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Institut d'Astrophysique et
de Géophysique (Bât. B5c)

Quartier Agora
Allée du 6 août, 19C
B-4000 Liège 1 (Sart-Tilman)

Tel.: 04.366.9774
Fax: 04.366.9729
Recul rapide Année précédente Séminaires : Archives 2018    
Jan Fév Mar Avr Mai Jun Jul Aoû Sep Oct Nov Déc
Mois précédent Mois suivant Février 2018
Séminaire suivant  1er séminaire : mercredi 21 février, 11h00
Cosmology with quasar time delays: a short history of Refsdal’s idea and of its implementation
Frédéric Courbin (EPFL Lausanne)

Time delays in gravitationally lensed quasars in principle allow to measure H0 independently of other cosmological parameters. I will review the field of quasar time delays from the very first measurements to the most recent ones and will show what are the main advantages and drawbacks of the method over others. Future prospects are given, especially in the context of Euclid, LSST, and monitoring with dedicated telescopes.
Séminaire précédant Séminaire suivant 2ème séminaire : lundi 26 février, 15h45
The curious case of scalar dark matter from exotic CP symmetry
Igor Ivanov (IST, Lisbon)
Séminaire précédant Séminaire suivant 3ème séminaire : mardi 27 février, 14h00
On critical thinking and cognitive pitfalls
Johan Braeckman (UGent)

In this lecture we investigate why people are so vulnerable to mental infections with totally irrational believes. Insights developed in social psychology, informal logic or neuroscience, make clear how quick human reasoning can go wrong, how easy one makes wrong connections, wrong statistical estimations and all to quick generalizations. Scientists doing research are often better armed against the danger of infection by irrational and pseudoscientific views. However, they are very good in rationalizing wrong views, picked up along the way, which often makes them stick to bad ideas much longer. Nobody is immune! Pseudoscientific theories will be discussed together with historical and current examples of apparent scientific and objective views that turned out to be infected by fallacies or wrong assumptions. The differences between science and pseudoscience and between rational and irrational thinking will be clarified. A pure rational way of thinking is most probably never to be reached, and may even be something we should not wish for, but we can get a better insight in how our brain processes information and creates false realities.
Mois précédent Mois suivant Mars 2018
Séminaire précédant Séminaire suivant 4ème séminaire : mercredi 14 mars, 15h45
Extrasolar planets meet star spots
Jürgen Schmitt (Universität Hamburg)

Transits of extrasolar planets offer not only the possibility to study the physical properties of planets, they also provide a new possibility to diagnose the surfaces of active stars, which allows the study of surface inhomogeneities with unprecedented angular resolution. I will discuss the modeling of extrasolar planet transit light curves, and in particular, how the analysis is affected by star spots and how the derived extrasolar planet parameters depend on the activity state of the spots. I will specifically discuss how the transit light curves change due to the presence of star spots and how this information can be used to construct surface maps of active stars and deduce stellar properties. I will discuss the potential of transit studies at shorter wavelengths and show how high-energy observations constrain the physical properties of extrasolar planets.
Séminaire précédant Séminaire suivant 5ème séminaire : vendredi 16 mars, 10h00
Digital Holographic Microscopy
Kent Wallace (Jet Propulsion Laboratory)
Séminaire précédant Séminaire suivant 6ème séminaire : jeudi 29 mars, 15h45
DOTIFS - a multi-deployable fiber-fed IFU Spectrograph
Sabyasachi Chattopadhyay (STAR)

Devasthal Optical Telescope Integral Field Spectrograph (DOTIFS) is a new multi-object integral field spectrograph being built by the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, India for the 3.6m Devasthal Optical Telescope, (DOT). The Devasthal Observatory has been constructed by the Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital. DOTIFS is mainly designed to study the physics and kinematics of ionized gas, star formation, and H II regions in the nearby galaxies. DOTIFS is a novel instrument in terms of multi-IFUs, built in deployment system, and high throughput. A magnifier at the Cassegrain side port of the telescope feeds sixteen integral field units (IFUs). The IFUs can be deployed over an 8’ diameter focal plane by orthogonal actuators. An intelligent deployment algorithm has been developed to allow optimized reconfiguration and to avoid any collision between IFUs. The whole deployment system has a complex 3-dimensional structure to allow maximum positioning freedom to the IFUs. The IFUs are developed using the novel technique of photolithography which makes the instrument precise but cost-effective. Digital correlated double sampling is implemented as the detector readout to minimize the readout noise with a thorough analytical understanding of the noise components. The speaker will provide details of the instruments and the challenges. The instrument is in the phase of fabrication and is scheduled to be commissioned in late 2018.
Mois précédent Mois suivant Mai 2018
Séminaire précédant Séminaire suivant 7ème séminaire : jeudi 03 mai, 15h45
On the determination of stellar ages, masses and radii from theoretical models
Andrea Bonfanti (STAR)

Determining the ages of stars is a very challenging task. Several indicators are available, but no single method works well for a broad range of spectral type or for each evolutionary phase of a star. My PhD project was related to the building of an algorithm for the determination of stellar ages, considering evolutionary tracks and isochrones. This model-dependent approach, which has been complemented by using gyrochronology, stellar magnetic activity and scaling relations coming from asteroseismology, also enables to retrieve other useful stellar parameters such as radius or mass. Here I will briefly discuss the problems of inferring ages from theoretical models and the characterization of solar-type stars of the solar neighbourhood, with a specific attention to the realistic uncertainties to be attributed to the main stellar parameters as a sum of internal and model-related ones. Moreover, considering that the determination of exoplanet properties requires the knowledge of stellar parameters, I will also show you the synergy between the characterization of stars and the exoplanetary science with particular references to the future Cheops mission and the analysis of stellar light curves.
Séminaire précédant Séminaire suivant 8ème séminaire : jeudi 24 mai, 16h00
L’océanographie opérationnelle au service de la conservation des tortues marines
Philippe GASPAR (CLS - Toulouse)

Toutes les espèces de tortues marines sont soumises à d’importantes pressions anthropiques qu’elles soient directes (braconnage des nids, pêche) ou indirectes (pollution marine, réchauffement climatique).

Après avoir rapidement passé en revue ces diverses pressions, nous nous focaliserons sur celles qui affectent les juvéniles en mer. Ce stade de vie, mal observé et donc mal connu, est pourtant crucial. En effet, l’évolution (expansion ou extinction) des populations de tortues marines dépend fortement de la mortalité juvénile. C’est pour étudier ce stade de vie critique que nous avons développé STAMM (Sea Turtle Active Movement Model), un modèle individu-centré qui permet de simuler la dispersion des tortues juvéniles en mer ainsi que les conditions de vie qu’elles y rencontrent. Dans ce modèle, les individus simulés se dispersent sous l’impact combiné de la dérive induite par les courants marins et des mouvements de nage motivés par la recherche d’habitats favorables. Ces habitats sont caractérisés par des eaux suffisamment chaudes et riches en nourriture.

Nous présenterons ici les premières simulations réalisées avec le modèle STAMM forcé par des champs de courant et de température issus d’une réanalyse longue de la circulation océanique fournie par MERCATOR, le centre européen d’océanographie opérationnelle. Ces simulations concernent les populations de tortues luth de l’Atlantique Nord-Ouest et du Pacifique Ouest.

L’analyse des résultats montrent que :

- les schémas de dispersion spatiale simulés par STAMM sont cohérents avec les rares observations disponibles ; - la variabilité de la circulation, de la température, et la productivité océanique modulent de façon très importante la mortalité naturelle ; - les mouvements de nage orientés vers les zones productives tendent à concentrer les individus dans des zones exploitées de façon intensive par les pêcheries thonières.

La comparaison des simulations Atlantique et Pacifique fournit également des éléments susceptibles d’expliquer, au moins partiellement, pourquoi la population de tortues luth de l’Atlantique Nord-Ouest se développe alors que celle du Pacifique Ouest diminue de façon alarmante.
Mois précédent Mois suivant Juin 2018
Séminaire précédant 9ème séminaire : vendredi 22 juin, 11h00 
Artificial Neural Networks and Applications to Astronomy
Ranjan Gupta (IUCAA, Pune, Inde)

Artificial Neural Networks (ANN) have been known as a powerful tool for pattern recognition in various applications over past several years since the multi-layer-back-propagation algorithm (MBPN) was developed. In the recent years, ANN have been successfully used in classification type applications in Astronomy. The talk would highlight ANN as a tool for pattern recognition in general and Astronomical applications in particular. It would also review the stellar spectral classification trends and new applications carried out by our group recently viz. extracting stellar atmospheric parameters from observed stellar spectra, determination of color excess from IUE-UV spectra and use of PCA as a pre-processor for ANN applications. Its application to a fairly large sample of 2000 spectra of IRAS and subsequent classification results will be shown. Recent applications of ANNs by our group are on the large 1273 spectra of CFLIB INDO-US spectral library and estimation of interstellar extinction from UV simulated satellite data etc. and star-galaxy classification for upcoming satellite missions TAUVEX/ASTROSAT/GAIA etc. It has been most recently applied to a very large spectral data base of LAMOST.
Université de Liège > Faculté des Sciences > Département d'Astrophysique, Géophysique et Océanographie : CoWebAGO, Juin 2009.