Qu’en est-il de l’état de santé des myes au Saguenay ? Un bilan d’études sur plus d’une décennie

Le fjord du Saguenay, reconnu pour sa faune diversifiée mais aussi pour la contamination reliée aux activités industrielles et anthropiques, a fait l’objet d’un vaste programme de suivi environnemental, entrepris par notre équipe et qui visait à répondre à la question fondamentale : L’état de santé des myes s’est-il modifié dans le fjord du Saguenay ? Dans cet article de synthèse, nous avons regroupé des résultats déjà publiés sur la condition physiologique de Mya arenaria ainsi que des résultats originaux pour extraire des tendances, de façon à répertorier les sites qui s’avèrent critiques pour le bien-être physiologique de la mye. Mya arenaria (LINNÉ, 1758) ou mye des sables, choisie comme espèce sentinelle, a été échantillonnée de 1994 à 2007, en période de maturité sexuelle, dans des sites situés à l’intérieur du fjord et à son embouchure. Les objectifs de cet article sont de comparer les résultats de différents indices de condition et de suivis hormonaux et de la gamétogenèse de chaque site et en fonction des sexes, pour identifier les sites moins favorables pour la croissance et la reproduction de la mye. Nous avons démontré que les myes de Baie‑Sainte-Catherine subissent des retards de gamétogenèse tandis que les niveaux d’hormones stéroïdiennes sont très bas à Tadoussac. Ces deux sites sont soumis à des influences portuaires et à la circulation navale. Le site de Baie‑Éternité, plus en amont, se caractérise par des influences portuaires (huiles et peintures antisalissures) et une forte contamination métallique de sources urbaines et terrigènes. Anse‑aux‑Érables est un site près des influences industrielles, tandis que Anse‑Saint‑Jean est fortement influencée par les effluents municipaux et domestiques. D’amont en aval sur la rivière Saguenay, les myes des sites Anse‑à‑la‑Croix, Anse‑aux‑Érables, Petit‑Saguenay, Anse‑à‑la‑Barque, Tadoussac et Pointe‑aux‑Alouettes ont montré une croissance moindre. Les sites de Baie‑Éternité, Anse‑aux‑Érables, Anse‑Saint‑Jean et Baie-Sainte-Catherine ont un indice de maturité sexuelle moindre qu’aux autres sites, les données regroupées démontrant que ce sont les sites les plus influencés dans le fjord du Saguenay, résultats corroborés par les résultats de phagocytose. Toutes ces données démontrent que l’état physiologique de la mye répond à différents facteurs, anthropiques, biotiques et abiotiques, et que les sources ponctuelles de contamination viennent renforcer les effets négatifs de paramètres abiotiques telles la température et les conditions trophiques.The Saguenay fjord has been submitted for many years to anthropogenic influences. We surveyed this ecosystem between 1994 and 2007 to assess if Mya arenaria health status was altered by the contamination present in this ecosystem. The physiological condition of clams was determined using grouped annual data from sites at the mouth and in the Saguenay fjord. The results were analyzed according to sex and sites for all the samplings done during the active gametogenesis. The aims of this paper are to compare results of condition signs, gametogenesis stages and hormonal levels between sites and according to sex, to finally identify which sites were less favorable for the growth and reproduction of clams. We have shown that clams from Baie-Sainte-Catherine had delayed gametogenesis while those from Tadoussac showed very low steroid hormonal levels. Portuary and naval circulation influences could explain these particular results that also correspond to those from phagocytosis. Upstream in Baie‑Éternité, portuary influences (oils, anti-fouling paints) and metallic inputs from urban and terrigenous sources were reported. In Anse-aux-Érables, metallic contamination comes from industrial sources, while Anse-Saint‑Jean is influenced by sewage discharges from domestic and urban origin. From upstream to downstream, clams from Anse‑à‑la‑Croix, Anse‑aux‑Érables, Petit‑Saguenay, Anse‑à‑la‑Barque, Tadoussac and Pointe‑aux‑Alouettes showed decreased growth. Baie‑Éternité, Anse‑aux‑Érables, Anse‑Saint‑Jean and Baie-Sainte-Catherine sites, with their lower sexual maturity index and decreased phagocytosis, were shown to be the more influenced by contamination. All these data show that physiological condition of Mya arenaria reflects the combined effects of abiotic factors such as contamination, trophic conditions and site characteristics

Factors Impacting the Variability of Post-Fire Forest Regeneration in Central European Pine Plantations

Fire is increasingly posing a risk to forests and plantations, even in the temperate latitudes of central Europe. Little is known about fire ecology in this region, and therefore, appropriate approaches for the management and reforestation of burned sites are mostly lacking. In a Scots pine plantation region in Brandenburg (northeast Germany), the early tree regeneration of two nearby areas that burned 1 year apart was investigated. We observed that 3 years after the fire events, the forest in one study area showed a relatively high regeneration with a mean density of 7765 saplings/ha, clearly dominated by European aspen (93%); whereas the other study area showed a lower mean density of 5061 saplings/ha, dominated by Scots pine (71%) and aspen (15%). Three years after the fires, the difference in aspen density was 11-fold between the two areas. We studied the effects of several variables about soil and environmental properties on the aspen establishment in these two study areas in the second and third years after the fire events. We found that the post-fire aspen regeneration was influenced by several factors, including soil texture, soil disturbance from forest management, volume of deadwood, and browsing. We also discussed that weather conditions during seed production and germination might have played a role in the difference in aspen establishment between the two study areas. We concluded that the post-fire forest regeneration potential in the study region is highly variable and could come under critical pressure as climate change progresses

The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory. Athena is a versatile observatory designed to address the Hot and Energetic Universe science theme, as selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), X-IFU aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over a hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (including the X-IFU cryostat and the cooling chain), due to an unanticipated cost overrun of Athena. In this paper, after illustrating the breakthrough capabilities of the X-IFU, we describe the instrument as presented at its SRR (i.e. in the course of its preliminary definition phase, so-called B1), browsing through all the subsystems and associated requirements. We then show the instrument budgets, with a particular emphasis on the anticipated budgets of some of its key performance parameters, such as the instrument efficiency, spectral resolution, energy scale knowledge, count rate capability, non X-ray background and target of opportunity efficiency. Finally, we briefly discuss the ongoing key technology demonstration activities, the calibration and the activities foreseen in the X-IFU Instrument Science Center, touch on communication and outreach activities, the consortium organisation and the life cycle assessment of X-IFU aiming at minimising the environmental footprint, associated with the development of the instrument. Thanks to the studies conducted so far on X-IFU, it is expected that along the design-to-cost exercise requested by ESA, the X-IFU will maintain flagship capabilities in spatially resolved high resolution X-ray spectroscopy, enabling most of the original X-IFU related scientific objectives of the Athena mission to be retained. The X-IFU will be provided by an international consortium led by France, The Netherlands and Italy, with ESA member state contributions from Belgium, Czech Republic, Finland, Germany, Poland, Spain, Switzerland, with additional contributions from the United States and Japan.The French contribution to X-IFU is funded by CNES, CNRS and CEA. This work has been also supported by ASI (Italian Space Agency) through the Contract 2019-27-HH.0, and by the ESA (European Space Agency) Core Technology Program (CTP) Contract No. 4000114932/15/NL/BW and the AREMBES - ESA CTP No.4000116655/16/NL/BW. This publication is part of grant RTI2018-096686-B-C21 funded by MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”. This publication is part of grant RTI2018-096686-B-C21 and PID2020-115325GB-C31 funded by MCIN/AEI/10.13039/501100011033

The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile observatory designed to address the Hot and Energetic Universe science theme, selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), it aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over an hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (including the X-IFU cryostat and the cooling chain), due to an unanticipated cost overrun of Athena. In this paper, after illustrating the breakthrough capabilities of the X-IFU, we describe the instrument as presented at its SRR, browsing through all the subsystems and associated requirements. We then show the instrument budgets, with a particular emphasis on the anticipated budgets of some of its key performance parameters. Finally we briefly discuss on the ongoing key technology demonstration activities, the calibration and the activities foreseen in the X-IFU Instrument Science Center, and touch on communication and outreach activities, the consortium organisation, and finally on the life cycle assessment of X-IFU aiming at minimising the environmental footprint, associated with the development of the instrument. Thanks to the studies conducted so far on X-IFU, it is expected that along the design-to-cost exercise requested by ESA, the X-IFU will maintain flagship capabilities in spatially resolved high resolution X-ray spectroscopy, enabling most of the original X-IFU related scientific objectives of the Athena mission to be retained. (abridged).Comment: 48 pages, 29 figures, Accepted for publication in Experimental Astronomy with minor editin

Machine learning-assisted extreme events forecasting in Kerr ring resonators

Predicting complex nonlinear dynamical systems has been even more urgent because of the emergence of extreme events such as earthquakes, volcanic eruptions, extreme weather events (lightning, hurricanes/cyclones, blizzards, tornadoes), and giant oceanic rogue waves, to mention a few. The recent milestones in the machine learning framework o↵er a new prospect in this area. For a high dimensional chaotic system, increasing the system’s size causes an augmentation of the complexity and, finally, the size of the artificial neural network. Here, we propose a new supervised machine learning strategy to locally forecast bursts occurring in the turbulent regime of a fiber ring cavity

X-IFU/Athena view of the most distant galaxy clusters in the Universe

International audienceThe X-ray Integral Field Unit (X-IFU) on-board the second large ESA mission "Athena" will be a high spatial (5") and spectral (2.5eV) resolution X-ray imaging spectrometer, operating in the 0.2-12 keV energy band. It will address the science question of the assembly and evolution through cosmic time of the largest halos of matter in the Universe, groups and clusters of galaxies. To this end, we present an on-going feasibility study to demonstrate the X-IFU capabilities to unveil the physics of massive halos at their epoch of formation. Starting from a distant (z=2) group of galaxies (M500 = 7 10^13 M⊙/h) extracted from the HYDRANGEA cosmological and hydrodynamical numerical simulations, we perform an end-to-end simulation of X-IFU observations. From the reconstruction of the global, 1D and 2D quantities, we plan to investigate the various X-IFU science cases for clusters of galaxies, such as the chemical enrichment of the intra-cluster medium (ICM), the dynamical assembly of groups and clusters and the impact of feedback from galaxy and super-massive black hole evolution