Ethical dilemmas in clinical social work practice : how are social workers affected and how do we respond?

This mixed-methods exploratory research was undertaken to gain insight into how social workers perceive, are affected by, and respond to situations in which they are not able to enact social work ethics, or are asked to facilitate perceived injustice because of workplace restrictions. Seventy-four social workers responded to my online mixed methods survey. In quantitative responses, Likert scaled responses rated participants’ frequency and level of distress when encountering ethical dilemmas involving structural racism, classism, cultural insensitivity, sexism, heterosexism, protocols prioritizing funding over client care, protocols interfering with the treatment relationship, and protocols interfering with client self-determination. Participants also rated their sense of burnout related to structurally imposed ethical dilemmas. Both descriptive statistics were derived, and correlations were obtained between demographic information and quantitative response re: frequency and distress. Qualitative text boxes allowed descriptions of experiences with ethical dilemmas in more detail – e.g., information about roles and social work settings in which dilemmas took place, and descriptions of participants’ suffering and action in relation to dilemmas. The study opens new avenues for social work as a profession to explore in the interest of preserving its loyalty to the social work code of ethics, and the individual social workers’ well-being and professional satisfaction

Assessing Students\u27 Acquisition of Scientific Reasoning in an Experimental Psychology Class

This pilot study is an initial exploration of a theoretical rubric proposed to describe the progress of students’ acquisition of scientific inquiry (Halonen et al., 2003, p. 196), and an application of the utility of the rubric. Twenty-two undergraduates from a woman’s college participated in two sections of experimental psychology. Students consisted of sophomores, juniors, and seniors who completed general psychology courses. Consistent with the Halonen et al. (2003) model, results indicated that authentic research experiences in the first phase of the course were positively correlated with changes in scientific thinking in a second phase. In turn, experiences in the second phase were positively correlated with evidence of advanced thinking skills in a third phase. The findings suggest that much of the basic skill knowledge acquired in the beginning lectures, textbook readings, and writing instruction of the course enhanced students’ ability to apply that knowledge in later classes and the lab components. Further, the authentic learning experiences were instrumental in fine-tuning the skills learned from the lectures and textbooks readings. As a result, the current authors advocate the use of authentic experiences in teaching research methods, as a way for teachers to transform such classes in a beneficial and systematic way, in order to enhance acquisition of scientific thinking skills and to examine changes in scientific thinking as explicated in the Halonen et al. (2003) model

The JCMT Gould Belt Survey: the effect of molecular contamination in SCUBA-2 observations of Orion A

Thermal emission from cold dust grains in giant molecular clouds can be used to probe the physical properties, such as density, temperature and emissivity in star-forming regions. We present the SCUBA-2 shared-risk observations at 450 $\mu$m and 850 $\mu$m of the Orion A molecular cloud complex taken at the James Clerk Maxwell Telescope (JCMT). Previous studies showed that molecular emission lines can contribute significantly to the measured fluxes in those continuum bands. We use the HARP $^{12}$CO J=3-2 integrated intensity map for Orion A in order to evaluate the molecular line contamination and its effects on the SCUBA-2 maps. With the corrected fluxes, we have obtained a new spectral index $\alpha$ map for the thermal emission of dust in the well-known integral-shaped filament. Furthermore, we compare a sample of 33 sources, selected over the Orion A molecular cloud complex for their high $^{12}$CO J=3-2 line contamination, to 27 previously identified clumps in OMC-4. This allows us to quantify the effect of line contamination on the ratio of 850 $\mu$m to 450 $\mu$m flux densities and how it modifies the deduced spectral index of emissivity $\beta$ for the dust grains. We also show that at least one Spitzer-identified protostellar core in OMC-5 has a $^{12}$CO J=3-2 contamination level of 16 %. Furthermore, we find the strongest contamination level (44 %) towards a young star with disk near OMC-2. This work is part of the JCMT Gould Belt Legacy Survey.Comment: 13 pages, 6 figures, Accepted for publication in Monthly Notices of the Royal Astronomical Society (MNRAS

Activity map of the tammar X chromosome shows that marsupial X inactivation is incomplete and escape is stochastic

BACKGROUND: X chromosome inactivation is a spectacular example of epigenetic silencing. In order to deduce how this complex system evolved, we examined X inactivation in a model marsupial, the tammar wallaby (Macropus eugenii). In marsupials, X inactivation is known to be paternal, incomplete and tissue-specific, and occurs in the absence of an XIST orthologue. RESULTS: We examined expression of X-borne genes using quantitative PCR, revealing a range of dosage compensation for different loci. To assess the frequency of 1X- or 2X-active fibroblasts, we investigated expression of 32 X-borne genes at the cellular level using RNA-FISH. In female fibroblasts, two-color RNA-FISH showed that genes were coordinately expressed from the same X (active X) in nuclei in which both loci were inactivated. However, loci on the other X escape inactivation independently, with each locus showing a characteristic frequency of 1X-active and 2X-active nuclei, equivalent to stochastic escape. We constructed an activity map of the tammar wallaby inactive X chromosome, which identified no relationship between gene location and extent of inactivation, nor any correlation with the presence or absence of a Y-borne paralog. CONCLUSIONS: In the tammar wallaby, one X (presumed to be maternal) is expressed in all cells, but genes on the other (paternal) X escape inactivation independently and at characteristic frequencies. The paternal and incomplete X chromosome inactivation in marsupials, with stochastic escape, appears to be quite distinct from the X chromosome inactivation process in eutherians. We find no evidence for a polar spread of inactivation from an X inactivation center.This project was funded by grants to JAMG and PDW from the Australian Research Council

Activity map of the tammar X chromosome shows that marsupial X inactivation is incomplete and escape is stochastic

BACKGROUND: X chromosome inactivation is a spectacular example of epigenetic silencing. In order to deduce how this complex system evolved, we examined X inactivation in a model marsupial, the tammar wallaby (Macropus eugenii). In marsupials, X inactivation is known to be paternal, incomplete and tissue-specific, and occurs in the absence of an XIST orthologue. RESULTS: We examined expression of X-borne genes using quantitative PCR, revealing a range of dosage compensation for different loci. To assess the frequency of 1X- or 2X-active fibroblasts, we investigated expression of 32 X-borne genes at the cellular level using RNA-FISH. In female fibroblasts, two-color RNA-FISH showed that genes were coordinately expressed from the same X (active X) in nuclei in which both loci were inactivated. However, loci on the other X escape inactivation independently, with each locus showing a characteristic frequency of 1X-active and 2X-active nuclei, equivalent to stochastic escape. We constructed an activity map of the tammar wallaby inactive X chromosome, which identified no relationship between gene location and extent of inactivation, nor any correlation with the presence or absence of a Y-borne paralog. CONCLUSIONS: In the tammar wallaby, one X (presumed to be maternal) is expressed in all cells, but genes on the other (paternal) X escape inactivation independently and at characteristic frequencies. The paternal and incomplete X chromosome inactivation in marsupials, with stochastic escape, appears to be quite distinct from the X chromosome inactivation process in eutherians. We find no evidence for a polar spread of inactivation from an X inactivation center.This project was funded by grants to JAMG and PDW from the Australian Research Council

Precision nomenclature for the new genomics

The confluence of two scientific disciplines may lead to nomenclature conflicts that require new terms while respecting historical definitions. This is the situation with the current state of cytology and genomics, which offer examples of distinct nomenclature and vocabularies that require reconciliation. In this article, we propose the new terms C-scaffold (for chromosome-scale assemblies of sequenced DNA fragments, commonly named scaffolds) and scaffotype (the resulting collection of C-scaffolds that represent an organism\u27s genome). This nomenclature avoids conflict with the historical definitions of the terms chromosome (a microscopic body made of DNA and protein) and karyotype (the collection of images of all chromosomes of an organism or species). As large-scale sequencing projects progress, adoption of this nomenclature will assist end users to properly classify genome assemblies, thus facilitating genomic analysis

The JCMT Gould Belt Survey: the effect of molecular contamination in SCUBA-2 observations of Orion A

JOURThis is the final version of the article. It was first published by Oxford Journals for the Royal Astronomical Society via http://dx.doi.org/ 10.1093/mnras/stv3009Thermal emission from cold dust grains in giant molecular clouds can be used to probe the physical properties, such as density, temperature and emissivity in star-forming regions. We present the Submillimetre Common-User Bolometer Array (SCUBA-2) shared-risk observations at 450 and 850 μm of the Orion A molecular cloud complex taken at the James Clerk Maxwell Telescope (JCMT). Previous studies showed that molecular emission lines can contribute significantly to the measured fluxes in those continuum bands. We use the Heterodyne Array Receiver Programme 12CO J = 3-2 integrated intensity map for Orion A in order to evaluate the molecular line contamination and its effects on the SCUBA-2 maps. With the corrected fluxes, we have obtained a new spectral index α map for the thermal emission of dust in the well-known integral-shaped filament. Furthermore, we compare a sample of 33 sources, selected over the Orion A molecular cloud complex for their high 12CO J = 3-2 line contamination, to 27 previously identified clumps in OMC 4. This allows us to quantify the effect of line contamination on the ratio of 850-450 μm flux densities and how it modifies the deduced spectral index of emissivity β for the dust grains. We also show that at least one Spitzer-identified protostellar core in OMC 5 has a 12CO J = 3-2 contamination level of 16 per cent. Furthermore, we find the strongest contamination level (44 per cent) towards a young star with disc near OMC 2. This work is part of the JCMT Gould Belt Legacy Survey