Physical fitness characteristics of an active firefighter population serving an urban area

Firefighters require a high level of physical fitness in order to meet the demands of their profession. While physical fitness testing is required to join the department, firefighters are not subject to further formal exercise testing throughout the duration of their careers. Active, career firefighters were tested on a variety of physical fitness measures related to body composition, strength, power, and endurance over three testing sessions. 49 firefighters (40.5 ± 8.3 yr, 89.5 ± 13.0 kg, 27.8 ± 3.6 kg/m2) were found to have a resting heart rate of 57.7 ± 8.2 bpm, blood pressure of 121.5 ± 11.9/71.5 ± 9.9 mmHg, and 24.2 ± 5.4 % body fat, culminating in 7.6 ± 6.8 points in the CPAFLA Healthy Body Composition Score. They performed 31.4 ± 11.6 pushups and scored 15.6 ± 1.6 on the 21-point Functional Movement Screen. A subset of participants also completed the Wingate Anaerobic Test, producing 10.6 ± 1.1 W/kg at peak revolutions and averaging 7.4 ± 1.0 W/kg of power with a fatigue index of 49.7 ± 8.7% over the test duration. Maximum strength, as measured by torque produced in a 60°/s isotonic, concentric contraction was 3.0 ± 0.7 Nm/kg for the quadriceps and 1.0 ± 0.1 Nm/kg for the bicep. Measures of core torso strength included the 60° abdominal endurance test (153.8 ± 94.2 s) and Biering-Sorensen test (113.4 ± 48.6 s) for back extensor endurance. Vertical jump was found to be 50.0 ± 9.6 cm. VO2 max was 42.2 ± 6.5 ml O2/kg/min while VO2 at the anaerobic threshold was 33.3 ± 8.2 ml O2/kg/min. Many of the measurements taken displayed large ranges and though many firefighters performed above-average, there were a number who did not. The contrast between the highest and lowest performers for many measures suggests that there may be a small, but significant, portion of the population that do not possess the requisite fitness to optimally perform their job responsibilities. This is cause for concern and may be mitigated by implementation of mandatory training and testing programs. Previous studies examining firefighter fitness have often used a young sample with little experience and fragmented testing while this report assessed greater numbers of senior firefighters and performed a more comprehensive range of testing. This is the first report of firefighter performance on Wingate tests, upper- and lower-body peak torque characteristics, and other performance and body composition characteristics. This data along with the other fitness measures assessed in this study will provide comprehensive baseline data to inform development of fitness training and maintenance protocols for active firefighters

Physical fitness characteristics of a front-line firefighter population

Firefighters require a high level of physical fitness in order to meet the demands of their profession. While physical performance testing is required to join the department, firefighters are not subject to further formal exercise or performance testing throughout the duration of their careers. The purpose of the present study was to gather information regarding the physical fitness of front-line Canadian firefighters, to determine whether a testing battery predictive of both performance and future injury risk is viable, and to make recommendations regarding the format of fitness testing and training programs for front-line firefighters. Front-line, career firefighters were tested on a variety of physical fitness measures related to body composition, strength, power, and endurance over three testing sessions. Large ranges of data were found for many of the measures taken and tests performed. Body fat percentage had the most significant correlations with other performance tests while performance in the pushup test and vertical jump correlated strongly with many of the more sophisticated fitness tests. Some firefighters may not possess adequate fitness levels to optimally perform their job responsibilities. Simple field tests may form the basis of predictive testing batteries for both fitness and future injury risk, though further research is needed

Observaciones sobre las madrigueras y comportamiento enterrador de Brachynotus gemmellari y otras especies de los fondos de Squilla en Ancona, Adriático Central

The paper presents information on the burrows of a number of species that occur on Squilla grounds in the coastal Adriatic off Ancona, Italy. The burrows and burrowing behaviour of Brachynotus gemmellari are described for the first time. For Upogebia tipica, Solecurtus strigilatus and Gobius niger, the observations add to sparse burrow information in the literature. Little is known of the burrows of Echiura in the Mediterranean: those of two species are briefly described from surface features.Este trabajo presenta información sobre las madrigueras de diversas especies presentes en los fondos de Squilla en las costas de Ancona, Italia, en el Adriático central. Se describen por vez primera las madrigueras y el comportamiento excavador de Brachynotus gemmellari. En el caso de Upogebia tipica, Solecurtus strigilatus y Gobius niger, las presentes observaciones se añaden a información dispersa sobre las madrigueras de Echiura en el Mediterráneo: se describen brevemente las de dos especies a partir de características de la superfície

First optical validation of a Schwarzschild Couder telescope: the ASTRI SST-2M Cherenkov telescope

The Cherenkov Telescope Array (CTA) represents the most advanced facility designed for Cherenkov Astronomy. ASTRI SST-2M has been developed as a demonstrator for the Small Size Telescope in the context of the upcoming CTA. Its main innovation consists in the optical layout which implements the Schwarzschild-Couder configuration and is fully validated for the first time. The ASTRI SST-2M optical system represents the first qualified example for two mirrors telescope for Cherenkov Astronomy. This configuration permits to (i) maintain a high optical quality across a large FoV (ii) de-magnify the plate scale, (iii) exploit new technological solutions for focal plane sensors. The goal of the paper is to present the optical qualification of the ASTRI SST-2M telescope. The qualification has been obtained measuring the PSF sizes generated in the focal plane at various distance from the optical axis. These values have been compared with the performances expected by design. After an introduction on the Gamma Astronomy from the ground, the optical design and how it has been implemented for ASTRI SST-2M is discussed. Moreover the description of the setup used to qualify the telescope over the full field of view is shown. We report the results of the first--light optical qualification. The required specification of a flat PSF of $\sim 10$ arcmin in a large field of view ~10 deg has been demonstrated. These results validate the design specifications, opening a new scenario for Cherenkov Gamma ray Astronomy and, in particular, for the detection of high energy (5 - 300 TeV) gamma rays and wide-field observations with CTA.Comment: 6 pages, 5 figure

The EEE Project

The new experiment ``Extreme Energy Events'' (EEE) to detect extensive air showers through muon detection is starting in Italy. The use of particle detectors based on Multigap Resistive Plate Chambers (MRPC) will allow to determine with a very high accuracy the direction of the axis of cosmic ray showers initiated by primaries of ultra-high energy, together with a high temporal resolution. The installation of many of such 'telescopes' in numerous High Schools scattered all over the Italian territory will also allow to investigate coincidences between multiple primaries producing distant showers. Here we present the experimental apparatus and its tasks.Comment: 4 pages, 29th ICRC 2005, Pune, Indi

Measuring primordial gravitational waves from CMB B-modes in cosmologies with generalized expansion histories

We evaluate our capability to constrain the abundance of primordial tensor perturbations in cosmologies with generalized expansion histories in the epoch of cosmic acceleration. Forthcoming satellite and sub-orbital experiments probing polarization in the CMB are expected to measure the B-mode power in CMB polarization, coming from PGWs on the degree scale, as well as gravitational lensing on arcmin scales; the latter is the main competitor for the measurement of PGWs, and is directly affected by the underlying expansion history, determined by the presence of a DE component. In particular, we consider early DE possible scenarios, in which the expansion history is substantially modified at the epoch in which the CMB lensing is most relevant. We show that the introduction of a parametrized DE may induce a variation as large as 30% in the ratio of the power of lensing and PGWs on the degree scale. We find that adopting the nominal specifications of upcoming satellite measurements the constraining power on PGWs is weakened by the inclusion of the extra degrees of freedom, resulting in a reduction of about 10% of the upper limits on r in fiducial models with no GWs, as well as a comparable increase in the error bars in models with non-zero r. Moreover, we find that the inclusion of sub-orbital CMB experiments, capable of mapping the B-mode power up to the angular scales affected by lensing, can restore the forecasted performances with a cosmological constant. Finally, we show how the combination of CMB data with Type Ia SNe, BAO and Hubble constant allows to constrain simultaneously r and the DE quantities in the parametrization we consider, consisting of present abundance and first redshift derivative of the energy density. We compare this study with results obtained using the forecasted lensing potential measurement precision from CMB satellite observations, finding consistent results.Comment: 17 pages, 9 figures, accepted for publication by JCAP. Modified version after the referee's comment

Photophysical and structural characterisation of in situ formed quantum dots

Conjugated polymer–semiconductor quantum dot (QD) composites are attracting increasing attention due to the complementary properties of the two classes of materials. We report a convenient method for in situ formation of QDs, and explore the conditions required for light emission of nanocomposite blends. In particular we explore the properties of nanocomposites of the blue emitting polymer poly[9,9-bis(3,5-di-tert-butylphenyl)-9H-fluorene] together with cadmium sulphide (CdS) and cadmium selenide (CdSe) precursors. We show the formation of emissive quantum dots of CdSe from thermally decomposed precursor. The dots are formed inside the polymer matrix and have a photoluminescence quantum yield of 7.5%. Our results show the importance of appropriate energy level alignment, and are relevant to the application of organic–inorganic systems in optoelectronic devices