The need for support: Young people living through a family health crisis

Young people living with a family health crisis are found to experience high levels of distress, anxiety, low mood and depressive symptoms and are at risk of becoming disengaged with education, socially isolated and uncertain regarding what the future will hold for them. A body of research indicates that practical intervention, including youth work, engagement with other young people and targeted support can have a significant impact upon a young person’s capacity to cope with a complex family health crisis and develop self-reliant behaviours. Despite the plethora of evidence to indicate the need for systems of support for children and young people experiencing a family health crisis, current provision across the UK is inconsistent, inequitable and not clearly underpinned by policy intervention. This study sets out to indicate the extent and nature of need of children and young people who are living with a family health crisis in Britain, the type of support they require and the ways in which Hope Support meets those needs

Competition & opportunity

Banks and banking ; Banking law ; Regulation Q: Prohibition Against Payment of Interest on Demand Deposits

Ebola – a societal pathogen in an epidemic of distrust

LSE’s Jane Cooper explores how our fears, representations and identities might account for the gap between threat and response to the Ebola epidemic

U.S. monetary policy in an integrating world: 1960 to 2000

Monetary policy ; Federal Open Market Committee ; Monetary policy - United States

Metal-poor, Strongly Star-Forming Galaxies in the DEEP2 Survey: The Relationship between Stellar Mass, Temperature-based Metallicity, and Star Formation Rate

We report on the discovery of 28 $z\approx0.8$ metal-poor galaxies in DEEP2. These galaxies were selected for their detection of the weak [OIII]$\lambda$4363 emission line, which provides a "direct" measure of the gas-phase metallicity. A primary goal for identifying these rare galaxies is to examine whether the fundamental metallicity relation (FMR) between stellar mass, gas metallicity, and star formation rate (SFR) holds for low stellar mass and high SFR galaxies. The FMR suggests that higher SFR galaxies have lower metallicity (at fixed stellar mass). To test this trend, we combine spectroscopic measurements of metallicity and dust-corrected SFRs, with stellar mass estimates from modeling the optical photometry. We find that these galaxies are $1.05\pm0.61$ dex above the z~1 stellar mass-SFR relation, and $0.23\pm0.23$ dex below the local mass-metallicity relation. Relative to the FMR, the latter offset is reduced to 0.01 dex, but significant dispersion remains (0.29 dex with 0.16 dex due to measurement uncertainties). This dispersion suggests that gas accretion, star formation and chemical enrichment have not reached equilibrium in these galaxies. This is evident by their short stellar mass doubling timescale of $\approx100^{+310}_{-75}$ Myr that suggests stochastic star formation. Combining our sample with other z~1 metal-poor galaxies, we find a weak positive SFR-metallicity dependence (at fixed stellar mass) that is significant at 94.4% confidence. We interpret this positive correlation as recent star formation that has enriched the gas, but has not had time to drive the metal-enriched gas out with feedback mechanisms.Comment: Resubmitted to ApJ on March 6, 2015. Revised to discuss selection biases and methodologies, and address the former by including more metal-rich galaxies with robust non-detections of [OIII]4363. Primary results on FMR analyses are unchanged. Additional figures are included to illustrate selection biases; previous figures have been revised to improve presentatio

A Brief Reflection at Twenty Years: Filling the Alumni Void

25th anniversary reflectio