Information technology and school libraries: a social justice perspective

This research takes an emergent approach to data analysis (Charmaz, 2008) through the use of an emic/etic data coding process, and proposes a typology for understanding the connection between social justice principles and the provision of information technology services in school libraries. The study used data from seven school libraries in the state of New Jersey, obtained from focus groups consisting of forty-eight teachers, eighteen librarians, ten department supervisors, eleven principals/assistant principals, four district directors, and three librarian-teachers. The emergent process and typology employed in this research can aid school libraries in assessing how particular factors of the school/school library environment influence the provision of IT services to school library users. This study confirmed that school librarians and teachers rely on several social justice principles, such as distributive justice, utilitarianism, and egalitarianism, in making decisions regarding how to provide information technology services within the school environment. In particular, it was found that the type of social justice principle used in the school environment depended on the school librarians’ and teachers’ perceptions of the information competencies of their constituents and the availability of resources within the school environment. This research contributes to the study of social justice in the library and information science (LIS) professions in the following ways: first, by expanding ideas of “social justice” in LIS beyond traditional notions of “disenfranchised groups”—such as people having lower socioeconomic status, racial/ethnic or sexual minorities, and individuals with physical or mental disabilities—to include any group that may experience injustice in the context of information, such as school teachers, librarians and students; second, by portraying how social justice principles are enacted as strategies in school librarianship and pedagogy that advance student information-seeking and learning objectives; third, by highlighting the value of social justice to both practice and scholarly research in school and school library environments; and fourth, by proposing a methodology for studying social justice in a library environment.published or submitted for publicatio

Gambling Behavior in Controlled Laboratory Experiments

We designed a slot machine interface to study gambling behavior over real monetary amounts in a controlled laboratory environment. The interface allowed us to study the effect of multiple playlines compared to single playlines, the use of abstract tokens instead of allowing the gambler to see expenditures and payoffs in a natural currency, the effect of “near miss” displays on subjective beliefs about the chances of winning, and the effect of “wins disguised as losses” on gambling behavior. We measured the risk preferences of each subject, allowing for probability weighting and loss aversion, as well as the evolution of subjective beliefs of expected winnings for some subjects. Every subject also completed popular survey screens for disordered gambling, allowing an evaluation of their predictive accuracy with respect to gambling over real stakes up to $1,500. All experiments were implemented for real rewards, so that responses were incentivized

UV Imaging Polarimetry of the Seyfert 2 Galaxy Mrk 3

We present UV imaging polarimetry data of the Seyfert 2 galaxy Mrk 3 taken by the Hubble Space Telescope. The polarized flux is found to be extended to ~1 kpc from the nucleus, and the position angles of polarization are centrosymmetric, confirming that the polarization is caused by scattering. We determine the location of the hidden nucleus as the center of this centrosymmetric pattern. From the polarization images taken in two broad bands, we have obtained the color distribution of the polarized flux. Some regions have blue polarized flux, consistent with optically-thin dust scattering, but some bright knots have a color similar to that of Seyfert 1 nucleus. Also, the recent Chandra X-ray observation suggests that the ratio of scattered UV flux to scattered X-ray flux is rather similar to the intrinsic UV/X-ray ratio in a Seyfert 1 nucleus, if the observed extended X-ray continuum is scattered light. While the scattered X-ray would be essentially from electron scattering, the UV slope and UV/X-ray ratio both being similar to Seyfert 1's would lead to two possibilities as to the nature of the UV scatterers. One is that the UV may also be scattered by electrons, in which case the scattering gas is somehow dust-free. The other is that the UV is scattered by dust grains, but the wavelength-independent UV scattering with low efficiency indicated by the UV slope and UV/X-ray ratio would suggest that the grains reside in UV-opaque clouds, or the dust might be mainly composed of large grains and lacks small-grain population.Comment: 15 pages, 8 figures (plus 2 color versions of grayscale figures), To appear in ApJ; minor corrections for the proofs of the manuscrip

Information Literacy: Agendas for a Sustainable Future

This paper, somewhat an incomplete historical overview and personal perspective, outlines a number of key challenges and opportunities in relation to future directions and developments in information literacy as a field of research and professional practice.  It gives attention to significant foundational (selective) scholarship in the field, identifies a number of challenges in relation to theoretical frameworks, research needs, determining outcomes and impacts, and pedagogical frameworks for information literacy instruction. It is posited that addressing these challenges can play a role in sustaining information literacy as a significant educational and social agenda.

The Sexual health of pupils in years 4 to 6 of primary schools in rural Tanzania

Background/objectives: There is an urgent need for effective interventions to improve the sexual and\ud reproductive health of adolescents. Reliable data on the sexual health of adolescents are needed to guide\ud the development of such interventions. The aim was to describe the sexual health of pupils in years 4 to 6 of\ud 121 rural primary schools in north western Tanzania, before the implementation of an innovative sexual\ud health intervention in 58 of the schools.\ud Methods: A cross sectional survey of primary school pupils in rural Tanzania was carried out. The study\ud population comprised pupils registered in years 4 to 6 of 121 primary schools in 20 rural communities in\ud 1998. Basic demographic information was collected from all pupils seen. Those born before 1 January\ud 1985 (aged approximately 14 years and over) were invited to participate in the survey, and asked about\ud their knowledge and attitudes towards sexual health issues, and their sexual experience. A urine specimen\ud was requested and tested for HIV, Chlamydia trachomatis (CT), Neisseria gonorrhoeae (NG) and, for\ud females, pregnancy.\ud Results: 9283 pupils born before 1 January 1985 were enrolled and provided demographic information\ud and a urine sample. Male pupils were significantly older than females (mean age 15.5 years v 14.8 years,\ud p,0.001), but all other demographic characteristics were similar between the sexes. 14 (0.2%) of the\ud enrolled pupils (four male and 10 female) were HIV positive, 83 (0.9%) were positive for CT, and 12\ud (0.1%) for NG. 32 female pupils (0.8%) were positive by pregnancy test. Sexual experience was reported\ud by one fifth of primary school girls, and by almost half of boys. Only 45/114 (39%) girls with biological\ud markers of sexual activity reported having had sex.\ud Conclusions: HIV, CT, NG, and pregnancy were present though at relatively low levels among pupils in\ud years 4 to 6 of primary school. A high proportion of pupils with a biological marker of sexual activity\ud denied ever having had sex. Alternative ways of collecting sensitive data about the sexual behaviour of\ud school pupils should be explored

UV Imaging Polarimetry of the peculiar Seyfert 2 galaxy Mrk 477

We present the results of UV imaging polarimetry of the Seyfert 2 galaxy Mrk 477 taken by the Faint Object Camera onboard the Hubble Space Telescope (HST). From a previous HST UV image (lambda ~ 2180A), Mrk 477 has been known to have a pointlike bright UV hotspot in the central region, peculiar among nearby Seyfert 2 galaxies. There are also claims of UV/optical variability, unusual for a Seyfert 2 galaxy. Our data show that there is an off-nuclear scattering region ~ 0."6 (~ 500 pc) NE from the hotspot. The data, after the subtraction of the instrumental effect due to this bright hotspot region, might indicate that the scattered light is also detected in the central 0."2 radius region and is extended to a very wide angle. The hotspot location is consistent with the symmetry center of the PA pattern, which represents the location of the hidden nucleus, but our data do not provide a strong upper limit to the distance between the symmetry center and the hotspot. We have obtained high spatial resolution color map of the continuum which shows that the nuclear spiral arm of 0."4 scale (~ 300pc) is significantly bluer than the off-nuclear mirror and the hotspot region. The nature of the hotspot is briefly discussed.Comment: To appear in Ap

Graduate students' sense making process in collaborative learning tasks

This current study explores how graduate students make sense together to accomplish real-life collaborative learning tasks. A class of 15 adult students at a large, public university in Northeast US is recruited. The purpose of their learning task is to work with team members and construct group presentations on their collective understandings on information behaviors within specific contexts. Data sources include pre- and post-questionnaires, classroom observations, and in-depth interviews that are structured within Dervin’s (1992) Sense-Making methodology. Our findings identify several task related situations, gaps, and sense-making strategies that incorporate the social dimensions. These social dimensions and emergent collaborative/cooperative learning processes are highlighted and discussed. Overall this study has implications for educators to design socially constructed learning environment and facilitate learners’ sense-making processes when undertaking collaborative tasks.ye

Understanding Accretion Outbursts in Massive Protostars through Maser Imaging

The bright maser emission produced by several molecular species at centimeter to long millimeter wavelengths provides an essential tool for understanding the process of massive star formation. Unimpeded by the high dust optical depths that affect shorter wavelength observations, the high brightness temperature of these emission lines offers a way to resolve accretion and outflow motions down to scales below $\sim$1 au in deeply embedded Galactic star-forming regions at kiloparsec distances. The recent identification of extraordinary accretion outbursts in two high-mass protostars, both of which were heralded by maser flares, has rapidly impacted the traditional view of massive protostellar evolution, leading to new hydrodynamic simulations that can produce such episodic outbursts. In order to understand how these massive protostars evolve in response to such events, larger, more sensitive ground-based centimeter wavelength interferometers are needed that can simultaneously image multiple maser species in the molecular gas along with faint continuum from the central ionized gas. Fiducial observations of a large sample of massive protostars will be essential in order to pinpoint the progenitors of future accretion outbursts, and to quantify the outburst-induced changes in their protostellar photospheres and outflow and accretion structures. Knowledge gained from these studies will have broader impact on the general topic of accretion onto massive objects.Comment: Science white paper submitted to the Astro2020 Decadal Survey. arXiv admin note: substantial text overlap with arXiv:1806.0698

Asymmetry and Inequity in the Inheritance of a Bacterial Adhesive

Pseudomonas aeruginosa is an opportunistic human pathogen that forms biofilm infections in a wide variety of contexts. Biofilms initiate when bacteria attach to a surface, which triggers changes in gene expression leading to the biofilm phenotype.Wehave previously shown, for the P. aeruginosa lab strain PAO1, that the self-produced polymer Psl is the most dominant adhesive for attachment to the surface but that another self-produced polymer, Pel, controls the geometry of attachment of these rod-shaped bacteria—strains that make Psl but not Pel are permanently attached to the surface but adhere at only one end (tilting up off the surface), whereas wild-type bacteria that make both Psl and Pel are permanently attached and lie down flat with very little or no tilting (Cooley et al 2013 Soft Matter 9 3871–6). Here we show that the change in attachment geometry reflects a change in the distribution of Psl on the bacterial cell surface. Bacteria that make Psl and Pel have Psl evenly coating the surface, whereas bacteria that make only Psl have Psl concentrated at only one end.Weshow that Psl can act as an inheritable, epigenetic factor. Rod-shaped P. aeruginosa grows lengthwise and divides across the middle.Wefind that asymmetry in the distribution of Psl on a parent cell is reflected in asymmetry between siblings in their attachment to the surface. Thus, Pel not only promotes P. aeruginosa lying downWe thank Professor Matthew Parsek (University of Washington, Seattle) for his generous gift of bacterial PAO1 strains.Wealso thank Professor Marvin Whiteley (University of Texas at Austin) forWTandΔpsl polysaccharide preparations. SIM imaging (for figure 1) was performed in the Microscopy Core Facility within the Institute for Cellular and Molecular Biology atUTAustin, with the assistance of Julie Hayes. This work was funded by startup funds fromUTAustin and a gift from ExxonMobil to VDG, and by a grant from the Human Frontiers Science Program (HFSP RGY0081/2012-GORDON).Center for Nonlinear Dynamic

The global distribution of Bacillus anthracis and associated anthrax risk to humans, livestock and wildlife.

Bacillus anthracis is a spore-forming, Gram-positive bacterium responsible for anthrax, an acute infection that most significantly affects grazing livestock and wild ungulates, but also poses a threat to human health. The geographic extent of B. anthracis is poorly understood, despite multi-decade research on anthrax epizootic and epidemic dynamics; many countries have limited or inadequate surveillance systems, even within known endemic regions. Here, we compile a global occurrence dataset of human, livestock and wildlife anthrax outbreaks. With these records, we use boosted regression trees to produce a map of the global distribution of B. anthracis as a proxy for anthrax risk. We estimate that 1.83 billion people (95% credible interval (CI): 0.59-4.16 billion) live within regions of anthrax risk, but most of that population faces little occupational exposure. More informatively, a global total of 63.8 million poor livestock keepers (95% CI: 17.5-168.6 million) and 1.1 billion livestock (95% CI: 0.4-2.3 billion) live within vulnerable regions. Human and livestock vulnerability are both concentrated in rural rainfed systems throughout arid and temperate land across Eurasia, Africa and North America. We conclude by mapping where anthrax risk could disrupt sensitive conservation efforts for wild ungulates that coincide with anthrax-prone landscapes