Digital Surveillance: Foucault, the Internet, and the Meaning for Democracy

In this paper, we discuss digital surveillance and ways it enhances and changes the surveillance society Foucault described. Digital technology often has positioned itself as being a new media formation that will enhance democracy through peer-to-peer networks that highlight user-generated content and user-generated prioritization. Often hidden, however, is the relationship between the user and the owner of the proprietary digital space. Here, we explore the ways that the phenomenon digital surveillance actually differs from Foucault\u27s interpretation as the social context has changed

A Brief History of the First 10 Years of the Curriculum Studies Summer Collaborative

To mark the inaugural issue of the Curriculum Studies Collaborative Journal, it is important to acknowledge the history of its origins,as an outgrowth of The Curriculum Studies Summer Collaborative (CSSC). The CSSC, which has grown into a successful international Collaborative, was our brainchild when we were just beginning our careers at Georgia Southern University. For years, Julie, an alumna ofthe Curriculum Studies program at Georgia Southern, had heard her mentors talk about the need for a conference that would both highlight Georgia Southern’s important contributions to the field of curriculum theory and provide opportunities for doctoral students, most of whom were practitioners, to gain more exposure to a diverse range of international curriculum scholars. Daniel, a graduate of the University of North Carolina-Greensboro, recognized the unique, practitioner-oriented nature of the doctoral program at Georgia Southern and saw an opportunity to bring the more traditional conference experience most Ph.D. candidates have directly to his students. Together, Julie, a faculty member in the then-named Department of Teaching and Learning, and Daniel, a faculty member in the Department of Curriculum, Foundations, and Reading, decided to organize a conference that emphasized collaboration – between the two departments; between the conference organizers; and between senior, junior and emerging scholars, as well as practitioners

SNP identification of Africanized honey bees

Pubertal growth results from increased sex steroid and growth hormone (GH) secretion. Estrogens appear to play an important role in the regulation of pubertal growth in both girls and boys. In girls, however, estrogens cannot be the only sex steroids responsible for pubertal growth, as exogenous estrogens do not initiate a complete growth spurt. We therefore investigated the levels of the different sex steroids and GH, and related them to pubertal growth. In addition, we studied the process of bone maturation and mineralization during this period. Levels of both estrogens and androgens were found to increase at the start of the female pubertal growth spurt, and it was demonstrated that height velocity is related to levels of GH, estradiol and androstenedione, but not dehydroepiandrosterone sulfate. In boys, GH, testosterone and estradiol increased at the time of peak height velocity. Bone mineralization increased as puberty began, and was associated with the increase in height velocity. Osteocalcin, a marker of bone formation, declined when height velocity decreased, although bone maturation progressed at a steady rate. We conclude, therefore, that in girls, the concerted actions of estradiol, GH and androstenedione play a role in the pubertal growth spurt, whereas in boys this role is fulfilled by testosterone, GH and estradiol. During puberty, an advanced rate of bone maturation with respect to cross-sectional standards is a physiological phenomenon

Development and Piloting of a Novel Evaluation Tool for Childhood Obesity Prevention Programs

Childhood obesity remains chronic and high in the U.S., driven by factors including poor dietary habits and lack of physical activity. Interventions that address multiple causal factors may be the most appropriate strategy to address rising childhood obesity rates. The Cooperative Extension Service offers programs across the country to address causal factors of childhood obesity, but few coordinated or concerted efforts have been made to determine overlap, reduce duplication, or identify best practices in programming. To fill this gap, the National Institute of Food and Agriculture Multistate Project W3005 Extension Workgroup sought to develop a novel tool to compare programs with components related to childhood obesity prevention. This manuscript details the iterative process used to develop the Childhood Obesity Prevention Program in Extension Rubric (COPPER), provides findings from the pilot process, and reveals the broad application and potential of this tool within Extension and nutrition education. The newly developed COPPER tool is multi-functional and may be beneficial in program development, implementation, adoption, and/or adaptation of programs in new settings. This tool will be useful for Extension, public health, and other community organizations focused on issues central to childhood obesity targeting children, parents, and/or caregivers

Effect of PPARγ Inhibition during Pregnancy on Posterior Cerebral Artery Function and Structure

Peroxisome proliferator-activated receptor-γ (PPARγ), a ligand-activated transcription factor, has protective roles in the cerebral circulation and is highly activated during pregnancy. Thus, we hypothesized that PPARγ is involved in the adaptation of cerebral vasculature to pregnancy. Non-pregnant (NP) and late-pregnant (LP) rats were treated with a specific PPARγ inhibitor GW9662 (10 ]mg/kg/day, in food) or vehicle for 10 days and vascular function and structural remodeling were determined in isolated and pressurized posterior cerebral arteries (PCA). Expression of PPARγ and angiotensin type 1 receptor (AT1R) in cerebral (pial) vessels was determined by real-time RT-PCR. PPARγ inhibition decreased blood pressure and increased blood glucose in NP rats, but not in LP rats. PPARγ inhibition reduced dilation to acetylcholine and sodium nitroprusside in PCA from NP (p < 0.05 vs. LP-GW), but not LP rats. PPARγ inhibition tended to increase basal tone and myogenic activity in PCA from NP rats, but not LP rats. Structurally, PPARγ inhibition increased wall thickness in PCA from both NP and LP rats (p < 0.05), but increased distensibility only in PCA from NP rats. Pregnancy decreased expression of PPARγ and AT1R (p < 0.05) in cerebral arteries that was not affected by GW9662 treatment. These results suggest that PPARγ inhibition had significant effects on the function and structure of PCA in the NP state, but appeared to have less influence during pregnancy. Down-regulation of PPARγ and AT1R in cerebral arteries may be responsible for the lack of effect of PPARγ in cerebral vasculature and may be part of the vascular adaptation to pregnancy

Using an Observational Framework to investigate adult language input to young children in a naturalistic environment

The correlation between the communicative intent of parents, in terms of their expectation of a response and the response patterns of young children aged 23—25 months during parent—child interactions, was investigated. An Observational Framework was used to code these parameters in interactions between 36 children and their mothers. The children were assigned by cluster analysis to `advanced', `typical' and `delayed' language groups and their responses were coded with respect to the degree of correctness or appropriateness within the interaction. Differences in both the parental response expectations and the children's response patterns across the three clusters are discussed

Constraining the Lyα escape fraction with far-infrared observations of Lyα emitters

We study the far-infrared properties of 498 Lyα emitters (LAEs) at z = 2.8, 3.1, and 4.5 in the Extended Chandra Deep Field-South, using 250, 350, and 500μm data from the Herschel Multi-tiered Extragalactic Survey and 870μm data from the LABOCA ECDFS Submillimeter Survey. None of the 126, 280, or 92 LAEs at z = 2.8, 3.1, and 4.5, respectively, are individually detected in the far-infrared data. We use stacking to probe the average emission to deeper flux limits, reaching 1σ depths of ∼0.1 to 0.4 mJy. The LAEs are also undetected at ?3σ in the stacks, although a 2.5σ signal is observed at 870μm for the z = 2.8 sources. We consider a wide range of far-infrared spectral energy distributions (SEDs), including an M82 and an Sd galaxy template, to determine upper limits on the far-infrared luminosities and far-infrared-derived star formation rates of the LAEs. These star formation rates are then combined with those inferred from the Lyα and UV emission to determine lower limits on the LAEs’ Lyα escape fraction (f esc (Lyα)). For the Sd SED template, the inferred LAEs f esc (Lyα) are ?30% (1σ) at z = 2.8, 3.1, and 4.5, which are all significantly higher than the global f esc (Lyα) at these redshifts. Thus, if the LAEs f esc (Lyα) follows the global evolution, then they have warmer far-infrared SEDs than the Sd galaxy template. The average and M82 SEDs produce lower limits on the LAE f esc (Lyα) of ∼10%–20% (1σ), all of which are slightly higher than the global evolution of f esc (Lyα), but consistent with it at the 2σ–3σ level

Disentangling a group of lensed submm galaxies at z∼ 2.9

MS0451.6−0305 is a rich galaxy cluster whose strong lensing is particularly prominent at submm wavelengths. We combine new Submillimetre Common-User Bolometer Array (SCUBA)-2 data with imaging from Herschel Spectral and Photometric Imaging Receiver (SPIRE) and PACS and Hubble Space Telescope in order to try to understand the nature of the sources being lensed. In the region of the ‘giant submm arc', we uncover seven multiply imaged galaxies (up from the previously known four), of which six are found to be at a redshift of z∼2.9, and possibly constitute an interacting system. Using a novel forward-modelling approach, we are able to simultaneously deblend and fit spectral energy distributions to the individual galaxies that contribute to the giant submm arc, constraining their dust temperatures, far-infrared luminosities, and star formation rates (SFRs). The submm arc first identified by SCUBA can now be seen to be composed of at least five distinct sources, four of these within a galaxy group at z∼2.9. Only a handful of lensed galaxy groups at this redshift are expected on the sky, and thus this is a unique opportunity for studying such systems in detail. The total unlensed luminosity for this galaxy group is (3.1±0.3)×1012 L⊙, which gives an unlensed SFR of (450±50) M⊙yr−1. This finding suggests that submm source multiplicity, due to physically associated groupings as opposed to chance alignment, extends to fainter flux densities than previously discovered. Many of these systems may also host optical companions undetected in the submm, as is the case her