Making Sense of Foster Care: An Evaluation of Family Group Decision Making in Kent County, Michigan

The University Archives has determined that this item is of continuing value to OSU's history.Crampton, David Stuart, Ph.D., University of Michigan, Ann Arbor, Michigan - "Making Sense of Foster Care: An Evaluation of Family Group Decision Making in Kent County, Michigan"The Ohio State University College of Social Wor

Family Involvement Interventions in Child Protection: Learning from Contextual Integrated Strategies

The use of family group conferencing and related family involvement interventions in child protection is rapidly increasing in the United States and many other countries. There is some concern that the child welfare field will travel down the same road as it did with intensive family preservation services; that is, tremendous enthusiasm later derailed by rigidly designed evaluations that showed unimpressive effects. The work of John Braithwaite suggests an alternative path for finding justifiable excitement about these interventions. Drawing upon Braithwaite\u27s writings and ongoing evaluation research, this article suggests a few steps we can take towards an integrative strategy for developing effective family involvement interventions

The Gravitational Lens CFRS03.1077

An exquisite gravitational arc with a radius of 2.1" has been discovered around the z = 0.938 field elliptical galaxy CFRS03.1077 during HST observations of Canada-France Redshift Survey (CFRS) fields. Spectroscopic observations of the arc show that the redshift of the resolved lensed galaxy is z = 2.941. This gravitational lens-source system is well-fitted using the position angle and ellipticity derived from the visible matter distribution and an isothermal mass profile with a mass corresponding to sigma =387+-5 km/s. Surprisingly, given the evidence for passive evolution of elliptical galaxies, this is in good agreement with an estimate based on the fundamental plane for z = 0 ellipticals. This, perhaps, indicates that this galaxy has not shared in the significant evolution observed for average elliptical galaxies at z ~ 1. A second elliptical galaxy with similar luminosity from the CFRS survey, CFRS 14.1311 at z=0.807, is also a lens but in this case the lens model gives a much smaller mass-to-light ratio, i.e., it appears to confirm the expected evolution. This suggests that this pair of field elliptical galaxies may have very different evolutionary histories, a significant result if confirmed. Clearly, CFRS03.1077 demonstrates that these "Einstein rings" are powerful probes of high redshift galaxies.Comment: 11 pages, 5 figures, accepted by Ap.

THE CANADA-FRANCE REDSHIFT SURVEY V: Global Properties of the Sample

The photometric and spectroscopic data of the CFRS survey of objects with 17.5 < I_{AB} < 22.5 are combined and analysed. The overall completeness is 85%. The redshift histogram of the sample is presented for 591 field galaxies with secure redshifts. The median redshift is z = 0.56, and the highest redshift observed is z = 1.3; 25 galaxies have z > 1 The distributions of magnitudes and colors demonstrate that galaxies at these high redshifts have very similar colors to those observed locally. The survey thus represents a major improvement in our knowledge of field galaxies at large look-back times. Only ~1% of the galaxies are as compact as stars (on images with FWHM ~ 0.9") and comparisons of the photometric and spectroscopic data show that only one galaxy was initially incorrectly classified spectroscopically as a star, and only two stars were misclassified as galaxies. It is demonstrated that the redshift distributions in the five fields are statistically consistent with each other, once the reduction in the effective number of independent galaxies due to small-scale clustering in redshift is taken into account. The photometric properties of the spectroscopically-unidentified objects indicate that most are likely to be galaxies rather than stars. At least half of these must have the same redshift distribution as the identified galaxies, and a combination of magnitudes, colors and compactness of the remaining unidentified galaxies is used to predict their redshifts. The majority are probably ordinary galaxies at the high redshift end of our sample, including some quiescent galaxies at z > 1.0, rather than some new or unusual population.Comment: 20 uuencoded postscript pages (first part) with 12 figures (second part). Also available at http://www.dao.nrc.ca/DAO/SCIENCE/science.html and coming soon on a CFRS homepage. Accepted June 19, scheduled for Dec 10 issue of Ap

Social Determinants of Health and Child Maltreatment Prevention: The Family Success Network Pilot

Child maltreatment is a highly prevalent public health concern that contributes to morbidity and mortality in childhood and short- and long-term health consequences that persist into adulthood. Past research suggests that social determinants of health such as socioeconomic status and intergenerational trauma are highly correlated with child maltreatment. With support from the U.S. Children’s Bureau, the Ohio Children’s Trust Fund is currently piloting the Family Success Network, a primary child maltreatment prevention strategy in Northeast Ohio that seeks to address these social determinants through pillars of service that include family coaching, financial assistance, financial education, parenting education, and basic life skills training. This study highlights the initial development phase of a pilot study. Plans for in-depth process and outcome evaluations are discussed. The project seeks to improve family functioning and reduce child protective services involvement and foster care entry in an economically disadvantaged region