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See detailEuropean Foreign Exchange Risk Exposure
Muller, Aline ULg; Verschoor, Willem

in European Financial Management (2006), 12(2), 195-220

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See detailEuropean geriatric examination. Looking in the future
Petermans, Jean ULg

Conference (2013, January)

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See detailEuropean geriatric examination. Looking in the future
Petermans, Jean ULg

Speech (2013)

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See detailEuropean guidance for the diagnosis and management of osteoporosis in postmenopausal women--what is the current message for clinical practice?
Kanis, John A; Reginster, Jean-Yves ULg

in Polskie Archiwum Medycyny Wewnetrznej (2008), 118(10), 538-40

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See detailEuropean guidance for the diagnosis and management of osteoporosis in postmenopausal women.
Kanis, J. A.; McCloskey, E. V.; Johansson, H. et al

in Osteoporosis international : a journal established as result of cooperation between the European Foundation for Osteoporosis and the National Osteoporosis Foundation of the USA (2013), 24(1), 23-57

Guidance is provided in a European setting on the assessment and treatment of postmenopausal women at risk of fractures due to osteoporosis. INTRODUCTION: The International Osteoporosis Foundation and ... [more ▼]

Guidance is provided in a European setting on the assessment and treatment of postmenopausal women at risk of fractures due to osteoporosis. INTRODUCTION: The International Osteoporosis Foundation and European Society for Clinical and Economic Aspects of Osteoporosis and Osteoarthritis published guidance for the diagnosis and management of osteoporosis in 2008. This manuscript updates these in a European setting. METHODS: Systematic literature reviews. RESULTS: The following areas are reviewed: the role of bone mineral density measurement for the diagnosis of osteoporosis and assessment of fracture risk, general and pharmacological management of osteoporosis, monitoring of treatment, assessment of fracture risk, case finding strategies, investigation of patients and health economics of treatment. CONCLUSIONS: A platform is provided on which specific guidelines can be developed for national use. [less ▲]

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See detailEuropean guidance for the diagnosis and management of osteoporosis in postmenopausal women.
Kanis, J. A.; Burlet, N.; Cooper, C. et al

in Osteoporosis International (2008), 19(4), 399-428

SUMMARY: Guidance is provided in a European setting on the assessment and treatment of postmenopausal women with or at risk from osteoporosis. INTRODUCTION: The European Foundation for Osteoporosis and ... [more ▼]

SUMMARY: Guidance is provided in a European setting on the assessment and treatment of postmenopausal women with or at risk from osteoporosis. INTRODUCTION: The European Foundation for Osteoporosis and Bone disease (subsequently the International Osteoporosis Foundation) published guidelines for the diagnosis and management of osteoporosis in 1997. This manuscript updates these in a European setting. METHODS: The following areas are reviewed: the role of bone mineral density measurement for the diagnosis of osteoporosis and assessment of fracture risk; general and pharmacological management of osteoporosis; monitoring of treatment; assessment of fracture risk; case finding strategies; investigation of patients; health economics of treatment. RESULTS AND CONCLUSIONS: A platform is provided on which specific guidelines can be developed for national use. [less ▲]

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See detailEuropean guidelines for the management of low back pain
Van Tulder, M.; Kovacs, F.; Müller, G. et al

in Acta Orthopaedica Scandinavica. Supplement (2002), 73((Suppl 305)), 20-25

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See detailThe European Hale-Bopp Team Observations of Comet Hale-Bopp
Cremonese, G.; Arpigny, Claude ULg; Manfroid, Jean ULg et al

in Bulletin of the American Astronomical Society (1997, July 01)

The poster reports some preliminary results obtained by the the European HB Team during an observational campaign, carried out with a substantial number of telescopes on the Canary Islands within a ... [more ▼]

The poster reports some preliminary results obtained by the the European HB Team during an observational campaign, carried out with a substantial number of telescopes on the Canary Islands within a programme supported by the European Union. The observations were devoted to a variety of spectroscopic and photometric topics and have already provided important results. A highlight of this work was the discovery of a third tail composed of neutral sodium and the detection of substantial amount of sodium in the dust tail. Potassium was found in the nuclear region and it was possible to obtain good definition of the rotation state of the comet nucleus. Other results are expected from the analysis of high resolution spectra, for instance the carbon isotopic ratio, the relative abundance of some ions in the coma, and of the very large collection of images from different telescopes with which the complex jet structure of the near nucleus region was monitored. [less ▲]

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See detailEuropean Initiative for the Exchange of Young Officers inspired by Erasmus
Paile, Sylvain ULg

in Weisserth, Hans-Bernhard; Rehrl, Jochen (Eds.) CSDP Handbook - The Common Security and Defence Policy of the European Union (2012)

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See detailEuropean Initiative for the Exchange of Young Officers inspired by Erasmus
Paile, Sylvain ULg

in Rehrl, Jochen; Weisserth, Hans-Bernhard (Eds.) Handbook on CSDP (2012)

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See detailEuropean Institute on Immigration Research (FIERI) Forum
Martiniello, Marco ULg

Scientific conference (2001, March 23)

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See detailEuropean inter-institutional impact study of MammaPrint
CUSUMANO, Giuseppe ULg; Generali, D; Ciruelos, E et al

Poster (2012)

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See detailThe European Interferometry Initiative (EII) within OPTICON
Surdej, Jean ULg; Chelli, A.; Garcia, P. et al

in Epchtein, N.; Candidi, M. (Eds.) EAS Publications Series, Volume 25 (2007)

We present a brief summary of past Network and Joint Research Activities of the European Interferometry Initiative Consortium in FP6 within OPTICON, of a Marie Curie exchange and education project within ... [more ▼]

We present a brief summary of past Network and Joint Research Activities of the European Interferometry Initiative Consortium in FP6 within OPTICON, of a Marie Curie exchange and education project within the EU program and of planned activitiesinFP7. [less ▲]

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See detailThe European Large Area ISO Survey - I. Goals, definition and observations
Oliver, Seb; Rowan-Robinson, Michael; Alexander, D. M. et al

in Monthly Notices of the Royal Astronomical Society (2000), 316

We describe the European Large Area ISO Survey (ELAIS). ELAIS was the largest single Open Time project conducted by ISO, mapping an area of 12deg[SUP]2[/SUP] at 15μm with ISOCAM and at 90μm with ISOPHOT ... [more ▼]

We describe the European Large Area ISO Survey (ELAIS). ELAIS was the largest single Open Time project conducted by ISO, mapping an area of 12deg[SUP]2[/SUP] at 15μm with ISOCAM and at 90μm with ISOPHOT. Secondary surveys in other ISO bands were undertaken by the ELAIS team within the fields of the primary survey, with 6deg[SUP]2[/SUP] being covered at 6.7μm and 1deg[SUP]2[/SUP] at 175μm. This paper discusses the goals of the project and the techniques employed in its construction, as well as presenting details of the observations carried out, the data from which are now in the public domain. We outline the ELAIS `preliminary analysis' which led to the detection of over 1000 sources from the 15 and 90-μm surveys (the majority selected at 15μm with a flux limit of ~3mJy), to be fed into a ground-based follow-up campaign, as well as a programme of photometric observations of detected sources using both ISOCAM and ISOPHOT. We detail how the ELAIS survey complements other ISO surveys in terms of depth and areal coverage, and show that the extensive multi-wavelength coverage of the ELAIS fields resulting from our concerted and on-going follow-up programme has made these regions amongst the best studied areas of their size in the entire sky, and, therefore, natural targets for future surveys. This paper accompanies the release of extremely reliable subsets of the `preliminary analysis' products. Subsequent papers in this series will give further details of our data reduction techniques, reliability and completeness estimates and present the 15- and 90-μm number counts from the `preliminary analysis', while a further series of papers will discuss in detail the results from the ELAIS `final analysis', as well as from the follow-up programme. [less ▲]

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See detailThe European Large Area ISO Survey - IV. The preliminary 90-microns luminosity function
Serjeant, S.; Efstathiou, A.; Oliver, S. et al

in Monthly Notices of the Royal Astronomical Society (2001), 322

We present the luminosity function of 90-μm-selected galaxies from the European Large Area ISO Survey (ELAIS), extending to z=0.3. Their luminosities are in the range 10[SUP]9[/SUP]< h 65 -2L/L[SUB]solar ... [more ▼]

We present the luminosity function of 90-μm-selected galaxies from the European Large Area ISO Survey (ELAIS), extending to z=0.3. Their luminosities are in the range 10[SUP]9[/SUP]< h 65 -2L/L[SUB]solar[/SUB]<10[SUP]12[/SUP], i.e. non-ultraluminous. From our sample of 37 reliably detected galaxies in the ELAIS S1 region from the Efstathiou et al. S[SUB]90[/SUB]>=100mJy data base, we have found optical, 15-μm or 1.4-GHz identifications for 24 (65 per cent). We have obtained 2dF and UK Schmidt FLAIR spectroscopy of 89 per cent of identifications to rigid multivariate flux limits. We construct a luminosity function assuming that (i) our spectroscopic subset is an unbiased sparse sample, and (ii) there are no galaxies that would not be represented in our spectroscopic sample at any redshift. We argue that we can be confident of both assumptions. We find that the luminosity function is well described by the local 100-μm luminosity function of Rowan-Robinson, Helou & Walker. Assuming this local normalization, we derive luminosity evolution of (1+z)[SUP]2.45+/-0.85[/SUP] (95 per cent confidence). We argue that star formation dominates the bolometric luminosities of these galaxies, and we derive comoving star formation rates in broad agreement with the Flores et al. and Rowan-Robinson et al. mid-infrared-based estimates. [less ▲]

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See detailThe European Large Area ISO Survey - VI. Discovery of a new hyperluminous infrared galaxy
Morel, Thierry ULg; Efstathiou, A.; Serjeant, S. et al

in Monthly Notices of the Royal Astronomical Society (2001), 327

We report the discovery of the first hyperluminous infrared galaxy (HyLIG) in the course of the European Large Area ISO Survey (ELAIS). This object has been detected by ISO at 6.7, 15 and 90μm, and is ... [more ▼]

We report the discovery of the first hyperluminous infrared galaxy (HyLIG) in the course of the European Large Area ISO Survey (ELAIS). This object has been detected by ISO at 6.7, 15 and 90μm, and is found to be a broad-line, radio-quiet quasar at a redshift [formmu4]z=1.099. From a detailed multicomponent model fit of the spectral energy distribution, we derive a total IR luminosity L[SUB]IR[/SUB] [formmu5](1-1000μm)~1.0à 10[SUP]13[/SUP]h65-2L[SUB]solar[/SUB] [formmu6](q[SUB]0[/SUB]=0.5), and discuss the possible existence of a starburst contributing to the far-IR output. Observations to date present no evidence for lens magnification. This galaxy is one of the very few HyLIGs with a X-ray detection. On the basis of its soft X-ray properties, we suggest that this broad-line object may be the face-on analogue of narrow-line, Seyfert-like HyLIGs. [less ▲]

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See detailThe European Large Area ISO Survey - VIII. 90-microns final analysis and source counts
Heraudeau, P.; Oliver, S.; del Burgo, C. et al

in Monthly Notices of the Royal Astronomical Society (2004), 354

We present a re-analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 90-μm observations carried out with ISOPHOT, an instrument on board the ISO of the European Space ... [more ▼]

We present a re-analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 90-μm observations carried out with ISOPHOT, an instrument on board the ISO of the European Space Agency. With more than 12 deg[SUP]2[/SUP], the ELAIS survey is the largest area covered by ISO in a single programme and is about one order of magnitude deeper than the IRAS 100-μm survey. The data analysis is presented and was mainly performed with the PHOT interactive analysis software but using the pairwise method of Stickel et al. for signal processing from edited raw data to signal per chopper plateau. The ELAIS 90-μm catalogue contains 237 reliable sources with fluxes larger than 70 mJy and is available in the electronic version of this article. Number counts are presented and show an excess above the no-evolution model prediction. This confirms the strong evolution detected at shorter (15 μm) and longer (170 μm) wavelengths in other ISO surveys. The ELAIS counts are in agreement with previous works at 90 μm and in particular with the deeper counts extracted from the Lockman hole observations. Comparison with recent evolutionary models show that the models of Franceschini et al. and Guiderdoni et al. (which includes a heavily extinguished population of galaxies) give the best fit to the data. Deeper observations are nevertheless required to discriminate better between the model predictions in the far-infrared, and are scheduled with the Spitzer Space Telescope, which has already started operating, and will also be performed by ASTRO-F. [less ▲]

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See detailThe European Large-Area ISO Survey (ELAIS): the final band-merged catalogue
Rowan-Robinson, M.; Lari, C.; Perez-Fournon, I. et al

in Monthly Notices of the Royal Astronomical Society (2004), 351

We present the final band-merged European Large-Area ISO Survey (ELAIS) Catalogue at 6.7, 15, 90 and 175 μm, and the associated data at U, g', r', i', Z, J, H, K and 20 cm. The origin of the survey ... [more ▼]

We present the final band-merged European Large-Area ISO Survey (ELAIS) Catalogue at 6.7, 15, 90 and 175 μm, and the associated data at U, g', r', i', Z, J, H, K and 20 cm. The origin of the survey, infrared and radio observations, data-reduction and optical identifications are briefly reviewed, and a summary of the area covered and the completeness limit for each infrared band is given. A detailed discussion of the band-merging and optical association strategy is given. The total Catalogue consists of 3762 sources. 23 per cent of the 15-μm sources and 75 per cent of the 6.7-μm sources are stars. For extragalactic sources observed in three or more infrared bands, colour-colour diagrams are presented and discussed in terms of the contributing infrared populations. Spectral energy distributions (SEDs) are shown for selected sources and compared with cirrus, M82 and Arp220 starburst, and active galactic nuclei (AGN) dust torus models. Spectroscopic redshifts are tabulated, where available. For the N1 and N2 areas, the Isaac Newton Telescope ugriz Wide Field Survey permits photometric redshifts to be estimated for galaxies and quasars. These agree well with the spectroscopic redshifts, within the uncertainty of the photometric method [~10 per cent in (1 +z) for galaxies]. The redshift distribution is given for selected ELAIS bands and colour-redshift diagrams are discussed. There is a high proportion of ultraluminous infrared galaxies (log[SUB]10[/SUB] of 1-1000 μm luminosity L[SUB]ir[/SUB] > 12.22) in the ELAIS Catalogue (14 per cent of 15-μm galaxies with known z), many with Arp220-like SEDs. 10 per cent of the 15-μm sources are genuine optically blank fields to r'= 24: these must have very high infrared-to-optical ratios and probably have z > 0.6, so are high-luminosity dusty starbursts or Type 2 AGN. Nine hyperluminous infrared galaxies (L[SUB]ir[/SUB] > 13.22) and nine extremely red objects (EROs) (r-K > 6) are found in the survey. The latter are interpreted as ultraluminous dusty infrared galaxies at z~ 1. The large numbers of ultraluminous galaxies imply very strong evolution in the star formation rate between z= 0 and 1. There is also a surprisingly large population of luminous (L[SUB]ir[/SUB] > 11.5), cool (cirrus-type SEDs) galaxies, with L[SUB]ir[/SUB]-L[SUB]opt[/SUB] > 0, implying A[SUB]V[/SUB] > 1. [less ▲]

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