De Canarias Research Articles

Determining the Role of the Aromatic Ring of N‐Arylmethyl ent‐conduramine F‐1 in their Interactions with α‐Glucosidases by Saturation Transfer Difference NMR Spectroscopy Experiments

Glucosidases are a group of enzymes responsible of the glycosidic bond cleavage with different specificities depending on the number of monosaccharides, the position of cleavage, and the configuration of the hydroxy groups in their substrates. In particular, inhibitors of α-1,4-glucosidases have generated great interest as potential therapeutic agents for the treatment of type II diabetes (e.g., miglitol (N-2-hydroxyethyl-1-deoxynojirimycin), Glyset, Diastabol, Glucobay),1, 2 obesity,3 hepatitis B and C4, 5 and other viral diseases,6 and cancer.7

Detection of transit timing variations in excess of one hour in theKeplermulti-planet candidate system KOI 806 with the GTC

We report the detection of transit timing variations (TTVs) well in excess of one hour in the Kepler multi-planet candidate system KOI 806. This system exhibits transits consistent with three separate planets -- a Super-Earth, a Jupiter, and a Saturn -- lying very nearly in a 1:2:5 resonance, respectively. We used the Kepler public data archive and observations with the Gran Telescopio de Canarias to compile the necessary photometry. For the largest candidate planet (KOI 806.02) in this system, we detected a large transit timing variation of -103.5$\pm$6.9 minutes against previously published ephemeris. We did not obtain a strong detection of a transit color signature consistent with a planet-sized object; however, we did not detect a color difference in transit depth, either. The large TTV is consistent with theoretical predictions that exoplanets in resonance can produce large transit timing variations, particularly if the orbits are eccentric. The presence of large TTVs among the bodies in this systems indicates that KOI806 is very likely to be a planetary system. This is supported by the lack of a strong color dependence in the transit depth, which would suggest a blended eclipsing binary.

Analysis of Phenotypic Characteristics and Exposure to UV Radiation in a Group of Patients With Cutaneous Melanoma

Background Melanoma is the most serious type of skin cancer and is caused by a combination of endogenous and exogenous risk factors. Here were describe the clinical and anatomical characteristics of melanoma along with the endogenous and exogenous risk factors in 120 patients diagnosed with cutaneous melanoma in a health care area of the province of Santa Cruz de Tenerife in Spain. Patients and methods A descriptive, cross-sectional study was undertaken in patients diagnosed with melanoma between January 1999 and July 2005 in the health care area served by Hospital Universitario de Canarias. Data were collected on demographic characteristics, phenotype, sun exposure, sun protection, and actinic damage. Results Melanoma was most commonly diagnosed in women (62.5%) and lesions were most frequently located on the trunk. The most frequent tumor subtype was superficial spreading melanoma (63.3%) and 51.5% of patients were classified as having skin phototype II. Intermittent sun exposure was reported by 81.8% of patients and 50% had a moderate cumulative sun exposure (50-120 h/y). Multiple melanomas were present in 3.3% of patients. In 43% of patients, the time to diagnosis of melanoma was more than 24 months. Conclusions A substantial percentage of melanomas were associated with actinic damage. Differences were observed in the level of sun exposure according to melanoma subtype. The most common causes for concern were growth and color changes in the lesion, and a substantial number of patients waited for some time between observing these changes and consulting a doctor.

Avian mortality due to power lines in the Canary Islands with special reference to the steppe-land birds

Biodiversity is being lost worldwide at an increased rate particularly as the result of human activities and infrastructure. Avian mortality through collision with power lines has been an important topic in animal ecology research, but studies of this kind have never been undertaken in the Canary Islands, a volcanic archipelago located near the northwest African coast that has important seabird colonies, several endemic bird species and endemic races of steppe-land birds of conservation concern. During two contrasting periods in 2008 (breeding vs post-breeding), a total of 366 km of power lines were surveyed on this archipelago covering the entire distributional range of the most important steppe-land bird species (i.e. 232 km, Fuerteventura; 134 km, Lanzarote). In all, 310 carcasses representing 23 families and 26 species were detected. We estimated with distance Sampling that 25.5% and 6.3% of individuals of the total population of Houbara bustards, Chlamydotis undulata fuertaventurae, and Eurasian stone curlews, Burhinus oedicnemus insularum, respectively, were killed in a year. We encourage the Canary Islands authorities (Consejería de Medio Ambiente del Gobierno de Canarias) to try to minimize the Houbara bustard collision rate, particularly in the northern plains of Lanzarote (i.e. Jables de Famara), as a means to reduce mortality of this emblematic species in this insular environment.

Estudio de las características fenotípicas y exposición a radiación ultravioleta en pacientes diagnosticados de melanoma cutáneo

Background Melanoma is the most serious type of skin cancer and is caused by a combination of endogenous and exogenous risk factors. Here were describe the clinical and anatomical characteristics of melanoma along with the endogenous and exogenous risk factors in 120 patients diagnosed with cutaneous melanoma in a health care area of the province of Santa Cruz de Tenerife in Spain. Patients and methods A descriptive, cross-sectional study was undertaken in patients diagnosed with melanoma between January 1999 and July 2005 in the health care area served by Hospital Universitario de Canarias. Data were collected on demographic characteristics, phenotype, sun exposure, sun protection, and actinic damage. Results Melanoma was most commonly diagnosed in women (62.5%) and lesions were most frequently located on the trunk. The most frequent tumor subtype was superficial spreading melanoma (63.3%) and 51.5% of patients were classified as having skin phototype II. Intermittent sun exposure was reported by 81.8% of patients and 50% had a moderate cumulative sun exposure (50-120 h/y). Multiple melanomas were present in 3.3% of patients. In 43% of patients, the time to diagnosis of melanoma was more than 24 months. Conclusions A substantial percentage of melanomas were associated with actinic damage. Differences were observed in the level of sun exposure according to melanoma subtype. The most common causes for concern were growth and color changes in the lesion, and a substantial number of patients waited for some time between observing these changes and consulting a doctor.

Oscillator strength measurements of atomic absorption lines from stellar spectra1This article is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.2Based in part on observations made with the Mercator Telescope, operated on the island of La Palma by the Flemish Community, at the Spanish Observatorio del Roque de

Herein we develop a new method to determine oscillator strength values of atomic absorption lines with state-of-the-art detailed spectral synthesis calculations of the optical spectrum of the Sun and of standard spectral reference stars. We update the log(gf) values of 911 neutral lines observed in the KPNO–FTS flux spectrum of the Sun and high-resolution echelle spectra (R = 80 000) of Procyon (F5 IV–V) and [Formula: see text] Eri (K2 V) observed with large signal-to-noise (S/N) ratios of ∼2000 using the new Mercator–Hermes spectrograph at La Palma Observatory (Spain). We find for 483 Fe i, 85 Ni i, and 51 Si i absorption lines in the sample a systematic overestimation of the literature log(gf) values with central line depths below 15%. We employ a curve-of-growth analysis technique to test the accuracy of the new oscillator strength values and compare calculated equivalent line widths to the Moore, Minnaert, and Houtgast atlas of the Sun. The online SpectroWeb database at spectra.freeshell.org interactively displays the observed and synthetic spectra and provides the new log(gf) values together with important atomic line data. The graphical database is under development for stellar reference spectra of every spectral sub-class observed with large spectral resolution and S/N ratios.

The design of an apochromatic optical spectrograph for astronomical purposes

An optical spectrograph for use in the OGS (Optical Ground Station), a 1 m telescope in Izaña Observatory (Tenerife, Spain) and the GTC telescope at Islas Canarias observatory has been designed, built and tested. The dispersive part was designed and built at the Centro de Investigaciones en Óptica, A.C. Due to requirements from Instituto Astrofísico de Canarias this Spectrograph has an f/5 collimator and camera with a plate factor of 6.55 nm/mm. Since the resolution of the system has to have a high resolution of the order of 15 μm or less, an apochromatic design was selected. This article describes this design and its main characteristics.

Patients treated with plasmapheresis: a case review from University Hospital of the Canary Islands.

Plasmapheresis (PP) is a therapeutic apheresis technique used in the treatment of various renal and systemic diseases with varying degrees of proven clinical efficacy. To review our experience with PP at the Hospital Universitario de Canarias, focused on effectiveness and safety results in different disease groups. A retrospective-descriptive study of patients treated with PP from 01/01/2006 to 31/12/2009 at the hospital. We analysed medical histories and demographic data (sex, age), biochemical parameters, underlying disease, volume and type of replacement used in the PP sessions (5% human albumin and/or fresh frozen plasma), complications with the technique, delay in starting PP treatment after suspected clinical diagnosis, number of PP sessions received, patient mortality, degree of renal impairment and evolution of renal function. There were 51 patients studied, aged 50±18 years, of whom 60% were male; 331 PP sessions were performed. The diseases treated were grouped as: 11 vasculitis, 15 transplant immune activation, 5 haemolytic-uraemic syndrome (HUS), 7 idiopathic or thrombotic thrombocytopaenic purpura, 2 foetal Rh immunisations, 2 haematological diseases, 4 neurological diseases, among others. Overall mortality was 19.6% (n=10): 6 cases secondary to septic shock and the rest as a result of the evolution of the underlying disease, with 1 due to haemorrhagic shock in the renal biopsy area. There were no deaths in the transplant immune activation group. In the vasculitis group, there were 3 deaths (2 secondary to septic shock). Of the 10 patients who died, 9 did so within the first three months after diagnosis. Of the 26 renal biopsies performed, the most frequent indications were: vasculitis (23%), humoral rejection (42%), humoral rejection with calcineurin-inhibitor toxicity (12%) and HUS (8%), among others. Haemodialysis (HD) was required by 24 patients at the start of clinical symptoms: 9 of the 11 patients with vasculitis, 4 of the 5 patients with HUS and 5 of the 15 patients with transplant immune activation. At the end of evolution, 14 of them remained on the HD programme: 5 of the 11 patients with vasculitis, 2 of the 15 transplant patients and 3 of the 5 HUS patients. Significantly, patients who developed end kiney disease (EKD) in the vasculitis group were older and had higher creatinine at the onset of the disease. The transplant patients were monitored for anti-HLA class I or II before and after PP; there was a mean decrease of antibody titres in all but one patient; with an average decrease of 51% to 31%. In general, the PP technique was virtually free of complications. There were only 5 (3%) mild-moderate reactions to fresh plasma (perioral tingling and urticarial reactions) requiring pre-medication with steroids, but which did not lead to discontinuation of the treatment. Taking into account the wide variety of diseases that can benefit from PP and the nature of some of them, publishing our experience with this therapeutic method is of great importance. By increasing the description of case series by centre, we can add survival and renal function evidence in many uncommon diseases. Our study provides useful information for clinical practice and has also led us to reflect on future strategies to optimise outcomes in our patients.

Prevalencia de obesidad en la población gestante de Gran Canaria

Background and objective Different epidemiological studies have shown that maternal excess of weight during pregnancy is associated with adverse outcomes of pregnancy, childbirth and morbidity of the neonate. Prevalence of obesity in a pregnant population of Canary Islands is reported here. Subjects and methods The group studied was an integrated cohort of all the pregnant women being followed-up at the Materno-Infant University Hospital of the Canarias [Hospital Universitario Materno-Infantil de Canarias; HUMIC] and who concluded their gestation during the year 2008 (n = 6693). BMI was measured at the beginning of the pregnancy. Results 25.0% of the sample of pregnant women were overweight and 17.1% were obese, increasing both with age and not influenced with the educational level. Conclusions The prevalence of obesity and overweight among pregnant women from the Canary Islands is high. Among the values available from other European countries, only the UK reported values greater than our study sample.

P24.05 Time trends and associated factors to antimicrobial resistance of Escherichia coli infections in hospitalized patients. Spain, 1999–2009

P24.05 Time trends and associated factors to antimicrobial resistance of Escherichia coli infections in hospitalized patients. Spain, 1999–2009

Identification of the optical and near-infrared counterpart of GRS 1758-258

<i>Context. <i/>Understood to be a microquasar in the Galactic center region, GRS 1758-258 has not yet been unambiguously identified to have an optical/near-infrared counterpart, mainly because of the high absorption and the historic lack of suitable astrometric stars, which led to the use of secondary astrometric solutions. Although it is considered with 1E 1740.7-2942 as the prototypical microquasar in the Galactic center region, the Galactic origin of both sources has not yet been confirmed.<i>Aims. <i/>We attempt to improve previous astrometry to identify a candidate counterpart to GRS 1758-258. We present observations with the Gran Telescopio de Canarias (GTC), in which we try to detect any powerful emission lines that would infer an extragalactic origin of this source.<i>Methods. <i/>We use modern star catalogues to reanalyze archival images of the GRS 1758-258 field in the optical and near-infrared wavelengths, and compute a new astrometric solution. We also reanalyzed archival radio data of GRS 1758-258 to determine a new and more accurate radio position.<i>Results. <i/>Our improved astrometric solution for the GRS 1758-258 field represents a significant advancement on previous works and allows us to identify a single optical/near-infrared source, which we propose as the counterpart of GRS 1758-258. The GTC spectrum of this source is however of low signal-to-noise ratio and does not rule out a Galactic origin. Hence, new spectral observations are required to confirm or discard a Galactic nature.

Estudio del primer brote por Enterococcus faecium vanA en Canarias

In July, 2005 the first vancomycin-resistant Enterococcus faecium (VREF) with a genotype vanA was isolated in Hospital Universitario de Canarias (HUC). From September to December 2005, VREF vanA was isolated from another 15 patients (3 nosocomial infections and 12 rectal carriers). All of them were kidney transplant patients hospitalized in the Nephrology ward. This study describes the first VREF vanA outbreak in the HUC and the epidemiological link of the first VREF vanA isolates found in another two university hospitals in the Canary Islands. We studied a total of 22 VREF isolates by microbiological and molecular methods. Epidemiological and clinical data of the patients involved were collected. We confirmed that these VREF isolates belonged to the same clone using pulse-field gel electrophoresis (PFGE). In November 2005 and February 2006, the first VREF were isolated in two other University Hospitals in the Canary Islands and we also confirmed the link with the HUC cluster by comparison of patient-related information with the molecular typing data. These VREF isolates belonged to the ST18 associated to the Clonal Complex-17 (CC17). CC17 is the major hospital adapted lineage, representing a polyclonal population and associated to VREF outbreaks and infections in the five continents.

Rituximab for the treatment of patients with chronic lymphocytic leukemia

Rituximab for the treatment of patients with chronic lymphocytic leukemia M Gentile, E Vigna, C Mazzone, E Lucia, AG Recchia, L Morabito2, MG Bisconte, C Gentile, F Morabito1UOC di Ematologia, Azienda Ospedaliera di Cosenza, Italy; 2Servicio de Hematolog&iacute;a y Hemoterapia, Hospital Universitario de Canarias, La Laguna, Tenerife, SpainAbstract: Chronic lymphocytic leukemia (CLL) is a lymphoproliferative disorder that originates from antigen-experienced B lymphocytes that do not die and hence accumulate due to external survival signals or undergo apoptosis and are replenished by proliferating precursors. These neoplastic lymphocytes exhibit a characteristic immunophenotype of CD5+/CD19+/CD20+/HLA-DR+/CD23+/sIgdim. Thus, the CD20 antigen has been an appealing target for therapy. The introduction of the monoclonal antibody rituximab (anti-CD20) enabled an outstanding advance in CLL treatment. The introduction of this monoclonal antibody into chemotherapy regimens has dramatically improved complete response rates and progression-free survival in patients with both untreated and relapsed CLL. Although only preliminary data from phase III confirmatory trials have been reported, the FCR regimen, which combines fludarabine and cyclophosphamide with rituximab, is currently the most effective treatment regimen for CLL patients, and has also been demonstrated to significantly improve overall survival . The success of rituximab and the identification of other CLL lymphocyte surface antigens have spurred the development of a multitude of monoclonal antibodies targeting distinct proteins and epitopes in an attempt to target CLL cells more effectively.Keywords: rituximab, chronic lymphocytic leukemia, chemotherapy

The STELLA Robotic Observatory on Tenerife

The Astrophysical Institute Potsdam (AIP) and the Instituto de Astrofísica de Canarias (IAC) inaugurated the robotic telescopes STELLA‐I and STELLA‐II (STELLar Activity) on Tenerife on May 18, 2006. The observatory is located on the Izaña ridge at an elevation of 2400 m near the German Vacuum Tower Telescope. STELLA consists of two 1.2 m alt‐az telescopes. One telescope fiber feeds a bench‐mounted high‐resolution echelle spectrograph while the other telescope feeds a wide‐field imaging photometer. Both scopes work autonomously by means of artificial intelligence. Not only that the telescopes are automated, but the entire observatory operates like a robot, and does not require any human presence on site.

Mission specification in underwater robotics

This work has been partially supported by the following research projects: Project PI2007/039 funded by the Autonomous Government of Canary Islands (Gobierno de Canarias — Consejería de Educación, Cultura y Deportes, Spain) with FEDER funding; and Project TIN2008-06068 funded by the Ministerio de Ciencia e Investigación, Gobierno de España.

GTC/OSIRIS SPECTROSCOPIC IDENTIFICATION OF A FAINT L SUBDWARF IN THE UKIRT INFRARED DEEP SKY SURVEY

We present the discovery of an L subdwarf in 234 square degrees common to the UK Infrared Telescope (UKIRT) Infrared Deep Sky Survey Large Area Survey Data Release 2 and the Sloan Digital Sky Survey Data Release 3. This is the fifth L subdwarf announced to date, the first one identified in the UKIRT Infrared Deep Sky Survey, and the faintest known. The blue optical and near-infrared colors of ULAS J135058.86+081506.8 and its overall spectra energy distribution are similar to the known mid-L subdwarfs. Low-resolution optical (700-1000 nm) spectroscopy with the Optical System for Imaging and low Resolution Integrated Spectroscopy spectrograph on the 10.4 m Gran Telescopio de Canarias reveals that ULAS J135058.86+081506.8 exhibits a strong KI pressure-broadened line at 770 nm and a red slope longward of 800 nm, features characteristics of L-type dwarfs. From direct comparison with the four known L subdwarfs, we estimate its spectral type to be sdL4-sdL6 and derive a distance in the interval 94-170 pc. We provide a rough estimate of the space density for mid-L subdwarfs of 1.5x10^(-4) pc^(-3).

LOW-RESOLUTION SPECTROSCOPY OF GAMMA-RAY BURST OPTICAL AFTERGLOWS: BIASES IN THE SWIFT SAMPLE AND CHARACTERIZATION OF THE ABSORBERS

We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts (GRBs) for which spectroscopic follow-up observations have been secured. Our first objective is to measure the redshifts of the bursts. For the majority (90%) of the afterglows, the redshifts have been determined from the spectra. We provide line lists and equivalent widths (EWs) for all detected lines redward of Lyα covered by the spectra. In addition to the GRB absorption systems, these lists include line strengths for a total of 33 intervening absorption systems. We discuss to what extent the current sample of Swift bursts with OA spectroscopy is a biased subsample of all Swift detected GRBs. For that purpose we define an X-ray-selected statistical sample of Swift bursts with optimal conditions for ground-based follow-up from the period 2005 March to 2008 September; 146 bursts fulfill our sample criteria. We derive the redshift distribution for the statistical (X-ray selected) sample and conclude that less than 18% of Swift bursts can be at z > 7. We compare the high-energy properties (e.g., γ-ray (15-350 keV) fluence and duration, X-ray flux, and excess absorption) for three subsamples of bursts in the statistical sample: (1) bursts with redshifts measured from OA spectroscopy; (2) bursts with detected optical and/or near-IR afterglow, but no afterglow-based redshift; and (3) bursts with no detection of the OA. The bursts in group (1) have slightly higher γ-ray fluences and higher X-ray fluxes and significantly less excess X-ray absorption than bursts in the other two groups. In addition, the fractions of dark bursts, defined as bursts with an optical to X-ray slope βOX 39% in group (3). For the full sample, the dark burst fraction is constrained to be in the range 25%-42%. From this we conclude that the sample of GRBs with OA spectroscopy is not representative for all Swift bursts, most likely due to a bias against the most dusty sight lines. This should be taken into account when determining, e.g., the redshift or metallicity distribution of GRBs and when using GRBs as a probe of star formation. Finally, we characterize GRB absorption systems as a class and compare them to QSO absorption systems, in particular the damped Lyα absorbers (DLAs). On average GRB absorbers are characterized by significantly stronger EWs for H I as well as for both low and high ionization metal lines than what is seen in intervening QSO absorbers. However, the distribution of line strengths is very broad and several GRB absorbers have lines with EWs well within the range spanned by QSO-DLAs. Based on the 33 z > 2 bursts in the sample, we place a 95% confidence upper limit of 7.5% on the mean escape fraction of ionizing photons from star-forming galaxies. Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere, Chile, under programs 275.D-5022 (PI: Chincarini), 075.D-0270 (PI: Fynbo), 077.D-0661 (PI: Vreeswijk), 077.D-0805 (PI: Tagliaferri), 177.A-0591 (PI: Hjorth), 078.D-0416 (PI: Vreeswijk), 079.D-0429 (PI: Vreeswijk), 080.D-0526 (PI: Vreeswijk), 081.A-0135 (PI: Greiner), 281.D-5002 (PI: Della Valle), and 081.A-0856 (PI: Vreeswijk). Also based on observations made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Some of the data obtained herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck foundation.

Androgen Receptor Gene Repeat Polymorphism, Leptin And Fat Mass In Young Men And Women

The exon-1 of the androgen receptor (AR) gene contains two length polymorphisms which modify either the amount of AR protein inside the cell (GGNn, polyglycine) or its transcriptional activity (CAGn, polyglutamine). Shorter CAG and/or GGN repeats provide stronger androgen signaling, and vice versa. On the other hand, androgen levels are inversely associated with fat mass. PURPOSE: To test the hypothesis that CAG and GGN repeat AR polymorphism influences body fat and serum leptin concentrations. METHODS: The length of CAG and GGN repeats was determined by PCR and fragment length analysis, serum leptin concentration by ELISA, and fat mass with DEXA in 282 men (28.6 ± 7.6 years) and 61 women (25.5 ± 6.7 years). All subjects were healthy and physically active. Individuals were grouped as CAG short (CAGs) if harboring repeat lengths of ≤21 in men and ≤22 in women, and CAG long (CAGL) if CAG >21 in men and >22 in women. GGN was considered short (GGNs) or long (GGNL) if GGN ≤23 or >23 in men and women. RESULTS: There was no relationship between GGN and CAG repeat length and serum leptin concentration neither in women nor men. CAGs and CAGL groups had similar leptin concentrations, and GGNs and GGNL groups as well. There was no relationship between CAG repeat length and whole body fat mass, percentage of fat mass accumulated in the trunk region and percentage of body fat neither in men nor women. The GGN repeat length was not associated to fat mass or to the percentage of body fat in men. However, in women, there was a linear relationship between the length of GGN repeat microsatellite and the percentage of body fat (% fat=2.16xGGN -21.73, r=0.31, P<0.05) and a trend for a similar relationship between whole body fat mass and GGN repeat length (fat mass (kg) = 1.41xGGN - 14.97, r=0.22, P=0.09). No association between CAG or GGN repeat length and trunk fat accumulation was observed. CONCLUSIONS: A long repeat GGN polymorphism is positively associated with increased percentage of body fat in physically active young women. Supported by Ministerio de Educación y Ciencia (DEP2006-56076-C06-04/ACTI), Consejería de Educación, Cultura y Deportes del Gob. de Canarias (2006/179 0001 and FEDER), Proyecto Interreg IIIB BIOPOLIS, Fundación del Instituto Canario de Investigación del Cáncer (FICIC), Cabildo de Gran Canaria, Cabildo de Tenerife and La Caja de Canarias.

An ear turned to “The Cosmos”: 50 projects to discover the universe

AbstractIn 1609, as Galileo pointed the sky with a telescope, he observed Jupiter's satellites and changed our vision of the universe. Four hundred years later, we celebrate this event all over the world, and also in the Canaries. 2009, the International Year of Astronomy, is a very special year for the Science and Cosmos Museum (Museo de la Ciencia y el Cosmos). This was the first museum in Spain supported by a public entity, The Local Government of Tenerife (Cabildo de Tenerife), through its Autonomous Council of Museums (Organismo Autónomo de Museos y Centros), and a research centre, the Instituto de Astrofísica de Canarias. Fifteen years later, this museum, which receives 50,000 visitors a year, celebrates the International Year of Astronomy with fifty projects described in this paper.

Presentación de la cohorte "CDC de Canarias": objetivos, diseño y resultados preliminares

The Canary Islands rank first in Spain with respect to the ischaemic heart disease and diabetes mortality rates. The Islands female population leads the country in deaths from breast cancer. The "CDC de Canarias" is a general population cohort study in order to analyse the prevalence and incidence of these diseases and the exposure to their risk factors (RF) in the adult population of the archipelago. Prospective study with a random sampling of the general population, in which 6,729 individuals participated between 2000 and 2005 (aged 18-75). Anthropometric measurements were taken, and blood was drawn for the storage of serum and genetic samples. The following information was gathered through a questionnaire: eating habits, physical activity, personal and family medical history, exposure to occupational or environmental risk factors, smoking, etc. The prevalence of obesity is close to 30%, without differences between sexes, however, more male subjects were overweight than women (45 vs. 33%; p <0.001) and also presented a greater prevalence of diabetes (12 vs. 10%; p =0.005), high blood pressure (43 vs. 33%; p <0.001), excessive intake of alcohol (13 vs. 2%; p <0.001) and lack of sun protection (46 vs. 18%; p <0.001). Exposure to low levels of HDL cholesterol is more frequent in women (37 vs. 30%; p <0.001) as is also the case with a sedentary life style (71 vs. 55%; p <0.001). The exposure to the risk factors studied, including poverty, is greater in advanced age groups, except for smoking (26%) which is greater in the younger subjects. The estimate of relative risks of exposure to cardiovascular and cancer risk factors is higher in low-income social classes. The current adult population of the Canaries presents a high prevalence of exposure to risk factors for cardiovascular disease, diabetes and cancer, among which overweight, obesity and lack of exercise stand out particularly.