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See detailTRAPPIST photometry and imaging monitoring of comet C/2013 R1 (Lovejoy): Implications for the origin of daughter species
Opitom, Cyrielle ULg; Jehin, Emmanuel ULg; Manfroid, Jean ULg et al

in Astronomy and Astrophysics (2015), 584

We report the results of the narrow-band photometry and imaging monitoring of comet C/2013 R1 (Lovejoy) with the robotic telescope TRAPPIST (La Silla observatory). We gathered around 400 images over 8 ... [more ▼]

We report the results of the narrow-band photometry and imaging monitoring of comet C/2013 R1 (Lovejoy) with the robotic telescope TRAPPIST (La Silla observatory). We gathered around 400 images over 8 months pre- and post-perihelion between September 12, 2013 and July 6, 2014. We followed the evolution of the OH, NH, CN, C[SUB]3[/SUB], and C[SUB]2[/SUB] production rates computed with the Haser model, as well as the evolution of the dust production. All five gas species display an asymmetry about perihelion, since the rate of brightening is steeper than the rate of fading. The study of the coma morphology reveals gas and dust jets that indicate one or several active zone(s) on the nucleus. The dust, C[SUB]2[/SUB], and C[SUB]3[/SUB] morphologies present some similarities, while the CN morphology is different. OH and NH are enhanced in the tail direction. The study of the evolution of the comet activity shows that the OH, NH, and C[SUB]2[/SUB] production rate evolution with the heliocentric distance is correlated to the dust evolution. The CN and, to a lesser extent, the C[SUB]3[/SUB] do not display such a correlation with the dust. This evidence and the comparison with parent species production rates indicate that C[SUB]2[/SUB] and C[SUB]3[/SUB], on one hand, and OH and NH, on the other, could be - at least partially - released from organic - rich grains and icy grains. On the contrary, all evidences point to HCN being the main parent of CN in this comet. [less ▲]

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See detailKroniek van het Nederlandse nationaliteitsrecht 2014-2015
Vonk, Olivier ULg

in Asiel- en Migrantenrecht (2015)

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See detailProtein structure modeling using backbone chemical shifts
Wanko Nembot, Alexis Marius ULg; Damblon, Christian ULg

Poster (2015, December 01)

The knowledge of the tridimensional structure of a protein is essential to study its interactions and understand its mode of action. The Purpose of our work is to quickly and easily determine the ... [more ▼]

The knowledge of the tridimensional structure of a protein is essential to study its interactions and understand its mode of action. The Purpose of our work is to quickly and easily determine the structure of proteins using the backbone chemical shifts. Backbone chemical shifts data are NMR parameters that can be rapidly, easily and accurately measured. This parameter is very sensitive to the conformation of amino acids and is used to deduct the secondary structure (TALOS, RCI,...). We therefore plan to use backbone chemical shifts as constraints on dihedral angles to quickly and easily determine protein structure. Several « de novo » methods like CS-Rosetta , CS23D et CHESHIRE have been recently developed in this purpose. We will use proteins of different sizes for which, the structure (X-ray or NMR structure) and chemical shifts backbone are available for testing the three softwares. Knowing that each of these softwares predicted a large number of low energy models on the one hand, and that the deployment and use of these tools constitutes obstacles for users who are not experts in computer science on the other hand, our goal will be to develop a platform that can easily compare these three methods based on quality of the structure produced. [less ▲]

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See detailAsteroseismic hare & hound exercises: the case of β Cephei stars
Salmon, Sébastien ULg; Montalbán, J.; Miglio, A. et al

in Martins, F.; Boissier, S.; Buat, V. (Eds.) et al SF2A-2015: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: F. Martins, S. Boissier, V. Buat, L. Cambrésy, P. Petit, pp.423-428 (2015, December 01)

The β Cephei pulsating stars present a unique opportunity to test and probe our knowledge of the interior of massive stars. The information that we can get depends on the quality and number of ... [more ▼]

The β Cephei pulsating stars present a unique opportunity to test and probe our knowledge of the interior of massive stars. The information that we can get depends on the quality and number of observational constraints, both seismic and classical ones. The asteroseismology of β Cephei stars proceeds by a forward approach, which can result in multiple solutions, without clear indication on the level of confidence. We seek a method to derive confidence intervals on stellar parameters and investigate how these latter behave depending on the seismic data accessible to the observer. We realise forward modelling with the help of a grid of pre-computed models. We also use Monte-Carlo simulations to build confidence intervals on the inferred stellar parameters. We apply and test this method in a series of hare and hound exercises on a subset of theoretical models simulating observed stars. Results show that a set of 5 frequencies (with knowledge of their associated angular degree) yields precise seismic constraints. Significant errors on the determination of the extent of the central mixed region may result when the theoretical models do not present the same chemical mixture as the observed star. [less ▲]

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See detailUnderstanding Marc Atkins
Delville, Michel ULg; Mengham, Rod; Salmon, Yvonne et al

Scientific conference (2015, December 01)

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See detailThe Mars discrete aurora: morphology, altitude and role of crustal magnetic field
Gérard, Jean-Claude ULg

Scientific conference (2015, December 01)

We present results obtained during 2015 in the framework of BELSPO's SCOOP/BRAIN project. They concern the morphology, frequency, structure of the Mars discrete aurora and the influence of the residual ... [more ▼]

We present results obtained during 2015 in the framework of BELSPO's SCOOP/BRAIN project. They concern the morphology, frequency, structure of the Mars discrete aurora and the influence of the residual crustal magnetic field. [less ▲]

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See detailA cross-sectional study to evaluate factors related to condom use with commercial sexual partners in workers from Ecuadorian companies
Cabezas, Maria C.; Fornasini, Marco; Dardenne, Nadia ULg et al

in BMC Public Health (2015), 15(1),

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See detailThe HARPS-N Rocky Planet Search. I. HD 219134 b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun
Motalebi, F.; Udry, S.; Gillon, Michaël ULg et al

in Astronomy and Astrophysics (2015), 584

We know now from radial velocity surveys and transit space missions that planets only a few times more massive than our Earth are frequent around solar-type stars. Fundamental questions about their ... [more ▼]

We know now from radial velocity surveys and transit space missions that planets only a few times more massive than our Earth are frequent around solar-type stars. Fundamental questions about their formation history, physical properties, internal structure, and atmosphere composition are, however, still to be solved. We present here the detection of a system of four low-mass planets around the bright (V = 5.5) and close-by (6.5 pc) star HD 219134. This is the first result of the Rocky Planet Search programme with HARPS-N on the Telescopio Nazionale Galileo in La Palma. The inner planet orbits the star in 3.0935 ± 0.0003 days, on a quasi-circular orbit with a semi-major axis of 0.0382 ± 0.0003 AU. Spitzer observations allowed us to detect the transit of the planet in front of the star making HD 219134 b the nearest known transiting planet to date. From the amplitude of the radial velocity variation (2.25 ± 0.22 ms[SUP]-1[/SUP]) and observed depth of the transit (359 ± 38 ppm), the planet mass and radius are estimated to be 4.36 ± 0.44 M[SUB]⊕[/SUB] and 1.606 ± 0.086 R[SUB]⊕[/SUB], leading to a mean density of 5.76 ± 1.09 g cm[SUP]-3[/SUP], suggesting a rocky composition. One additional planet with minimum-mass of 2.78 ± 0.65 M[SUB]⊕[/SUB] moves on a close-in, quasi-circular orbit with a period of 6.767 ± 0.004 days. The third planet in the system has a period of 46.66 ± 0.08 days and a minimum-mass of 8.94 ± 1.13 M[SUB]⊕[/SUB], at 0.233 ± 0.002 AU from the star. Its eccentricity is 0.46 ± 0.11. The period of this planet is close to the rotational period of the star estimated from variations of activity indicators (42.3 ± 0.1 days). The planetary origin of the signal is, however, thepreferred solution as no indication of variation at the corresponding frequency is observed for activity-sensitive parameters. Finally, a fourth additional longer-period planet of mass of 71 M[SUB]⊕[/SUB] orbits the star in 1842 days, on an eccentric orbit (e = 0.34 ± 0.17) at a distance of 2.56 AU. The photometric time series and radial velocities used in this work are available in electronic form at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">http://cdsarc.u-strasbg.fr</A> (ftp://130.79.128.5) or via <A href="http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/584/A72">http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/584/A72</A> [less ▲]

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See detailLarger and faster: revised properties and a shorter orbital period for the WASP-57 planetary system from a pro-am collaboration
Southworth, John; Mancini, L.; Tregloan-Reed, J. et al

in Monthly Notices of the Royal Astronomical Society (2015), 454

Transits in the WASP-57 planetary system have been found to occur half an hour earlier than expected. We present 10 transit light curves from amateur telescopes, on which this discovery was based, 13 ... [more ▼]

Transits in the WASP-57 planetary system have been found to occur half an hour earlier than expected. We present 10 transit light curves from amateur telescopes, on which this discovery was based, 13 transit light curves from professional facilities which confirm and refine this finding, and high-resolution imaging which show no evidence for nearby companions. We use these data to determine a new and precise orbital ephemeris, and measure the physical properties of the system. Our revised orbital period is 4.5 s shorter than found from the discovery data alone, which explains the early occurrence of the transits. We also find both the star and planet to be larger and less massive than previously thought. The measured mass and radius of the planet are now consistent with theoretical models of gas giants containing no heavy-element core, as expected for the subsolar metallicity of the host star. Two transits were observed simultaneously in four passbands. We use the resulting light curves to measure the planet's radius as a function of wavelength, finding that our data are sufficient in principle but not in practise to constrain its atmospheric properties. We conclude with a discussion of the current and future status of transmission photometry studies for probing the atmospheres of gas-giant transiting planets. [less ▲]

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See detailPolarization microlensing in the quadruply imaged broad absorption line quasar H1413+117
Hutsemekers, Damien ULg; Sluse, Dominique ULg; Braibant, Lorraine ULg et al

in Astronomy and Astrophysics (2015), 584

We have obtained spectropolarimetric observations of the four images of the gravitationally lensed broad absorption line quasar H1413+117. The polarization of the microlensed image D is significantly ... [more ▼]

We have obtained spectropolarimetric observations of the four images of the gravitationally lensed broad absorption line quasar H1413+117. The polarization of the microlensed image D is significantly different, both in the continuum and in the broad lines, from the polarization of image A, which is essentially unaffected by microlensing. The observations suggest that the continuum is scattered off two regions, spatially separated, and producing roughly perpendicular polarizations. These results are compatible with a model in which the microlensed polarized continuum comes from a compact region located in the equatorial plane close to the accretion disk and the non-microlensed continuum from an extended region located along the polar axis. Based on observations made with ESO Telescopes at the Paranal Observatory (Chile). ESO program ID: 386.B-0337. [less ▲]

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See detailDrug-polymer electrostatic complexes as new structuring agents for the formation of drug-loaded ordered mesoporous silica
Molina, Emilie; Warnant, Jérôme; Mathonnat, Mélody et al

in Langmuir (2015), 31(47), 12839-12844

Using aminoglycoside antibiotics as drug models, it was shown that electrostatic complexes between hydrophilic drugs and oppositely charged double-hydrophilic block copolymers can form ordered mesophases ... [more ▼]

Using aminoglycoside antibiotics as drug models, it was shown that electrostatic complexes between hydrophilic drugs and oppositely charged double-hydrophilic block copolymers can form ordered mesophases. This phase behaviour was evidenced by using poly(acrylic acid)-block-poly(ethylene oxide) block copolymers in the presence of silica precursors and, this allowed preparing drug-loaded mesoporous silica directly from the drug-polymer complexes. The novel synthetic strategy of the hybrid materials is highly efficient, avoiding waste and multi-step processes; it also ensures optimal drug loading and provides pH-dependence of the drug release from the materials. [less ▲]

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See detailDevelopment and validation of a short Italian UPPS-P Impulsive Behavior Scale
D'Orta, Isabella; Burnay, Jonathan ULg; Aiello, Daniela et al

in Addictive Behaviors Reports (2015), 2

Impulsivity is a multidimensional construct that plays a prominent role in the development, maintenance, and relapse of addictive disorders. The UPPS-P model of impulsivity, which distinguishes between ... [more ▼]

Impulsivity is a multidimensional construct that plays a prominent role in the development, maintenance, and relapse of addictive disorders. The UPPS-P model of impulsivity, which distinguishes between five impulsivity components (positive urgency, negative urgency, lack of perseverance, lack of premeditation, sensation seeking), has been increasingly investigated during the last decade in relation to addictive and risky behaviors. Unfortunately, it currently lacks a validated scale that allows Italian researchers and clinicians to measure impulsivity based on the UPPS-P model. The current study fills this gap by testing the psychometric properties of a short 20-item Italian scale used to assess the five dimensions of the UPPS-P model in 188 volunteer participants from the community. Confirmatory factor analysis supported a model of five distinct, but interrelated, impulsivity components. The results indicated good internal consistency (Cronbach's α ranges from .73 to .84). Construct validity was evidenced by specific relations with measures of addictive behaviors and depressive symptoms. On the whole, this study demonstrated that the Italian short UPPS-P has good psychometric properties. [less ▲]

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See detailUpdated checklist of the mosquitoes (Diptera: Culicidae) of Belgium
Boukraa, Slimane ULg; Dekoninck, Wouter; Versteirt, Veerle et al

in Journal of Vector Ecology : Journal of the Society for Vector Ecology (2015), 40(2), 398-407

Most information about the systematics and bioecology of Belgian mosquitoes dates back from before 1950, and only scattered information was produced during the last decades. In this paper we review and ... [more ▼]

Most information about the systematics and bioecology of Belgian mosquitoes dates back from before 1950, and only scattered information was produced during the last decades. In this paper we review and update the list of mosquito species recorded in Belgium, from first report (1908) to 2015. Six genera and 31 species were recorded so far, including 28 autochthonous species and three invasive alien species recently recorded in Belgium: Aedes albopictus (Skuse 1894), Ae. japonicus japonicus (Theobald 1901), and Ae. koreicus (Edwards 1917). The six genera are Anopheles (five species), Aedes (sixteen species), Coquillettidia (one species), Culex (four species), Culiseta (four species), and Orthopodomyia (one species). [less ▲]

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See detailAgriculture et environnement : genèse des relations
Habran, Maxime ULg

in Revue de l'Union européenne (2015), (593), 604-617

Les négociations portant sur la réforme de la politique agricole commune (PAC) auraient dû mettre la politique de protection de l’environnement sur le devant de la scène. Au lieu de cela, la PAC s’est vu ... [more ▼]

Les négociations portant sur la réforme de la politique agricole commune (PAC) auraient dû mettre la politique de protection de l’environnement sur le devant de la scène. Au lieu de cela, la PAC s’est vu doter d’un nouveau mécanisme appelé verdissement ou paiement vert destiné à verdir le pilier des soutiens de marché. Ce mécanisme rend opaque la prise en compte de l’environnement et affaiblit la conditionnalité. D’un greening, les négociateurs se sont mis d’accord sur un greenwashing. L’objectif de cette contribution est de montrer la manière dont est intégrée la politique de protection de l’environnement au sein de la politique agricole commune. La notion de conditionnalité environnementale permet de comprendre l’articulation et l’interaction entre ces deux politiques. [less ▲]

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See detailRevue épidémiologique des tendinopathies les plus fréquentes
Sancerne, Audrey; Kaux, Jean-François ULg

in Journal de Traumatologie du Sport (2015), 32(4), 223-228

Tendinopathies are overused pathologies essentially present among sportsmen as well as workers. They represent 19 % of musculo-skeletaldisorders, more than 30 % the consultations of general and sports ... [more ▼]

Tendinopathies are overused pathologies essentially present among sportsmen as well as workers. They represent 19 % of musculo-skeletaldisorders, more than 30 % the consultations of general and sports medicine on musculoskeletal system. At present, general epidemiology studiesare few. Data will therefore be included for each tendinopathy: rotator cuff tendinopathies, epicondylitis, trochanteric pain syndrome, patellar andcalcaneal tendinopathies and plantar fasciitis. The articles have been searched on the databases PubMed and Pedro. [less ▲]

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See detailQuantum manifestations of classical nonlinear resonances
Wisniacki, Diego A.; Schlagheck, Peter ULg

in Physical Review. E : Statistical, Nonlinear, and Soft Matter Physics (2015), 92

When an integrable classical system is perturbed, nonlinear resonances are born, grow, and eventually disappear due to chaos. In this paper the quantum manifestations of such a transition are studied in ... [more ▼]

When an integrable classical system is perturbed, nonlinear resonances are born, grow, and eventually disappear due to chaos. In this paper the quantum manifestations of such a transition are studied in the standard map. We show that nonlinear resonances act as a perturbation that break eigenphase degeneracies for unperturbed states with quantum numbers that differ in a multiple of the order of the resonance. We show that the eigenphase splittings are well described by a semiclassical expression based on an integrable approximation of the Hamiltonian in the vicinity of the resonance. The morphology in phase space of these states is also studied. We show that the nonlinear resonance imprints a systematic influence in their localization properties [less ▲]

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See detailPressure-impulse diagram of a beam developing non-linear membrane action under blast loading
Hamra, Lotfi ULg; Demonceau, Jean-François ULg; Denoël, Vincent ULg

in International Journal of Impact Engineering (2015), 86

The p–I diagram of a frame beam subjected to blast loading is established, including the elastic lateral restraint and inertia offered by the rest of the structure, the development of nonlinear membrane ... [more ▼]

The p–I diagram of a frame beam subjected to blast loading is established, including the elastic lateral restraint and inertia offered by the rest of the structure, the development of nonlinear membrane action and also, the bending-tension (M−N) interaction that develops in the plastic hinges. The analytical procedures to compute the asymptotes in the p–I diagram as well as a parametric study on the p–I diagram are provided. A dimensional analysis of the problem reveals that, under the considered assumptions, four dimensionless parameters mainly influence the required ductility of the beam. Two of them are related to the behavior of the indirectly affected part (the lateral restraint and mass). Another one is related to the mechanical properties of the investigated beam (i.e. the ratio of the bending to axial resistance). The last parameter incorporates scales of the geometry and of the deformed configuration at the onset of the plastic mechanism. [less ▲]

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See detailValorisation des produits laitiers dans les ménages peuls du Nord-Est du Bénin
Chabi Toko, Roukayath ULg; Adégbidi, Anselme; Lebailly, Philippe ULg

in International Journal of Biological and Chemical Sciences (2015)

La population pastorale et agro-pastorale du Bénin détient presque la totalité du cheptel bovin national. Le lait constitue le produit le plus fréquent issu de l'élevage bovin. Une enquête a été menée ... [more ▼]

La population pastorale et agro-pastorale du Bénin détient presque la totalité du cheptel bovin national. Le lait constitue le produit le plus fréquent issu de l'élevage bovin. Une enquête a été menée dans la commune de Kalalé au sein de 16 ménages peuls afin de comprendre l'organisation de ces ménages dans la gestion du lait. Il ressort que l'organisation autour du capital lait est genre sensible: l'homme aussi bien que la femme, dans leurs rôles respectifs, contribuent à assurer la pérennité du capital bétail. Le lait est géré de façon à privilégier la consommation du ménage et à assurer la reproduction du troupeau. La rémunération du travail fournit ainsi que l'équité dans la distribution des richesses au sein du ménage peul octroi aux femmes qui sont dans le troupeau plus de bénéfices issues du lait provenant du troupeau familial. La disponibilité des produits laitiers dépend de la saison et du milieu. Le lait prévu pour la consommation humaine est gérée de sorte à avoir, une utilisation optimale du lait et de la viande, afin de combler les besoins actuels des membres du ménage, d'assurer la reproduction des biens du ménage ; avant d'alimenter le marché de produits laitiers. [less ▲]

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See detailQualité de vie du patient sarcopénique : apport de l’étude liégeoise SarcoPhAge
Beaudart, Charlotte ULg; Reginster, Jean-Yves ULg; PETERMANS, Jean ULg et al

in Gériatrie et Psychologie Neuropsychiatrie du Vieillissement (2015), 13(4), 391-5

The consequences of sarcopenia on quality are difficult to evaluate and consequently are quite poorly studied. The few studies assessing the quality of life in sarcopenic subjects currently use generic ... [more ▼]

The consequences of sarcopenia on quality are difficult to evaluate and consequently are quite poorly studied. The few studies assessing the quality of life in sarcopenic subjects currently use generic quality of life questionnaires such as SF36 and EQ5D. The SarcoPhAge study, conducted on a cohort developed in Liège including 534 subjects of 65 years or older, suggested that sarcopenic subjects present a significant worse quality of life in the domains of physical function compared to nonsarcopenic subjects. Generic tools do not cover exhaustively all the areas of potential dysfunction concerned in this geriatric syndrome. Yet, there is no specific and validated quality of life questionnaire for sarcopenia. It would be useful to have at our disposal a sarcopenia specific quality of life questionnaire to assess not only the prospective quality of life of sarcopenic subjects but also to assess the efficacy and the rele [less ▲]

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See detailÉditorial=Woord vooraf
Decoster, Sara ULg

in Cahiers de la Documentation = Bladen voor Documentatie (2015), 69(4),

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