Constructing conceptualizations of English academic writing within an EFL context: streams of influence at a Taiwan university

The thesis draws upon in-depth research into the question of how English Academic Writing (EAW) is conceptualized at a Department of Applied English in a Taiwanese university. A qualitative research approach was taken within a social constructionism framework. Administrators, teachers, and students, were interviewed to explore the impact each of these three streams of influence has on the construction of the idea of EAW within this particular EFL context. These influences add to the mixture forming the conceptualization of EAW with a knock on effect to curriculum planning, teaching pedagogy, and the academic texts students produce. Administrators' design of a writing program and teachers' conceptualizations of EAW have implications for students' experience in learning to write and their own conceptualizations of what EAW is. Excerpts from interviews with teachers across the writing programme reveal how teachers do not share a coherent approach to teaching writing and yet have the understanding that they are conforming to a standardized conception of EAW. This research has important implications for curriculum design and lesson planning in EAW and EFL teacher training. Administrators need to implement a writing program with clear mutual goals as conceptualizations of EAW in an EFL context may be particularly fragile and lack consistency. Further implications of this research touch upon the training EFL teachers receive in graduate programs abroad which contribute to molding their conceptualizations of EAW. This research also points to the importance for administrators, teachers, and students to share a common language with which to discuss EAW issues

Promoting the Autonomy of Taiwanese EFL Learners in Higher Education by Using Self-Assessment Learning Logs

This study revealed how the classroom teaching practice of self-assessment learning logs helps to promote the autonomy of L2 learners in the context of higher education in Taiwan. L2 learners completed a self-assessment learning log entry on a biweekly basis, reflecting on what they had done outside of the classroom to improve their English. These learners then shared their learning log entries in class approximately once a month. Data from 30 participants were collected using a questionnaire containing both closed and open-ended questions. The results indicated that most participants believed that learning logs facilitated language learning; in particular, sharing what they had done with their classmates was a strong motivation to continue out-of-class learning activities. This paper offers specific suggestions for teachers regarding effective techniques for promoting learner autonomy

UB Knightlines Fall/Winter 2016

The UB Knightlines newsletter for fall and winter of 2016. This issue contains articles discussing winners of the UB Alumni Association's Distinguished Alumni Award, Alumni Association Scholarship winner Mendel Murray, professor Jeongkyu Lee’s Young Data Science program, president emeritus Richard Rubenstein and this book After Auschwitz, UB receiving a National Institutes of Health grant to expand research, SASD students winning third place in the Sherwin-Williams STIR Student Design Challenge, the opening of the new dorm University Hall, student Michael Asmerom a National Association of Black Accountants, professor Marsha Matto and SASD students work with couple to design beach home, faculty news, alumni news, books published by alums and faculty, and other campus and sports news

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

We systematically surveyed period variations of superhumps in SU UMa-type dwarf novae based on newly obtained data and past publications. In many systems, the evolution of superhump period are found to be composed of three distinct stages: early evolutionary stage with a longer superhump period, middle stage with systematically varying periods, final stage with a shorter, stable superhump period. During the middle stage, many systems with superhump periods less than 0.08 d show positive period derivatives. Contrary to the earlier claim, we found no clear evidence for variation of period derivatives between superoutburst of the same object. We present an interpretation that the lengthening of the superhump period is a result of outward propagation of the eccentricity wave and is limited by the radius near the tidal truncation. We interpret that late stage superhumps are rejuvenized excitation of 3:1 resonance when the superhumps in the outer disk is effectively quenched. Many of WZ Sge-type dwarf novae showed long-enduring superhumps during the post-superoutburst stage having periods longer than those during the main superoutburst. The period derivatives in WZ Sge-type dwarf novae are found to be strongly correlated with the fractional superhump excess, or consequently, mass ratio. WZ Sge-type dwarf novae with a long-lasting rebrightening or with multiple rebrightenings tend to have smaller period derivatives and are excellent candidate for the systems around or after the period minimum of evolution of cataclysmic variables (abridged).Comment: 239 pages, 225 figures, PASJ accepte

LSST: from Science Drivers to Reference Design and Anticipated Data Products

(Abridged) We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). A vast array of science will be enabled by a single wide-deep-fast sky survey, and LSST will have unique survey capability in the faint time domain. The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the Solar System, exploring the transient optical sky, and mapping the Milky Way. LSST will be a wide-field ground-based system sited at Cerro Pach\'{o}n in northern Chile. The telescope will have an 8.4 m (6.5 m effective) primary mirror, a 9.6 deg$^2$ field of view, and a 3.2 Gigapixel camera. The standard observing sequence will consist of pairs of 15-second exposures in a given field, with two such visits in each pointing in a given night. With these repeats, the LSST system is capable of imaging about 10,000 square degrees of sky in a single filter in three nights. The typical 5$\sigma$ point-source depth in a single visit in $r$ will be $\sim 24.5$ (AB). The project is in the construction phase and will begin regular survey operations by 2022. The survey area will be contained within 30,000 deg$^2$ with $\delta<+34.5^\circ$, and will be imaged multiple times in six bands, $ugrizy$, covering the wavelength range 320--1050 nm. About 90\% of the observing time will be devoted to a deep-wide-fast survey mode which will uniformly observe a 18,000 deg$^2$ region about 800 times (summed over all six bands) during the anticipated 10 years of operations, and yield a coadded map to $r\sim27.5$. The remaining 10\% of the observing time will be allocated to projects such as a Very Deep and Fast time domain survey. The goal is to make LSST data products, including a relational database of about 32 trillion observations of 40 billion objects, available to the public and scientists around the world.Comment: 57 pages, 32 color figures, version with high-resolution figures available from https://www.lsst.org/overvie

Pregnancy-specific stress, fetoplacental haemodynamics, and neonatal outcomes in women with small for gestational age pregnancies: a secondary analysis of the multicentre Prospective Observational Trial to Optimise Paediatric Health in Intrauterine Growth Restriction

Objectives: To examine associations between maternal pregnancy-specific stress and umbilical (UA PI) and middle cerebral artery pulsatility indices (MCA PI), cerebroplacental ratio, absent end diastolic flow (AEDF), birthweight, prematurity, neonatal intensive care unit admission and adverse obstetric outcomes in women with small for gestational age pregnancies. It was hypothesised that maternal pregnancy-specific stress would be associated with fetoplacental haemodynamics and neonatal outcomes. Design: This is a secondary analysis of data collected for a large-scale prospective observational study. Setting: This study was conducted in the seven major obstetric hospitals in Ireland and Northern Ireland. Participants: Participants included 331 women who participated in the Prospective Observational Trial to Optimise Paediatric Health in Intrauterine Growth Restriction. Women with singleton pregnancies between 24 and 36 weeks gestation, estimated fetal weight <10th percentile and no major structural or chromosomal abnormalities were included. Primary and secondary outcome measures Serial Doppler ultrasound examinations of the umbilical and middle cerebral arteries between 20 and 42 weeks gestation, Pregnancy Distress Questionnaire (PDQ) scores between 23 and 40 weeks gestation and neonatal outcomes. Results: Concerns about physical symptoms and body image at 35–40 weeks were associated with lower odds of abnormal UAPI (OR 0.826, 95% CI 0.696 to 0.979, p=0.028). PDQ score (OR 1.073, 95% CI 1.012 to 1.137, p=0.017), concerns about birth and the baby (OR 1.143, 95% CI 1.037 to 1.260, p=0.007) and concerns about physical symptoms and body image (OR 1.283, 95% CI 1.070 to 1.538, p=0.007) at 29–34 weeks were associated with higher odds of abnormal MCA PI. Concerns about birth and the baby at 29–34 weeks (OR 1.202, 95% CI 1.018 to 1.421, p=0.030) were associated with higher odds of AEDF. Concerns about physical symptoms and body image at 35–40 weeks were associated with decreased odds of neonatal intensive care unit admission (OR 0.635, 95% CI 0.435 to 0.927, p=0.019). Conclusions: These findings suggest that fetoplacental haemodynamics may be a mechanistic link between maternal prenatal stress and fetal and neonatal well-being, but additional research is required

LSST Science Book, Version 2.0

A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade. The Large Synoptic Survey Telescope (LSST) will have an effective aperture of 6.7 meters and an imaging camera with field of view of 9.6 deg^2, and will be devoted to a ten-year imaging survey over 20,000 deg^2 south of +15 deg. Each pointing will be imaged 2000 times with fifteen second exposures in six broad bands from 0.35 to 1.1 microns, to a total point-source depth of r~27.5. The LSST Science Book describes the basic parameters of the LSST hardware, software, and observing plans. The book discusses educational and outreach opportunities, then goes on to describe a broad range of science that LSST will revolutionize: mapping the inner and outer Solar System, stellar populations in the Milky Way and nearby galaxies, the structure of the Milky Way disk and halo and other objects in the Local Volume, transient and variable objects both at low and high redshift, and the properties of normal and active galaxies at low and high redshift. It then turns to far-field cosmological topics, exploring properties of supernovae to z~1, strong and weak lensing, the large-scale distribution of galaxies and baryon oscillations, and how these different probes may be combined to constrain cosmological models and the physics of dark energy.Comment: 596 pages. Also available at full resolution at http://www.lsst.org/lsst/sciboo