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See detailDécrets Présidentiels portant création du PNPS et nomination de son Directeur
Manzambi Kuwekita, Joseph ULiege

Scientific conference (2017, May 09)

Social Protection refers to all mechanisms of (i) prevention, (ii) protection and collective as well as (iii) promotion or social rehabilitation for individuals and households to support social risks ... [more ▼]

Social Protection refers to all mechanisms of (i) prevention, (ii) protection and collective as well as (iii) promotion or social rehabilitation for individuals and households to support social risks. Social Protection in the DRC is not a recent concern. Well before independence, a series of initiatives and devices had been implemented by the Belgian kingdom. Upon its accession to independence, the DRC became a member of the ILO. More than 80% of the population of the DRC has no social protection coverage. To remedy this, the Congolese Government has implemented the PNPS (National program of support to Social Protection (PNPS) in November 2005, with 5 missions: (i) extend the coverage of social protection, (ii) improve the quality of social services, (iii) establish and maintain a system of coverage of health care, (iv) contribute to the work of reform with the appointed commission, (v) make effective social protection for all. The formulation of the National Social Protection policy is one of the assignments entrusted to the Council of the PNPS, which the Minister of social security is the President. The Secretariat of the Council of the PNPS is managed by its Director. The two presidential decrees here presented deal about (i) the creation of the PNPS and (ii) the appointment of its Director, both signed in November 24, 2005. [less ▲]

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See detailDécrire et analyser un dispositif professionnalisant
Scheepers, Caroline ULiege

Scientific conference (2006, March)

La conférence s'adresse aux étudiants en économie de l'ULB qui préparent l'agrégation. Elle vise à leur communiquer les principaux résultats de la recherche DiPro, menée conjointement par l'ULg et l'UCL.

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See detailDécrire/Agir
Klinkenberg, Jean-Marie ULiege

in AAVV (Ed.) Séminaire international sur la méthodologie d’observation de la langue française dans le monde (2008)

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See detailDécrochage de la courbe de périmètre crânien et si l’origine n'était pas neurologique
LONGTON, Julie ULiege; DRESSE, Marie-Françoise ULiege; Hoyoux, Marie et al

in Tijdschrift van de Belgische Kinderarts = Journal du Pédiatre Belge (2015), 17(1), 46

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See detailLa décroissance : nécessité ou utopie ?
Artige, Lionel ULiege

Conference given outside the academic context (2012)

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See detailLe décumul intégral des revenus des conjoints
Romer, Adeline ULiege

Article for general public (2005)

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See detailLes dédicaces latines des motets et "Sacrae Cantiones" de René del Mel
Corswarem, Emilie ULiege

in Bossuyt, Ignace; Gabriëls, Nele; Sacré, Dirk (Eds.) et al Cui dono lepidum novum libellum ? Dedicating Latin Works and Motets in the Sixteenth Century Theory and Practice (2008)

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See detailA dedicated photometric system for the classification of Wolf-Rayet stars
Royer, P.; Vreux, Jean-Marie ULiege; Manfroid, Jean ULiege

in Astronomy and Astrophysics. Supplement Series (1998), 130

We present here tests of a five-filter photometric system aimed at WR classification. In addition to the well-known easy separation between the WN and WC spectral types, these tests indicate interesting ... [more ▼]

We present here tests of a five-filter photometric system aimed at WR classification. In addition to the well-known easy separation between the WN and WC spectral types, these tests indicate interesting potentialities in the discrimination of subgroups among the WN and the WC which look well related to the classical subtypes. The proposed combinations of filters (or derived ones) bear enough discriminating power to satisfy some evolutionary studies in crowded fields where spectroscopic follow-up is not possible. Based on observations collected at the European Southern Observatory, La Silla, Chile. [less ▲]

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See detailDedication - Michel Frankignoulle
Borges, Alberto ULiege; Delille, Bruno ULiege

in Journal of Marine Systems (2007), 66(1-4), 4-5

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See detailDéductions paléoclimatiques d'une comparaison entre les assemblages de miospores du Dévonien Moyen et Supérieur de Libye et du Brésil.
Loboziak, S; Streel, Maurice ULiege; Burjack, M.I.A.

in Geobios (1989), 22(2), 247-251

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See detailDeeds not declarations: Ukraine's convergence with the EU's foreign and security policies until 2010
Natorski, Michal ULiege

in Noutcheva, Gergana; Pomorksa, Karolina; Bosse, Giselle (Eds.) The EU and its neighbours. Values versus security in European foreign policy (2013)

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See detailDeel IV De belastingplichtige
Peeters, Bart ULiege

in Vandebergh, Henri (Ed.) BTW-Handboek (2014)

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See detailDeelrapport: Bevraging van de aanbodzijde In het kader van de DIVERSITEITSBAROMETER HUISVESTING
Verstrate, Jana; Perrin, Nathalie ULiege; De Decker, Pascal

in Centre Interfédéral pour l'Egalité des Chances (Ed.) Baromètre de la diversité - Logement (2014)

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See detailDeep asteroseismic sounding of the compact hot B subdwarf pulsator KIC02697388 from Kepler time series photometry
Charpinet, Stéphane; Van Grootel, Valérie ULiege; Fontaine, Gilles et al

in Astronomy and Astrophysics (2011), 530

Context. Contemporary high precision photometry from space provided by the Kepler and CoRoT satellites generates significant breakthroughs in terms of exploiting the long-period, g-mode pulsating hot B ... [more ▼]

Context. Contemporary high precision photometry from space provided by the Kepler and CoRoT satellites generates significant breakthroughs in terms of exploiting the long-period, g-mode pulsating hot B subdwarf (sdBVs) stars with asteroseismology. Aims: We present a detailed asteroseismic study of the sdBVs star KIC02697388 monitored with Kepler, using the rich pulsation spectrum uncovered during the ~27-day-long exploratory run Q2.3. Methods: We analyse new high-S/N spectroscopy of KIC02697388 using appropriate NLTE model atmospheres to provide accurate atmospheric parameters for this star. We also reanalyse the Kepler light curve using standard prewhitening techniques. On this basis, we apply a forward modelling technique using our latest generation of sdB models. The simultaneous match of the independent periods observed in KIC02697388 with those of models leads objectively to the identification of the pulsation modes and, more importantly, to the determination of some of the parameters of the star. Results: The light curve analysis reveals 43 independent frequencies that can be associated with oscillation modes. All the modulations observed in this star correspond to g-mode pulsations except one high-frequency signal, which is typical of a p-mode oscillation. Although the presence of this p-mode is surprising considering the atmospheric parameters that we derive for this cool sdB star (Teff = 25 395 ± 227 K, log g = 5.500 ± 0.031 (cgs), and log N(He) /N(H) = -2.767 ± 0.122), we show that this mode can be accounted for particularly well by our optimal seismic models, both in terms of frequency match and nonadiabatic properties. The seismic analysis leads us to identify two model solutions that can both account for the observed pulsation properties of KIC02697388. Despite this remaining ambiguity, several key parameters of the star can be derived with stringent constraints, such as its mass, its H-rich envelope mass, its radius, and its luminosity. We derive the properties of the core proposing that it is a relatively young sdB star that has burnt less than ~34% (in mass) of its central helium and has a relatively large mixed He/C/O core. This latter measurement is in line with the trend already uncovered for two other g-mode sdB pulsators analysed with asteroseismology and suggests that extra mixing is occurring quite early in the evolution of He cores on the horizontal branch. Conclusions: Additional monitoring with Kepler of this particularly interesting sdB star should reveal the inner properties of KIC02697388 and provide important information about the mode driving mechanism and the helium core properties. [less ▲]

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