The Evolution of the Baryonic Tully-Fisher Relation over the past 6 Gyr

Scaling relations are salient ingredients of galaxy evolution and formation models. I summarize results from the IMAGES survey, which combines spatially-resolved kinematics from FLAMES/GIRAFFE with imaging from HST/ACS and other facilities. Specifically, I will focus on the evolution of the stellar mass and baryonic Tully-Fisher Relations (TFR) from z=0.6 down to z=0. We found a significant evolution in zero point and scatter of the stellar mass TFR compared to the local Universe. Combined with gas fractions derived by inverting the Schmidt-Kennicutt relation, we derived for the first time a baryonic TFR at high redshift. Conversely to the stellar mass TFR, the baryonic relation does not appear to evolve in zero point, which suggests that most of the reservoir of gas converted into stars over the past 6 Gyr was already gravitationally bound to galaxies at z=0.6.Comment: To be published in the proceedings of the IAU Symposium 277 "Tracing the Ancestry of Galaxies"; 4 pages, 1 figur

Are Educated Societies Less Violent? Education, Deprivation and Crime in Minas Gerais

The intuition behind this paper is that education has a significant role to play in the reduction crime policies in developing countries. In other words, the fact that universal education is not completed in developing countries could be one of the reasons of their high crime rates. This paper brings an augmented economic model of individual crime behavior in order to take into account relative deprivation, discusses the impact of education in this model, distinguishing between property and interpersonal crime and furnishes an econometric estimation of the model for 723 municipalities of Minas Gerais, one of the 26 Brazilian states. Violent property crime seems to be influenced directly by inequality but not by education, which has however a significant reducing effect upon interpersonal violence.Brazil, education, deprivation, violence, crime

How Do Criminals Locate? Crime and Spatial Dependence in Minas Gerais

The aim of this paper is to investigate the existence of a spatial dependence of crime rates at a local level in the case of municipalities of Minas Gerais, one of the 26 Brazilian states. Results suggest the existence of a positive spatial autocorrelation of municipal violent crime rates. However, it also appears that violent crime against property and against persons do not follow the same spatial behavior. While violent economic crime seems to spread a lot, interpersonal violence is a much more localized phenomenon.violent crime, spatial autocorrelation, Brazil

Macro-Economic Instability and Crime

This paper adds to the literature on the economic determinants of crime by examining the impact of macro-economic instability. Instability increases the frustration level of individuals and incites them to smooth their income by using illegal earnings. Results from a panel of developed and developing countries for the period 1980-97 suggests that macro-economic instability had a significant impact on crime, both homicide and robbery. However, homicide and robbery do not react to instability in the same way.macro-economic instability, crime, institutions

The Physics and Mass Assembly of distant galaxies with the E-ELT

One of the main science goal of the future European Extremely Large Telescope will be to understand the mass assembly process in galaxies as a function of cosmic time. To this aim, a multi-object, AO-assisted integral field spectrograph will be required to map the physical and chemical properties of very distant galaxies. In this paper, we examine the ability of such an instrument to obtain spatially resolved spectroscopy of a large sample of massive (0.1<Mstellar<5e11Mo) galaxies at 2<z<6, selected from future large area optical-near IR surveys. We produced a set of about one thousand numerical simulations of 3D observations using reasonable assumptions about the site, telescope, and instrument, and about the physics of distant galaxies. These data-cubes were analysed as real data to produce realistic kinematic measurements of very distant galaxies. We then studied how sensible the scientific goals are to the observational (i.e., site-, telescope-, and instrument-related) and physical (i.e., galaxy-related) parameters. We specifically investigated the impact of AO performance on the science goal. We did not identify any breaking points with respect to the parameters (e.g., the telescope diameter), with the exception of the telescope thermal background, which strongly limits the performance in the highest (z>5) redshift bin. We find that a survey of Ngal galaxies that fulfil the range of science goals can be achieved with a ~90 nights program on the E-ELT, provided a multiplex capability M Ngal/8.Comment: 21 pages, 13 figures, 7 tables. Accepted for publication in MNRA

Coupling MOAO with Integral Field Spectroscopy: specifications for the VLT and the E-ELT

[Abridged] We have developed an end-to-end simulation to specify the science requirements of a MOAO-fed integral field spectrograph on either an 8m or 42m telescope. Our simulations re-scales observations of local galaxies or results from numerical simulations of disk or interacting galaxies. For the current analysis, we limit ourselves to a local disk galaxy which exhibits simple rotation and a simulation of a merger. We have attempted to generalize our results by introducing the simple concepts of "PSF contrast" which is the amount of light polluting adjacent spectra which we find drives the smallest EE at a given spatial scale. The choice of the spatial sampling is driven by the "scale-coupling", i.e., the relationship between the IFU pixel scale and the size of the features that need to be recovered by 3D spectroscopy in order to understand the nature of the galaxy and its substructure. Because the dynamical nature of galaxies are mostly reflected in their large-scale motions, a relatively coarse spatial resolution is enough to distinguish between a rotating disk and a major merger. Although we used a limited number of morpho-kinematic cases, our simulations suggest that, on a 42m telescope, the choice of an IFU pixel scale of 50-75 mas seems to be sufficient. Such a coarse sampling has the benefit of lowering the exposure time to reach a specific signal-to-noise as well as relaxing the performance of the MOAO system. On the other hand, recovering the full 2D-kinematics of z~4 galaxies requires high signal-to-noise and at least an EE of 34% in 150 mas (2 pixels of 75 mas). Finally, we carried out a similar study at z=1.6 with a MOAO-fed spectrograph for an 8m, and find that at least an EE of 30% at 0.25 arcsec spatial sampling is required to understand the nature of disks and mergers.Comment: 17 pages, 20 figures, accepted for publication in the MNRA

Enhanced blind decoding of Tardos codes with new map-based functions

This paper presents a new decoder for probabilistic binary traitor tracing codes under the marking assumption. It is based on a binary hypothesis testing rule which integrates a collusion channel relaxation so as to obtain numerical and simple accusation functions. This decoder is blind as no estimation of the collusion channel prior to the accusation is required. Experimentations show that using the proposed decoder gives better performance than the well-known symmetric version of the Tardos decoder for common attack channels

The formation of disks in massive spiral galaxies

The flatness of the rotation curve inside spiral galaxies is interpreted as the imprint of a halo of invisible matter. Using the deepest observations of distant galaxies, we have investigated how large disks could have been formed. Observations include spatially resolved kinematics, detailed morphologies and photometry from UV to mid-IR. Six Giga-years ago, half of the present-day spirals had anomalous kinematics and morphologies that considerably affect the scatter of the Tully Fisher relation. All anomalous galaxies can be modelled through gas-rich, major mergers that lead to a rebuilt of a new disk. The spiral-rebuilding scenario is proposed as a new channel to form large disks in present-day spirals and it accounts for all the observed evolutions since the last 6 Giga-years. A large fraction of the star formation is linked to merging events during their whole durations.Comment: AIP Proceedings of a review given at the "Invisible Universe International Conference" held in Paris, June 2009. 16 pages, 9 Figure

L’esprit de Saussure : réception et héritage (l’héritage linguistique saussurien : Paris contre Genève)

International audienceQue porte au fait et au juste avec lui le terme d’héritage ? En quoi concerne-t-il en effet de près la linguistique saussurienne ? Jusqu’à quel point ? Comment distribuer ici la série des sèmes plus ou moins virtuels et toujours très « lourds » qui lui sont associés : le legs, la dette, la légitimation par ascendance plus ou moins directe, mais aussi la limite, pourquoi pas le fardeau ou l’obstacle… ? D’autre part, le titre et le texte de présentation installent une opposition « Paris contre Genève » qui, modulée par une interrogation, est soumise à notre appréciation et à notre faculté de réagir à une petite provocation (imagine-t-on une guerre franco-suisse déclarée par Saussure ou à son sujet?) propre à faire tourner, en somme, une table-ronde