Patient engagement in clinical guidelines development: input from > 1000 members of the Canadian Osteoporosis Patient Network.

Patient engagement in clinical guidelines development is essential. The results of a self-administered online survey identified themes important to people living with osteoporosis and will inform the development of Osteoporosis Canada clinical guidelines recommendations. INTRODUCTION: Patient engagement is essential in the development of high-quality and relevant guidelines for osteoporosis management. Osteoporosis Canada (OC) is updating its national clinical practice guidelines in collaboration with people living with osteoporosis in the process. METHODS: Using electronic mail, we contacted 6937 members of the Canadian Osteoporosis Patient Network (COPN) to provide input on the selection of relevant content, outcomes, and research questions via a self-administered online survey. Close-ended questions were analyzed using descriptive statistics, and conventional content analysis was conducted for open-ended questions. RESULTS: A total of 1108 individuals completed the survey (97% women, 86% stated they lived with osteoporosis). Most participants considered it critical to have recommendations on physical activity and exercise (74%), fall prevention (69%), nutrition (68%), and initial bone mineral density testing (67%). In addition to preventing fractures, over 75% of respondents stated that consideration of preserving quality of life and ability to perform daily activities, preventing admission to long-term care and fracture-related death, and avoiding serious harms from medications were essential outcomes to consider in evaluating the evidence. In terms of selection of research questions, seven themes emerged from the content analysis including pharmacotherapy, screening and monitoring, diet and supplements, education, exercise, alternative therapies, and pain management. CONCLUSIONS: Patients emphasized that autonomy, mobility, and quality of life are highly valued outcomes and must be integral to practice guideline development. As expected, guidance on pharmacotherapy, screening and monitoring, and fracture prevention were priorities identified to be included in osteoporosis management guidelines.

Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory.

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (E_{CM}=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy.

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.

Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory.

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with [Formula: see text] eV by analyzing cosmic rays with energies above [Formula: see text] eV arriving within an angular separation of approximately 15[Formula: see text]. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.

Bone disease in systemic sclerosis: outcomes and associations.

OBJECTIVES: The relationship between systemic sclerosis (SSc) and low bone mineral density (BMD) is poorly understood. The aim of this study is to improve our understanding of low bone density in SSc and its potential consequences. METHODS: Fifty consecutive unselected SSc patients were approached. Demographics, disease manifestations, BMD (lumbar spine and femoral neck) were collected at baseline and occurrence of fracture and death were collected over 2 years. The 10-year risk of osteoporotic fracture was estimated using the fracture risk assessment tool (FRAX) v2.0 with the Canadian population reference. Fisher's Exact and Student's t-tests were used to evaluate differences between patients with and without low BMD. Logistic regression was used for multivariate analysis. RESULTS: Forty-five patients had complete BMD data. Twenty-eight patients (62%) had low BMD, of those 10 (36%) had osteoporosis. There was no difference in age, sex, or disease duration between both groups. Low BMD was associated with non-Caucasian race (57% vs. 18%, p=0.01), postmenopausal status (83% vs. 47%, p<0.01), low body mass index (24.5 vs. 26.2, p=0.05). The mean 10-year risk of developing a major osteoporotic fracture and a femoral neck fracture was higher in the low BMD group (10.2% vs. 4.8%, p=0.12) and (4.1% vs. 0.5%, p = 0.16) respectively. Fourteen percent (4/28) of SSc patients with low BMD had a fracture, compared to 6% (1/17) SSc patients without low BMD. Fracture-related mortality did not occur in any patients. CONCLUSIONS: Low BMD and fracture are frequently seen in SSc patients. A number of clinically relevant factors are associated with low BMD. Further research is needed to evaluate these factors and the role of bone-specific treatments in SSc.

Measurement of the proton-air cross section at √s=57 TeV with the Pierre Auger Observatory.

We report a measurement of the proton-air cross section for particle production at the center-of-mass energy per nucleon of 57 TeV. This is derived from the distribution of the depths of shower maxima observed with the Pierre Auger Observatory: systematic uncertainties are studied in detail. Analyzing the tail of the distribution of the shower maxima, a proton-air cross section of [505±22(stat)(-36)(+28)(syst)] mb is found.

Measurement of the depth of maximum of extensive air showers above 10{18} eV.

We describe the measurement of the depth of maximum, X{max}, of the longitudinal development of air showers induced by cosmic rays. Almost 4000 events above 10;{18} eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106{-21}{+35}) g/cm{2}/decade below 10{18.24+/-0.05} eV, and (24+/-3) g/cm{2}/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm{2}. The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.

Observation of the suppression of the flux of cosmic rays above 4 x 10 (19) eV.

The energy spectrum of cosmic rays above 2.5 x 10;{18} eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index gamma of the particle flux, J proportional, variantE;{-gamma}, at energies between 4 x 10;{18} eV and 4 x 10;{19} eV is 2.69+/-0.02(stat)+/-0.06(syst), steepening to 4.2+/-0.4(stat)+/-0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.

Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory.

The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth's crust. Tau leptons from nu(tau) charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January 2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of nu(tau) at EeV energies. Assuming an E(nu)(-2) differential energy spectrum the limit set at 90% C.L. is E(nu)(2)dN(nu)(tau)/dE(nu)<1.3 x 10(-7) GeV cm(-2) s(-1) sr(-1) in the energy range 2 x 10(17) eV< E(nu)< 2 x 10(19) eV.

Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above 6 x 10(19) electron volts and the positions of active galactic nuclei (AGN) lying within approximately 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest-energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar spatial distribution are possible sources.