bluuebunny/crossref_metadata_2025_split huggingface dataset:
The Non-Subscription Controversy amongst Dissenters in 1719: the Salters' Hall Debate
Authors: Thomas Roger 
Published: March 2011

It was as a breath of fresh air that the first news of the debates at Salters' Hall came to a young minister in a remote country village in Somerset, where he had found asylum because he had deviated slightly from the received Calvinism of his day and been made to feel the oppressiveness of the orthodox atmosphere of Dissenting congregations in the neighbouring county of Devon. When the news came he had recently seen two of the four Exeter ministers, James Peirce and Joseph Hallett ejected by the Trustees from the city meeting houses as the result of what seemed to him a vendetta led by a certain John Ball, minister at Honiton. It is with evident exhilaration, therefore, that on the first news of the Salters' Hall debates he wrote to a friend:‘Mr. [Ball]'s conduct with respect to Mr. Peirce and Mr. Hallet, will render him infamous throughout the kingdom. … Blessed be God, that he has stirred up such a noble spirit of Christian liberty in London: where it was carried in a meeting of above an hundred ministers, at Salters-Hall, that no human tests, articles, or interpretations should be urged as the trial of a man's orthodoxy; and that no minister should be condemned as heterodox, or an heretick, unless he taught, &c. contrary to express scripture. This was the substance of one part of their determination.’
The Heretics Combatted by Ignatius of Antioch
Authors: Molland Einar 
Published: March 2011

In all the Ignatian epistles, except the Epistle to the Romans, we find polemical remarks and warnings against heretical tendencies which threatened the churches of Asia Minor.It is not quite easy to obtain a clear picture of the heretics combatted by Ignatius. One point only is evident: their docetism. They considered Christ's life on earth, his birth, his human body, his death and resurrection as mere appearance.
The Impact of Impaired “Theory of Mind” on Social Interactions in Schizophrenia
Authors: Kosmidis Mary H. , Giannakou Maria , Garyfallos Giorgos , Kiosseoglou Grigoris , Bozikas Vassilis P. 
Published: March 2011

AbstractGiven the importance of social dysfunction in schizophrenia, many studies have explored how social cognition, and, particularly, Theory of Mind (ToM) may affect patients’ social interactions. In the present study, we investigated the impact of ToM deficits on social interactions, taking into account overall neuropsychological functioning as well as clinical and demographic characteristics. We assessed 28 patients with schizophrenia and 30 healthy participants on a series of tasks including tests of ToM, neuropsychological tests focused on functions potentially relevant to ToM and role plays as an indicator of social interactions. Patients performed more poorly than healthy controls across most ToM and some of the neuropsychological tests. Correlations and hierarchical regression analyses indicated the impact of some, but not all, facets of ToM on patients’ social interactions, over and above neuropsychological functioning, positive and negative symptom ratings, duration of illness and demographic characteristics. These findings suggest that remediation of ToM deficits in patients with schizophrenia may help to improve their social interactions. (JINS, 2011, 17, 511–521)
Recovered or dead? A Swedish study of 321 persons surveyed as severely mentally ill in 1995/96 but not so ten years later
Authors: Arvidsson H. 
Published: March 2011

Aim.The aim was to follow-up a group of persons who were considered severely and persistently mentally ill (SMI) at the time of the 1995 Swedish mental health-care reform but not so ten years later.Methods.Surveys were conducted in 1995/96 and 2006 in an area of Sweden. Of 602 persons surveyed as SMI in 1995/96, 321 were not found to be so in a similar survey in 2006. These persons were followed up concerning death rates and causes, as well as concerning recovery and present care. Comparisons between subgroups were made using the results of interviews conducted in 1995/96.Results.Nineteen percent of the persons considered SMI in 1995/96 were recovered in 2006 in the sense that they no longer were considered SMI. The only variable found to predict recovery was diagnosis. Half of the persons in the sample given a diagnosis of neurosis were recovered but only 6% of those given a diagnosis of psychosis. Death rates and death causes seemed to be in line with previous research.Conclusions.Relatively few persons were considered recovered after ten years. Most persons in the sample were still in contact with care and services.
Risk factors for postoperative depression in 150 subjects treated for drug-resistant focal epilepsy
Authors: Barbieri V. , Cardinale F. , Luoni A. , Russo G. L. , Francione S. , Tassi L. , Sartori I. , Castana L. , Scarone S. , Gambini O. 
Published: March 2011

Objective.The primary goal was to identify risk factors for post-surgical depression in subjects operated on for drug-resistant epilepsy. Secondary goals were to confirm the high rate of depression in subjects suffering from epilepsy (prior to surgery) and to look for first post-surgical depressive episode.Methods.Case series study of 150 subjects surgically treated for partial epilepsy (side of surgery: 72 right, 78 left; site of surgery: 97 Unilobar Temporal, 17 Unilobar Frontal, 14 Posterior, 22 Multilobar). All subjects routinely had three psychiatric evaluations: before surgery (baseline) and at 6 and 12 months after surgery. Psychiatric diagnoses were made according to DSM-IV-TR criteria. Bivariate (Fisher exact test and Kruskal–Wallis rank sum test) and multivariate (logistic regression model fitting) analyses were performed.Results.Thirty-three (22%) subjects had post-surgical depressive episodes, 31 of them in the first 6 months. Fourteen out of 33 experienced depression for the first time. Post-surgical depressive episodes are not associated with gender, outcome on seizures, side/site of surgical resection, histological diagnosis, psychiatric diagnoses other than depression. Depressive episodes before surgery and older age at surgery time are risk factors for post-surgical depression (p = 0.0001 and 0.01, respectively, at logistic regression analysis). No protective factors were identified.Conclusions.Our data show that lifetime depressive episodes and older age at surgery time are risk factors for post-surgery depression. Moreover, a prospective study could be useful in order to assess whether depression is really a consequence of surgery.
Mapping the Hidden Universe: The Galaxy Distribution in the Zone of Avoidance
Authors: Kraan-Korteweg Renée C. , Juraszek Sebastian 
Published: March 2011

AbstractDue to the foreground extinction of the Milky Way, galaxies become increasingly faint as they approach the Galactic Equator creating a ‘zone of avoidance’ (ZOA) in the distribution of optically visible galaxies of about 25%. A ‘whole-sky’ map of galaxies is essential, however, for understanding the dynamics in our local Universe, in particular the peculiar velocity of the Local Group with respect to the Cosmic Microwave Background and velocity flow fields such as in the Great Attractor (GA) region. The current status of deep optical galaxy searches behind the Milky Way and their completeness as a function of foreground extinction will be reviewed. It has been shown that these surveys—which in the mean time cover the whole ZOA (Figure 2)—result in a considerable reduction of the ZOA from extinction levels of AB =1m.0 (Figure 1) to AB =3m.0 (Figure 3). In the remaining, optically opaque ZOA, systematic HI surveys are powerful in uncovering galaxies, as is demonstrated for the GA region with data from the full sensitivity Parkes Multibeam HI survey (300°≤l≤332°, ∣b∣≤5°.5, Figure 4).
Neutrino Telescopes in Antarctica
Authors: Adams Jenni 
Published: March 2011

AbstractIt is hoped that in the near future neutrino astronomy will reach throughout and beyond our galaxy and make measurements relevant to cosmology, astrophysics, cosmic-ray and particle physics. The construction of a high-energy neutrino telescope requires a huge volume of very transparent, deeply buried material such as ocean water or ice, which acts as the medium for detecting the particles. I will describe two experiments using Antarctic ice as this medium: the AMANDA experiment employing photomultiplier tubes and RICE utilising radio receivers.
Infrared and Submillimetre Observing Conditions on the Antarctic Plateau
Authors: Hidas Marton G. , Burton Michael G. , Chamberlain Matthew A. , Storey John W. V. 
Published: March 2011

AbstractThe Antarctic Plateau provides the best terrestrial sites for infrared (IR) and submillimetre (sub-mm) astronomy. In this paper we examine the relative importance of temperature, aerosol content and precipitable water vapour to determine which parameters have the greatest influence on atmospheric transmission and sky brightness. We use the atmospheric modelling program MODTRAN to model the observed sky spectrum at the South Pole from the near-IR to the sub-mm. We find that temperature and aerosol content determine the quality of near-IR observing conditions, aerosol content is the determining factor in the mid-IR up to 20 μm, while at longer wavelengths, including the sub-mm, it is the water vapour content that matters. Finding a location where aerosol levels are minimised is a key constraint in determining the optimum site on the Antarctic Plateau for an IR observatory.
Observations from Australasia using the Gravitational Microlensing Technique
Authors: Yock Philip 
Published: March 2011

AbstractThe astronomical technique of gravitational microlensing provides new opportunities to make measurements which are difficult or impossible by other methods, or which are complementary to those obtained more directly. These include detection of dark matter, determination of galactic structure, measurement of limb darkening of stars, and searches for extra-solar planets. The technique is best suited to the southern sky, and several observations have been made from Australasia. A sample of these observations is described here. A case is also made for a telescope at the Antarctic dedicated to gravitational microlensing.
Redshift Surveys and Cosmology: A Summary of the Dunk Island Conference
Authors: Colless Matthew 
Published: March 2011

AbstractRedshift surveys constitute one of the prime tools of observational cosmology. Imaging surveys of the whole sky are now available at a wide range of wavelengths, and provide a basis for the new generation of massive redshift surveys currently in progress. The very large datasets produced by these surveys call for new and sophisticated approaches to the analysis of large-scale structure and the galaxy population. These issues, and some preliminary results from the new redshift surveys, were discussed at the second Coral Sea Cosmology Conference, held at Dunk Island on 24–28 August 1999. This is a summary of the conference; the full conference proceedings are on the WWW at http://www.mso.anu.edu.au/DunkIsland/Proceedings.
Standard Stars: CCD Photometry, Transformations and Comparisons
Authors: Sung Hwankyung , Bessell Michael. S. 
Published: March 2011

AbstractWe discuss variations of the atmospheric extinction coefficients and transformation equations to the standard UBVRI system based on observations of standard stars during 1996–1997 at Siding Spring Observatory using a thinned SITe CCD and coloured glass filters. In the transformation from the initial natural system to the Landolt version of the standard system, a large nonlinear term related to the Balmer discontinuity was required for the U transformation. We then modified the U filter, and the subsequent transformation to the SAAO version of the standard UBVRI system had only small nonlinear correction terms for U, B, and I. The correction terms relating to U and B are evidently due to the Balmer discontinuity, while that relating to I seems to be due to the Paschen discontinuity at λ ≈ 8200 Å. We also compared the results with Landolt's observations, and confirmed the difference between the two sets of standard stars (SAAO and Landolt).
Impact of Observatory Visitor Centres on the Public's Understanding of Astronomy
Authors: Burtnyk Kimberly 
Published: March 2011

AbstractIn recent years, formal astronomy education has become an issue of great interest. Indeed, some boards of education now officially include astronomy in their curricula. While formal astronomy education continues to gain attention, informal astronomy education for the general public has rarely been addressed. One valuable source of informal astronomy education is the observatory ‘visitor centre’. Observatories draw thousands of visitors each year, and as such represent a golden opportunity for the astronomical community to communicate directly with the public. This paper summarises an exploratory study of the cognitive and affective impacts of a visit to the visitor centres located at Mount Stromlo and Siding Spring Observatories.
Long-term Monitoring of Molonglo Calibrators
Authors: Gaensler B. M. , Hunstead R. W. 
Published: March 2011

AbstractBefore and after every 12 hour synthesis observation, the Molonglo Observatory Synthesis Telescope (MOST) measures the flux densities of ∼5 compact extragalactic radio sources, chosen from a list of 55 calibrators. From 1984 to 1996, the MOST made some 58,000 such measurements. We have developed an algorithm to process this dataset to produce a light curve for each source spanning this thirteen-year period. We find that 18 of the 55 calibrators are variable, on time scales between one and ten years. There is the tendency for sources closer to the Galactic Plane to be more likely to vary, which suggests that the variability is a result of refractive scintillation in the Galactic interstellar medium. The sources with the flattest radio spectra show the highest levels of variability, an effect possibly resulting from differing orientations of the radio axes to the line of sight.
STaRS: Space Science Teaching and Resource Site
Authors: Mackie Glen 
Published: March 2011

AbstractA World Wide Web site has been developed by astronomers and educators at Carter Observatory. STaRS is the Space science Teaching and Resource Site (www.vuw.ac.nz/~mackie/STaRS.html) and its objectives are to (1) present astronomy investigations for 8 to 12 year olds and (2) promote topical astronomy and space science studies for a general audience. The educational investigations drawn from local and international sources and the resources provided to teachers are described. The structure and content of the general audience pages are summarised. Details of site promotion and usage and critical comment from users and educators are given.
Astronomy Laboratory: What are we going to make today?
Authors: Feteris Susan , Hutton Don 
Published: March 2011

AbstractThe workshop programme of a new first year university astronomy subject with low capital costs incorporates diverse learning experiences: planisphere, time around the world, sundial, telescope, computer simulation, planetarium, spectroscope, poster, debate, night-time observatory trip. The practical activities, used to address specific learning objectives, emerged clearly as a major strength of the subject as evaluated by the mixed student cohort.
Assessment Techniques in an Online Astronomy Course
Authors: Mazzolini Margaret 
Published: March 2011

AbstractTeaching an astronomy course online involves many challenges. One major challenge is the design of appropriate, practical and challenging forms of assessment which focus both on the astronomy content of the course and on the particular astronomy interests of the enrollees. This paper will discuss the assessment approaches we have chosen for our introductory-level subjects, the outcomes obtained and the reactions of the course participants. In particular, some of the wide variety of project work undertaken by the participants will be described.
Preparing Astronomy Majors for the Job Market of the New Millennium
Authors: Migenes Victor 
Published: March 2011

AbstractIn the past few years the American Physical Society (APS) has conducted a number of surveys among the graduate student population in the US and also among young researchers. The purpose was to get an idea of the career expectations of the students and how these are met later on in their life. Two of the conclusions were: (1) students want to work in a research environment, preferably academic, and (2) graduate and undergraduate programs are not preparing them well for the different challenges and goals found in industry, the private sector and national laboratories. Jobs in academia, especially tenured positions, have been difficult to obtain forcing many students to give up on their goals after one or two postdoctoral positions. Some have found jobs in other sectors but others feel frustrated that their careers have not met their expectations and are poorly ‘prepared’ for other options. In the areas of Physics and Astronomy there is not much of a job market without graduate studies. So most students must continue graduate work, in these or other fields, in order to compete well in the job market. Graduate and undergraduate programs must become more responsible for the present state of affairs and for implementing improvements. This can be done by broadening the scope of the present programs so that a student is better prepared to face the challenges of other job opportunities. We present here a BSc program designed by astronomers and physicists, at the University of Guanajuato, to try to address some of these concerns and better prepare the students for either continuing with graduate studies or finding employment in an ever-changing job market.
Astro Concepts: Learning Underlying Physics Principles in Conceptual Astronomy
Authors: Mazzolini Margaret , Halls Bronwyn 
Published: March 2011

AbstractAstro Concepts is a project within Swinburne University of Technology in Melbourne developing browser-based software modules on Optical Telescopes, Nebulae and Binary Stars. The modules are designed to enhance students' understanding of basic physics concepts, which underlie introductory-level conceptual astronomy courses. When complete, the Astro Concepts modules will be available for use in university courses in introductory astronomy, introductory physics teaching, secondary teaching and online astronomy education. The strategy outlined here is to obtain a reasonable level of understanding of the necessary physics concepts by presenting them embedded in relevant and interesting astronomy contexts, and by the use of an engaging educational approach requiring active learning by the student.
Pre-course Results from the Astronomy Diagnostic Test
Authors: Hufnagel Beth , Slater Timothy , Deming Grace , Adams Jeff , Adrian Rebecca L. , Brick Christine , Zeilik Michael 
Published: March 2011

AbstractWe present selected results from the January 1999 semester pre-course administration of the Astronomy Diagnostic Test (ADT), a research-based, multiple-choice instrument that assesses student knowledge and understanding about selected concepts in astronomy. The ADT is valid for undergraduate non-science majors taking an introductory astronomy course. This paper briefly summarises the development and validation processes, which included pre-course administration to 1557 students in 22 classes attending 17 various post-secondary institutions across the USA in the January 1999 semester. Two interesting results of the ADT's pre-course administration are (1) the average class score of the ADT is about the same (32%) regardless of type of post-secondary institution or class size and (2) there is a significant gender difference, with women scoring an average of 28% and men 38%, with the standard errors both less than 1%. The current version of the ADT (Version 2 dated 21 June 1999) and a comparative by-class database is available to astronomy instructors at the (USA) Association of Astronomy Educators' and the National Institute for Science Education's (NISE) WebPages.
A Cosmic Ray Muon Detector for Astronomy Teaching
Authors: Clay R. W. , Kurban Z. , Maghrabi A. H. , Wild N. R. 
Published: March 2011

AbstractPractical astronomy is usually taught using optical telescopes or, more rarely, radio telescopes. For a similar cost, complementary studies may be made of astrophysical particles through the use of a modestly sized muon detector. Such a detector records the arrival of cosmic ray particles that have traversed the heliosphere and the rate of muon detections reflects the flux of those particles. That flux is controlled by the day to day properties of the heliosphere which is in a state of constant change as the outflowing solar wind is affected by solar activity. As a consequence, a laboratory muon detector, whose count rate depends on the state of the heliosphere, can be an interesting and useful teaching tool that is complementary to optical or radio studies of the Sun.
Large-scale Structures behind the Southern Milky Way from Observations of Partially Obscured Galaxies
Authors: Kraan-Korteweg R. C. , Woudt P. A. , Henning P. A. 
Published: March 2011

AbstractWe report here on extragalactic large-scale structures uncovered by a deep optical survey for galaxies behind the southern Milky Way. Systematic visual inspection of the ESO/SRC survey revealed over 10000 previously unknown galaxies in the region 265° ≲ l ≲ 340°, ∣b∣ ≲ 10°. With subsequently obtained redshifts of more than 10% of these galaxies, new structures across the Milky Way are unveiled, such as a filament at ∼2500 km s−1 connecting to the Hydra and Antlia clusters, a shallow extended superduster in Vela (∼6000 km s−1), and a nearby (4882 km s−1), very massive (M ∼ 2 – 5 × 1015M☉), rich Coma-like cluster which seems to constitute the previously unidentified centre of the Great Attractor.The innermost part of the Milky Way, where the foreground obscuration in the blue is AB ≳ 5m, i.e. where HI-column densities Nhi ≳ 6·1021cm−2, remains fully opaque. In this approximately 8° wide strip, the forthcoming blind HI survey with the multibeam system at Parkes will provide the only tool to unveil this part of the extragalactic sky.
HI Searches in the Zone of Avoidance: Past and Present (and Future)
Authors: Henning P. A. 
Published: March 2011

AbstractIn the regions of highest optical obscuration and infrared confusion, only 21-cm emission can be used to find galaxies in the Zone of Avoidance. A feasibility study conducted with the 300-ft telescope successfully uncovered galaxies which seem to be consistent with populations of optically-selected low surface brightness galaxies. A complete survey is currently being conducted in the north with the Dwingeloo telescope. The big breakthrough should come in the south, however, with the advent of the Parkes telescope multibeam system.
Cosmology using the Parkes HI Multibeam Southern Sky Survey
Authors: Thomas P. A. 
Published: March 2011

AbstractI discuss the implications of the Parkes Multibeam Southern Sky HI Survey for cosmology. It will determine the local mass function of HI clouds, detecting several hundred per decade of mass. Each of these will come with a redshift and, for the more massive clouds, an estimate of the velocity width. This will provide an ideal database for peculiar motion studies and for measurements of biasing of galaxies relative to the underlying matter distribution.