Hunger among Inuit children in Canada

Background and objectives. Inuit populations may be at increased risk for experiencing poor nutrition or hunger due to limited access and availability to food. The prevalence and correlates of parental perceptions of hunger among a nationally representative sample of Inuit children in Canada have not yet been reported. Design. Data are from the 2006 Aboriginal Children's Survey (ACS). Sociodemographic information, dietary behaviours and hunger status were parent-reported via a household interview for Inuit children aged 2–5 years (n=1,234). Prevalence of hunger was calculated among Inuit children by sociodemographic factors and by dietary behaviours. In addition, a multivariate logistic regression model was conducted to determine factors associated with parental perception of ever experiencing hunger. Results. The prevalence of Inuit children in Canada aged 2–5 years ever experiencing hunger was 24.4%. Children who were reported to have experienced hunger consumed milk and milk products (p<0.001); fish, eggs and meat (p<0.05); fruits (p<0.001); and vegetables (p<0.001) significantly less often than never-hungry children. Fast food and processed foods, soft drinks and juice, and salty snacks, sweets and desserts were consumed as often as never-hungry children (all p>0.05). The majority (81%) of Inuit parents/guardians of ever-hungry children sought help from family or friends. Factors associated with an increased likelihood of experiencing hunger include sociodemographic characteristics (such as income and household size), living in an Inuit region and living in a community with cultural activities. Conclusion. About 1 in 4 Inuit children were reported by their parents to have experienced hunger, and hunger was associated with region, sociodemographic and community factors. Future research could further examine the impact of ever experiencing hunger on the health status of Inuit children and their families in Canada

Do clusters contain a large population of dwarf galaxies?

We analyze systematic effects in the determination of the galaxy luminosity function in clusters using a deep mock catalogue constructed from a numerical simulation of a hierarchical universe. The results indicate a strong tendency to derive a rising faint end (\alpha \lsim -1.5) in clusters selected in two dimensions, using a galaxy catalogue constructed with a universal flat luminosity function with $\alpha \simeq -1.0$. This is due to the projection effects inherent in catalogues of clusters constructed using 2 dimensional data. Many of the clusters found in 2d have no significant 3d counterparts, and most suffer from massive background contamination that cannot be corrected for by subtracting random offset fields. The luminosity function of high surface brightness galaxies in the field and within small groups follows a Schechter function with a fairly flat faint end slope, $n(L)\propto L^{\alpha}$ with $\alpha = -0.9$ to -1.2. On the contrary, observational studies of clusters constructed using Abell, EDCC and APM catalogues are systematically found to have steeper luminosity functions with $\alpha = -1.4$ to -2.0. This may be attributed to projection effects rather than a dominant population of high surface brightness dwarf galaxies (M\gsim M^*+2) in clusters. It should be straighforward to confirm our results by measuring redshifts of these faint cluster galaxies.Comment: 23 pages, 7 Postscript figures TeX, accepted for publication in the Astrophysical Journal, e-mail:[email protected] http://iate.oac.uncor.edu/cv.htm