We report the results of Long Baseline Array observations made in 2001 of ten southern sources proposed by Mattox et al. as counterparts to EGRET >100 MeV gamma-ray sources. Source structures are compared with published data where available and possible superluminal motions identified in several cases. The associations are examined in the light of Fermi observations, indicating that the confirmed counterparts tend to have radio properties consistent with other identifications, including flat radio spectral index, high brightness temperature, greater radio variability, and higher core dominance.

We present results from a multiwavelength study of the blazar PKS 1954–388 at radio, UV, X-ray, and gamma-ray energies. A RadioAstron observation at 1.66 GHz in June 2012 resulted in the detection of interferometric fringes on baselines of 6.2 Earth-diameters. This suggests a source frame brightness temperature of greater than 2 × 1012 K, well in excess of both equipartition and inverse Compton limits and implying the existence of Doppler boosting in the core. An 8.4-GHz TANAMI VLBI image, made less than a month after the RadioAstron observations, is consistent with a previously reported superluminal motion for a jet component. Flux density monitoring with the Australia Telescope Compact Array confirms previous evidence for long-term variability that increases with observing frequency. A search for more rapid variability revealed no evidence for significant day-scale flux density variation. The ATCA light-curve reveals a strong radio flare beginning in late 2013, which peaks higher, and earlier, at higher frequencies. Comparison with the Fermi gamma-ray light-curve indicates this followed ~ 9 months after the start of a prolonged gamma-ray high-state—a radio lag comparable to that seen in other blazars. The multiwavelength data are combined to derive a Spectral Energy Distribution, which is fitted by a one-zone synchrotron-self-Compton (SSC) model with the addition of external Compton (EC) emission.

We are undertaking an observational program using the ATCA to monitor the intraday variability (IDV) of a sample of sources at 4.8 and 8.6 GHz. The sources were selected to include the known strong southern IDV sources plus a number of sources whose IDV was recently discovered. The present monitoring program will extend over a full year in order to search for any annual cycle that may be present in the long-term IDV characteristics of these sources. In this paper we discuss the observing strategy and data analysis, and present the first results from our observations.

Flux density monitoring data at 2.3 and 8.4 GHz is presented for a sample of 33 southern hemisphere GPS sources, drawn from the 2.7 GHz Parkes survey. This monitoring data, together with VLBI monitoring data, shows that a small fraction of these sources, ∼10%, vary. Their variability falls into several categories: sources whose spectral classification is, at best, ephemeral on a timescale of years; sources with a stable GPS classification that vary, but retain their classification; and a small number of sources that exhibit interstellar scintillation, but that maintain a mean GPS spectrum. Existing data on GPS sources with higher frequency peaks, ≥3 GHz, reveals that many such sources vary. However, the majority of these sources possess a GPS spectrum only during outbursts, and hence should perhaps be classified as ephemeral GPS sources. In addition, significant levels of circular polarisation have been found in a number of GPS sources, both amongst the variables and non-variables. Remarkable amongst these is PKS 1519–273, which possesses strong and variable circular polarisation, and which exhibits IDV in all Stokes parameters.

We give a classification of all the cycle types occurring in the automorphism groups of countable homogeneous graphs.

Common mental health problems are highly prevalent in primary care, the UK National Service Framework for mental health demanding that effective and accessible services be made available. Although built upon a strong evidence base, traditional psychological therapies are often limited in terms of their applicability and availability. As a consequence innovative self-help programmes are increasingly being advocated as an alternative means of managing mental health illness within primary care. This study reports the results of a three month evaluation of a self-help service provided by a busy UK urban Primary Care Trust. Levels of utilization, effectiveness and stakeholder acceptability were examined through a combination of quantitative and qualitative data. A total of 662 patients were referred to the self-help clinics over a three month period, 67% of whom attended their first appointment. The mean number of sessions per patient was 2.8 (SD = 2.4), with an average total time of 69.6 min (SD = 48.2). Mean Clinical Outcomes in Routine Evaluation (CORE-OM) scores improved significantly between baseline and three month follow-up (P < 0.001), 39% of patients demonstrating a clinically significant improvement. Both selfhelp therapists and referring general practitioners reported moderate to high satisfaction with the self-help treatment model, with the majority of patients perceiving the intervention to be appropriate to their needs. Data demonstrated that, whilst there was a clear need for a simple self-help service to be based in primary care, the ultimate success of this provision necessitates a well developed infrastructure capable of providing sufficient support and information to ensure that it is flexible and responsive to individual needs.

In February 1997 the Japanese radio astronomy satellite HALCA was launched to provide the space-borne element for the VSOP mission. HALCA provided linear baselines three-times greater than that of ground arrays, thus providing higher resolution and higher AGN brightness temperature measurements and limits. Twenty-five percent of the scientific time of the mission was devoted to the “VSOP survey” of bright, compact, extra-galactic radio sources at 5 GHz. A complete list of 294 survey targets were selected from pre-launch surveys, 91% of which were observed during the satellite's lifetime.

The major goals of the VSOP Survey are statistical in nature: to determine the brightness temperature and approximate structure, to provide a source list for use with future space VLBI missions, and to compare radio properties with other data throughout the electro-magnetic spectrum. All the data collected have now been analysed and is being prepared for the final image Survey paper. In this paper we present details of the mission, and some statistics of the images and brightness temperatures.

Extended abstract of a paper presented at Microscopy and Microanalysis 2006 in Chicago, Illinois, USA, July 30 – August 3, 2005

Summary

Background and objectives: The potential for increased drug administration errors during the transition to the International Colour Coding syringe labelling system has been highlighted. The purpose of this study was to assess the potential effects before their introduction into our department. Methods: Thirty-one anaesthetists, 19 with no previous practical experience of the new labelling system (Group 1), and 12 with previous experience (Group 2), volunteered to induce general anaesthesia for a standardized simulated patient in a designated theatre. They were presented with a scenario designed to suggest the need for a rapid sequence induction and provided with drug syringes labelled with the International Colour Coding system. All drug administrations were recorded. Active error was defined as the injection of the wrong drug. Latent error was defined as the selection of a syringe in error but stopping short of administering the drug. Results: In Group 1 a total of 107 drug injections were recorded of which 1 (0.9%) was an active error and 16 (15%) involved latent errors. Eleven anaesthetists (58%) performed at least one latent error. Group 2 had an error rate of 3%, a 6.9 (1.3–26.7) fold reduction in the rate of error (P = 0.023). Conclusions: Although only one drug was given in active error, latent errors occurred in 15% of drug administrations. The only factor conferring protection against error was prior experience of the new labelling system. The period of transition to the International Colour Coding syringe labelling system represents a time of increased risk of drug administration error.

PKS 1257—326 is one of three quasars known to show unusually large and rapid, intra-hour intensity variations, as a result of scintillation in the turbulent Galactic interstellar medium. We have measured time delays in the variability pattern arrival times at the VLA and the ATCA, as well as an annual cycle in the time-scale of variability for this source. Results of the two-station time delay observations are presented here. Implications for the scintillation of this source are discussed in the light of these results, together with results from two years of monitoring with the ATCA.

Considerable and reproducible differences were observed in the amount and duration of faecal excretion when in-bred lines of chickens were infected orally with S. enterica serovar Typhimurium at 6 weeks of age after being given a gut flora preparation when newly hatched. Similar but less pronounced results were observed with S. Enteritidis or S. Infantis. Differences in the viable numbers of the inoculated bacteria in caecal contents were detectable within 24 h of inoculation. No major differences were seen in Salmonella-specific serum IgA or IgG titres. Small differences were seen in the numbers of circulating heterophilic cells. Caecal contents taken from the more resistant lines immediately prior to challenge appeared to be no more inhibitory for Salmonella in vivo than contents taken from susceptible lines. The more resistant lines showed a slightly higher rate of intestinal flow, as indicated by the rate of production of faecal droppings, although there was no difference in the rate of emptying of the caeca. In an F1 generation resistance was dominant and not sex-linked. There was no MHC linkage or any association with SAL1, the gene implicated in resistance to systemic salmonellosis in chickens, or NRAMP1.

The in vivo determination of methane (CH4) production requires specialist equipment which is costly to maintain. Whilst the in vitro gas production technique has been demonstrated to show potential to rank diets for their methanongenic potential at maintenance planes of nutrition (Moss and Givens, 1997) no study has investigated this relationship when feedstuffs are fed ad libitum. The objective of this study was to assess the ability of the technique to predict in vivo CH4 production and animal performance from six diets differing in their chemical composition.

Background. Few studies have shown that maladaptive beliefs relate to treatment outcome.

Method. In a randomized controlled study, 87 patients with post-traumatic stress disorder (PTSD) had exposure therapy alone or cognitive restructuring alone, or both combined, or relaxation. Independent blind assessors assessed patients at pre-, mid- and post-treatment and at follow-up; at those times patients rated cognitive, behavioural and emotional aspects of their disorder.

Results. Baseline beliefs about mistrust, helplessness, meaninglessness and unjustness of the world related to baseline PTSD symptoms but did not predict treatment outcome, though improvement in certain beliefs correlated with more symptom improvement. Several ‘key’ beliefs changed after, and none before, symptoms improved. At post-treatment, sense of control and attribution of gains to personal efforts predicted maintenance of gains at follow-up.

Conclusions. Baseline beliefs and improvement in beliefs did not predict outcome. Post-treatment sense of control/internal attribution predicted maintenance of gains at follow-up. How much sense of control is produced by or causes improvement deserves testing.