Revue des principales méthodes d’identification des sources de pollutions fécales des eaux et coquillages

Les contaminations fécales des eaux et des coquillages induisent des risques pour la santé humaine et des pertes économiques liées, entre autres, aux interdictions de baignade et à la fermeture des zones de conchyliculture. La réduction des apports à l’origine de cette contamination est facilitée par une identification précise des sources (humaines ou animales) qui peut aussi servir à hié rarchiser les mesures à adopter en cas de besoin. De nombreux marqueurs ont été proposés à ce titre durant les deux dernières décennies. Ils correspondent :-à des micro-organismes (bactéries, virus ou bactériophages) mis en évidence par des approaches culturales, biochimiques ou moléculaires; -à des molécules chimiques présentes naturellement dans les fèces ou associées à l’une des sources de pollution; -et à la mise en évidence de cellules spécifiques de l’hôte dissimulées dans les matières fécales. Cet article présente ces différentes methods d’identification des sources de contaminations fécales en décrivant leur utilisation et la nature des résultats qu’elles permettent d’obtenir. Le principal corollaire de cette revue bibliographique est qu’il semble nécessaire de coupler différents marqueurs pour pouvoir identifier les sources

A new tool based on faecal stanols can distinguish specific mammalian species in modern and past environments

Publisher PD

Développement d'outils microbiologiques et chimiques permettant d'identifier l'origine des pollutions fécales dans les eaux de baignades

La pollution organique issue des effluents d'élevage et des stations d'épuration urbaines conduit à un problème essentiel de santé publique lié à la contamination des eaux de surface où s'exercent des activités sensibles telles que la baignade. S'il est possible de déterminer les pollutions localisées liées à un dysfonctionnement des systèmes de traitement, il est beaucoup plus difficile d'identifier les pollutions organiques diffuses qui participent pourtant majoritairement à la dégradation de la qualité des eaux de surface. La problématique des pollutions diffuses est d'autant plus importante que la nouvelle réglementation européenne concernant les eaux de baignade (Directive 2006/7/CE) demande de constituer des profils de baignade qui nécessitent une identification et une hiérarchisation des sources de pollutions fécales. Le dénombrement de Escherichia coli et des entérocoques intestinaux stipulé par les textes réglementaires européens, représente actuellement le seul outil analytique permettant la mise en évidence d'une contamination fécale du milieu aquatique, sans toutefois différencier l'origine humaine ou animale de cette contamination. Il est donc nécessaire de développer de nouvelles méthodes de détection de la pollution fécale qui puissent non seulement mettre en évidence une contamination mais aussi en indiquer l'origine. C'est d'ailleurs dans cet objectif que s'est développé depuis quelques années, le concept de "Microbial Source Tracking" ("Traceurs de Sources Microbiennes") qui consiste à identifier à l'aide de marqueurs microbiologiques ou chimiques les sources de pollutions fécales. Dans ce contexte, six laboratoires de recherche se sont associés pour développer des techniques de traçage des contaminations fécales afin de proposer un outil opérationnel utilisable pour différencier les sources de pollution, de leur point d'émission jusqu'au milieu récepteur final que constituent les eaux de surface. Les marqueurs qui ont fait l'objet de cette étude sont des molécules chimiques naturelles (stéroïdes, caféine), des molécules de synthèse retrouvées dans les effluents de stations d'épuration ou des rapports de fluorescence de la matière organique ainsi que des micro-organismes (bactériophages, bactéries). A la suite des développements méthodologiques, plusieurs marqueurs ont été sélectionnés : - bactéries appartenant aux groupes bactériens dominants du tractus intestinal humain (Bifidobacterium adolescentis) et porcin (Lactobacillus amylovorus) ; - Bacteroidales spécifiques des humains, porcins et bovins (HF183, Pig-2-Bac, Rum-2-Bac); - génogroupes humains des bactériophages F ARN spécifiques; - rapports de stéroïdes : coprostanol/(24ethylcoprostanol+coprostanol) (R1) et sitostanol/coprostanol (R2); - caféine, benzophénone et tri(2-chloroethyl)phosphate (TCEP)

Neutron imaging with a Micromegas detector

The micropattern gaseous detector Micromegas has been developed for several years in Saclay and presents good performance for neutron detection. A prototype for neutron imaging has been designed and new results obtained in thermal neutron beams are presented. Based on previous results demonstrating a good 1D spatial resolution, a tomographic image of a multiwire cable has been performed using a 1D Micromegas prototype. The number of pillars supporting the micromesh is too large and leads to local losses of efficiency that distort the tomographic reconstruction. Nevertheless, this first tomographic image achieved with this kind of detector is very encouraging. The next worthwhile development for neutron imaging is to achieve a bi-dimensional detector, which is presented in the second part of this study. The purpose of measurements was to investigate various operational parameters to optimize the spatial resolution. Through these measurements the optimum spatial resolution has been found to be around 160 microns (standard deviation) using Micromegas operating in double amplification mode. Several 2D imaging tests have been carried out. Some of these results have revealed fabrication defects that occurred during the manufacture of Micromegas and that are limiting the full potential of the present neutron imaging system.Comment: 6 pages, 10 figures, presented at IEEE 2004 conference in Roma, Ital

Sources of pro-cyclicality in east Asian financial systems

Procyclicality is a normal feature of economic systems, but financial sector weaknesses can exacerbate it sufficiently to pose a threat to macroeconomic and financial stability. These include shortcomings in bank risk management and governance, in supervision and in terms of dependence on volatile sources of funds. The paper tests econometrically for the importance of such features leading to pro-cyclicality in the financial systems of 11 East Asian countries. This analysis makes it possible to identify specific policy measures for East Asian countries that could limit the extent to which financial systems exacerbate pro-cyclicality

The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS)

Aims. We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters. The sample consists of 603 continuum-faint (−23 < MUV < −14) lensed Lyman-α emitters (producing 959 images) with secure spectroscopic redshifts between 2.9 and 6.7. Combining the power of cluster magnification with 3D spectroscopic observations, we were able to reveal the resolved morphological properties of 268 Lyman-α emitters. Methods. We used a forward-modeling approach to model both Lyman-α and rest-frame UV continuum emission profiles in the source plane and measure spatial extent, ellipticity, and spatial offsets between UV and Lyman-α emission. Results. We find a significant correlation between UV continuum and Lyman-α spatial extent. Our characterization of the Lyman-α halos indicates that the halo size is linked to the physical properties of the host galaxy (SFR, Lyman-α equivalent width, Lyman-α line FWHM). We find that 48% of Lyman-α halos are best fit by an elliptical emission distribution with a median axis ratio of q = 0.48. We observe that 60% of galaxies detected both in UV and Lyman-α emission show a significant spatial offset (ΔLyα − UV). We measure a median offset of ΔLyα − UV = 0.58 ± 0.14 kpc for the entire sample. By comparing the spatial offset values with the size of the UV component, we show that 40% of the offsets could be due to star-forming sub-structures in the UV component, while the larger offsets (60%) are more likely due to greater-distance processes such as scattering effects inside the circumgalactic medium or emission from faint satellites or merging galaxies. Comparisons with a zoom-in radiative hydrodynamics simulation of a typical Lyman-α emitting galaxy show a very good agreement with LLAMAS galaxies and indicate that bright star-formation clumps and satellite galaxies could produce a similar spatial offset distribution

The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS): I. Characterisation of extended Lyman-alpha halos and spatial offsets

Aims. We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters. The sample consists of 603 continuum-faint (23 < MUV<-14) lensed Lyman-α emitters (producing 959 images) with secure spectroscopic redshifts between 2.9 and 6.7. Combining the power of cluster magnification with 3D spectroscopic observations, we were able to reveal the resolved morphological properties of 268 Lyman-α emitters. Methods. We used a forward-modeling approach to model both Lyman-α and rest-frame UV continuum emission profiles in the source plane and measure spatial extent, ellipticity, and spatial offsets between UV and Lyman-α emission. Results. We find a significant correlation between UV continuum and Lyman-α spatial extent. Our characterization of the Lyman-α halos indicates that the halo size is linked to the physical properties of the host galaxy (SFR, Lyman-α equivalent width, Lyman-α line FWHM). We find that 48% of Lyman-α halos are best fit by an elliptical emission distribution with a median axis ratio of q =0.48. We observe that 60% of galaxies detected both in UV and Lyman-α emission show a significant spatial offset (ΔLyα-UV). We measure a median offset of ΔLyα-UV=0.58± 0.14 kpc for the entire sample. By comparing the spatial offset values with the size of the UV component, we show that 40% of the offsets could be due to star-forming sub-structures in the UV component, while the larger offsets (60%) are more likely due to greater-distance processes such as scattering effects inside the circumgalactic medium or emission from faint satellites or merging galaxies. Comparisons with a zoom-in radiative hydrodynamics simulation of a typical Lyman-α emitting galaxy show a very good agreement with LLAMAS galaxies and indicate that bright star-formation clumps and satellite galaxies could produce a similar spatial offset distribution

Relative Decay of Fecal Indicator Bacteria and Human-Associated Markers: A Microcosm Study Simulating Wastewater Input into Seawater and Freshwater

Fecal contaminations of inland and coastal waters induce risks to human health and economic losses. To improve water management, specific markers have been developed to differentiate between sources of contamination. This study investigates the relative decay of fecal indicator bacteria (FIB, Escherichia coli and enterococci) and six human-associated markers (two bacterial markers: Bacteroidales HF183 (HF183) and Bifidobacterium adolescentis (BifAd); one viral marker: genogroup II F-specific RNA bacteriophages (FRNAPH II); three chemical markers: caffeine and two fecal stanol ratios) in freshwater and seawater microcosms seeded with human wastewater. These experiments were performed in darkness, at 20 °C and under aerobic conditions. The modeling of the decay curves allows us (i) to compare FIB and markers and (ii) to classify markers according to their persistence in seawater (FRNAPH II &lt; HF183, stanol ratios &lt; BifAd, caffeine) and in freshwater (HF183, stanol ratios &lt; FRNAPH II &lt; BifAd &lt; caffeine). Although those results depend on the experimental conditions, this study represents a necessary step to develop and validate an interdisciplinary toolbox for the investigation of the sources of fecal contaminations