Both the Galactic Centre and the ‘ultrafaint' dwarfs are likely to be better targets and will be considered in future wor

Looking at Gender Differences Through the Lens of Sport Spectators

This paper explores common assumptions about the intrinsic differences between male and female consumers within a subset of leisure consumption - sport spectating. This research utilized the Sports Interest Inventory (SII) (Funk, Mahony & Ridinger, 2002) to examine differences between spectators (N = 959) attending men\u27s and women\u27s basketball games at a NCAA Division I institution. MANOVA results revealed nine differences for Team-Gender, seven differences for Spectator-Gender, and three interaction effects. Multiple linear regression analyses revealed that three core interest factors (university pride, team interest, and vicarious achievement) explained a significant proportion of variance in commitment and attendance behavior for fans of both teams. However, a number of interest factors related to Team-Gender and Spectator-Gender emerged to differentially explain levels of commitment and behavior. The results indicate that while there are some commonalities that motivate people to attend college basketball games involving athletes of each gender, there are also differences that make women\u27s basketball unique from men\u27s basketball

The first GCT camera for the Cherenkov Telescope Array

The Gamma Cherenkov Telescope (GCT) is proposed to be part of the Small Size Telescope (SST) array of the Cherenkov Telescope Array (CTA). The GCT dual-mirror optical design allows the use of a compact camera of diameter roughly 0.4 m. The curved focal plane is equipped with 2048 pixels of ~0.2{\deg} angular size, resulting in a field of view of ~9{\deg}. The GCT camera is designed to record the flashes of Cherenkov light from electromagnetic cascades, which last only a few tens of nanoseconds. Modules based on custom ASICs provide the required fast electronics, facilitating sampling and digitisation as well as first level of triggering. The first GCT camera prototype is currently being commissioned in the UK. On-telescope tests are planned later this year. Here we give a detailed description of the camera prototype and present recent progress with testing and commissioning.Comment: In Proceedings of the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. All CTA contributions at arXiv:1508.0589

Characterizing Consumer Motivation as Individual Difference Factors: Augmenting the Sports Interest Inventory (SII) to Explain Level of Spectator Support

The central focus of this study was to examine how individual difference factors could be used to explain various levels of consumer support for a specific sport property. The present study extends the Sport Interest Inventory (SII) in order to enhance current understanding of consumer motives in relation to sport in general and women\u27s competitive sport in particular. Confirmatory factor analysis confirmed the 12-item Sport Interest Inventory, measuring 14 individual difference factors related to spectator interest in soccer. Multiple Linear regression analysis revealed that five motivational characteristic--(a) sport interest, (b) team interest, (c) vicarious achievement, (d) role modeling, and (e) entertainment value--explained 54% of variance in level of spectator support for women\u27s professional soccer. These results suggest that augmenting traditional spectator measures offers a better understanding of motivational characteristics in different sport situations and of the impact these motivations have on behavior. Implications for marketers of women\u27s professional sports and of sports in general are discussed

‘I was there from the start’: The identity maintenance strategies used by fans to combat the threat of losing

On-field performances are a key, yet uncontrollable, determinant of team identification. In this research, we explore how fans of a new team, with an overwhelming loss to win ratio, maintain a positive social identity. Qualitative data gathered from 20 semi-structured interviews were used to address this research objective. Our findings indicated fans use social creativity and social mobility strategies to help preserve a positive and distinctive group identity. In the absence of success, fans evaluated the group on dimensions that reflected positively on, and emphasised the distinctiveness of, group membership. Fans also sought to increase their status in the group to increase the positivity of this association. We use these findings to extend understanding of social identity theory and provide recommendations for sport organisations with unfavourable performance records. Recommendations are themed around highlighting the unique nature of the group and and favourable status comparisons between members of the in-group

How to Advertise? Role of Congruence and Involvement on Multiscreen Consumption

It has become increasingly common for consumers to use additional devices while watching TV, a phenomenon called multiscreen viewing. This provides an additional advertising channel for marketers, specifically the second screen. However, it is not without its complexities; marketers must optimally time advertisements on the second screen conditional on the primary screen activity. Using a behavioral experiment this study proposes to investigate how consumers’ engagement and psychological involvement with the program on the primary screen affects their multiscreen behavior and its effect on brand recall. We further expect this relationship to be moderated by the congruence of the advertisement relative to the primary screen. Results of the study will not only contribute to the second screen literature in marketing and Information systems, but also help marketers develop actionable strategies for the second screen in multiscreen viewing contexts

Fermi Large Area Telescope Constraints on the Gamma-ray Opacity of the Universe

The Extragalactic Background Light (EBL) includes photons with wavelengths from ultraviolet to infrared, which are effective at attenuating gamma rays with energy above ~10 GeV during propagation from sources at cosmological distances. This results in a redshift- and energy-dependent attenuation of the gamma-ray flux of extragalactic sources such as blazars and Gamma-Ray Bursts (GRBs). The Large Area Telescope onboard Fermi detects a sample of gamma-ray blazars with redshift up to z~3, and GRBs with redshift up to z~4.3. Using photons above 10 GeV collected by Fermi over more than one year of observations for these sources, we investigate the effect of gamma-ray flux attenuation by the EBL. We place upper limits on the gamma-ray opacity of the Universe at various energies and redshifts, and compare this with predictions from well-known EBL models. We find that an EBL intensity in the optical-ultraviolet wavelengths as great as predicted by the "baseline" model of Stecker et al. (2006) can be ruled out with high confidence.Comment: 42 pages, 12 figures, accepted version (24 Aug.2010) for publication in ApJ; Contact authors: A. Bouvier, A. Chen, S. Raino, S. Razzaque, A. Reimer, L.C. Reye