Project acronym A-BINGOS
Project Accreting binary populations in Nearby Galaxies: Observations and Simulations
Researcher (PI) Andreas Zezas
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Country Greece
Call Details Consolidator Grant (CoG), PE9, ERC-2013-CoG
Summary "High-energy observations of our Galaxy offer a good, albeit not complete, picture of the X-ray source populations, in particular the accreting binary sources. Recent ability to study accreting binaries in nearby galaxies has shown that we would be short-sighted if we restricted ourselves to our Galaxy or to a few nearby ones. I propose an ambitious project that involves a comprehensive study of all the galaxies within 10 Mpc for which we can study in detail their X-ray sources and stellar populations. The study will combine data from a unique suite of observatories (Chandra, XMM-Newton, HST, Spitzer) with state-of-the-art theoretical modelling of binary systems. I propose a novel approach that links the accreting binary populations to their parent stellar populations and surpasses any current studies of X-ray binary populations, both in scale and in scope, by: (a) combining methods and results from several different areas of astrophysics (compact objects, binary systems, stellar populations, galaxy evolution); (b) using data from almost the whole electromagnetic spectrum (infrared to X-ray bands); (c) identifying and studying the different sub-populations of accreting binaries; and (d) performing direct comparison between observations and theoretical predictions, over a broad parameter space. The project: (a) will answer the long-standing question of the formation efficiency of accreting binaries in different environments; and (b) will constrain their evolutionary paths. As by-products the project will provide eagerly awaited input to the fields of gravitational-wave sources, γ-ray bursts, and X-ray emitting galaxies at cosmological distances and it will produce a heritage multi-wavelength dataset and library of models for future studies of galaxies and accreting binaries."
Summary
"High-energy observations of our Galaxy offer a good, albeit not complete, picture of the X-ray source populations, in particular the accreting binary sources. Recent ability to study accreting binaries in nearby galaxies has shown that we would be short-sighted if we restricted ourselves to our Galaxy or to a few nearby ones. I propose an ambitious project that involves a comprehensive study of all the galaxies within 10 Mpc for which we can study in detail their X-ray sources and stellar populations. The study will combine data from a unique suite of observatories (Chandra, XMM-Newton, HST, Spitzer) with state-of-the-art theoretical modelling of binary systems. I propose a novel approach that links the accreting binary populations to their parent stellar populations and surpasses any current studies of X-ray binary populations, both in scale and in scope, by: (a) combining methods and results from several different areas of astrophysics (compact objects, binary systems, stellar populations, galaxy evolution); (b) using data from almost the whole electromagnetic spectrum (infrared to X-ray bands); (c) identifying and studying the different sub-populations of accreting binaries; and (d) performing direct comparison between observations and theoretical predictions, over a broad parameter space. The project: (a) will answer the long-standing question of the formation efficiency of accreting binaries in different environments; and (b) will constrain their evolutionary paths. As by-products the project will provide eagerly awaited input to the fields of gravitational-wave sources, γ-ray bursts, and X-ray emitting galaxies at cosmological distances and it will produce a heritage multi-wavelength dataset and library of models for future studies of galaxies and accreting binaries."
Max ERC Funding
1 242 000 €
Duration
Start date: 2014-04-01, End date: 2019-03-31
Project acronym ASSESS
Project Episodic Mass Loss in the Most Massive Stars: Key to Understanding the Explosive Early Universe
Researcher (PI) Alceste BONANOS
Host Institution (HI) ETHNIKO ASTEROSKOPEIO ATHINON
Country Greece
Call Details Consolidator Grant (CoG), PE9, ERC-2017-COG
Summary Massive stars dominate their surroundings during their short lifetimes, while their explosive deaths impact the chemical evolution and spatial cohesion of their hosts. After birth, their evolution is largely dictated by their ability to remove layers of hydrogen from their envelopes. Multiple lines of evidence are pointing to violent, episodic mass-loss events being responsible for removing a large part of the massive stellar envelope, especially in low-metallicity galaxies. Episodic mass loss, however, is not understood theoretically, neither accounted for in state-of-the-art models of stellar evolution, which has far-reaching consequences for many areas of astronomy. We aim to determine whether episodic mass loss is a dominant process in the evolution of the most massive stars by conducting the first extensive, multi-wavelength survey of evolved massive stars in the nearby Universe. The project hinges on the fact that mass-losing stars form dust and are bright in the mid-infrared. We plan to (i) derive physical parameters of a large sample of dusty, evolved targets and estimate the amount of ejected mass, (ii) constrain evolutionary models, (iii) quantify the duration and frequency of episodic mass loss as a function of metallicity. The approach involves applying machine-learning algorithms to existing multi-band and time-series photometry of luminous sources in ~25 nearby galaxies. Dusty, luminous evolved massive stars will thus be automatically classified and follow-up spectroscopy will be obtained for selected targets. Atmospheric and SED modeling will yield parameters and estimates of time-dependent mass loss for ~1000 luminous stars. The emerging trend for the ubiquity of episodic mass loss, if confirmed, will be key to understanding the explosive early Universe and will have profound consequences for low-metallicity stars, reionization, and the chemical evolution of galaxies.
Summary
Massive stars dominate their surroundings during their short lifetimes, while their explosive deaths impact the chemical evolution and spatial cohesion of their hosts. After birth, their evolution is largely dictated by their ability to remove layers of hydrogen from their envelopes. Multiple lines of evidence are pointing to violent, episodic mass-loss events being responsible for removing a large part of the massive stellar envelope, especially in low-metallicity galaxies. Episodic mass loss, however, is not understood theoretically, neither accounted for in state-of-the-art models of stellar evolution, which has far-reaching consequences for many areas of astronomy. We aim to determine whether episodic mass loss is a dominant process in the evolution of the most massive stars by conducting the first extensive, multi-wavelength survey of evolved massive stars in the nearby Universe. The project hinges on the fact that mass-losing stars form dust and are bright in the mid-infrared. We plan to (i) derive physical parameters of a large sample of dusty, evolved targets and estimate the amount of ejected mass, (ii) constrain evolutionary models, (iii) quantify the duration and frequency of episodic mass loss as a function of metallicity. The approach involves applying machine-learning algorithms to existing multi-band and time-series photometry of luminous sources in ~25 nearby galaxies. Dusty, luminous evolved massive stars will thus be automatically classified and follow-up spectroscopy will be obtained for selected targets. Atmospheric and SED modeling will yield parameters and estimates of time-dependent mass loss for ~1000 luminous stars. The emerging trend for the ubiquity of episodic mass loss, if confirmed, will be key to understanding the explosive early Universe and will have profound consequences for low-metallicity stars, reionization, and the chemical evolution of galaxies.
Max ERC Funding
1 128 750 €
Duration
Start date: 2018-09-01, End date: 2023-08-31
Project acronym CAUSALPATH
Project Next Generation Causal Analysis: Inspired by the Induction of Biological Pathways from Cytometry Data
Researcher (PI) Ioannis Tsamardinos
Host Institution (HI) PANEPISTIMIO KRITIS
Country Greece
Call Details Consolidator Grant (CoG), PE6, ERC-2013-CoG
Summary Discovering the causal mechanisms of a complex system of interacting components is necessary in order to control it. Computational Causal Discovery (CD) is a field that offers the potential to discover causal relations under certain conditions from observational data alone or with a limited number of interventions/manipulations.
An important, challenging biological problem that may take decades of experimental work is the induction of biological cellular pathways; pathways are informal causal models indispensable in biological research and drug design. Recent exciting advances in flow/mass cytometry biotechnology allow the generation of large-sample datasets containing measurements on single cells, thus setting the problem of pathway learning suitable for CD methods.
CAUSALPATH builds upon and further advances recent breakthrough developments in CD methods to enable the induction of biological pathways from cytometry and other omics data. As a testbed problem we focus on the differentiation of human T-cells; these are involved in autoimmune and inflammatory diseases, as well as cancer and thus, are targets of new drug development for a range of chronic diseases. The biological problem acts as our campus for general novel formalisms, practical algorithms, and useful tools development, pointing to fundamental CD problems: presence of feedback cycles, presence of latent confounding variables, CD from time-course data, Integrative Causal Analysis (INCA) of heterogeneous datasets and others.
Three features complement CAUSALPATH’s approach: (A) methods development will co-evolve with biological wet-lab experiments periodically testing the algorithmic postulates, (B) Open-source tools will be developed for the non-expert, and (C) Commercial exploitation of the results will be sought out.
CAUSALPATH brings together an interdisciplinary team, committed to this vision. It builds upon the PI’s group recent important results on INCA algorithms.
Summary
Discovering the causal mechanisms of a complex system of interacting components is necessary in order to control it. Computational Causal Discovery (CD) is a field that offers the potential to discover causal relations under certain conditions from observational data alone or with a limited number of interventions/manipulations.
An important, challenging biological problem that may take decades of experimental work is the induction of biological cellular pathways; pathways are informal causal models indispensable in biological research and drug design. Recent exciting advances in flow/mass cytometry biotechnology allow the generation of large-sample datasets containing measurements on single cells, thus setting the problem of pathway learning suitable for CD methods.
CAUSALPATH builds upon and further advances recent breakthrough developments in CD methods to enable the induction of biological pathways from cytometry and other omics data. As a testbed problem we focus on the differentiation of human T-cells; these are involved in autoimmune and inflammatory diseases, as well as cancer and thus, are targets of new drug development for a range of chronic diseases. The biological problem acts as our campus for general novel formalisms, practical algorithms, and useful tools development, pointing to fundamental CD problems: presence of feedback cycles, presence of latent confounding variables, CD from time-course data, Integrative Causal Analysis (INCA) of heterogeneous datasets and others.
Three features complement CAUSALPATH’s approach: (A) methods development will co-evolve with biological wet-lab experiments periodically testing the algorithmic postulates, (B) Open-source tools will be developed for the non-expert, and (C) Commercial exploitation of the results will be sought out.
CAUSALPATH brings together an interdisciplinary team, committed to this vision. It builds upon the PI’s group recent important results on INCA algorithms.
Max ERC Funding
1 724 000 €
Duration
Start date: 2015-01-01, End date: 2019-12-31
Project acronym D-TECT
Project Does dust triboelectrification affect our climate?
Researcher (PI) Vasileios AMOIRIDIS
Host Institution (HI) ETHNIKO ASTEROSKOPEIO ATHINON
Country Greece
Call Details Consolidator Grant (CoG), PE10, ERC-2016-COG
Summary The recent IPCC report identifies mineral dust and the associated uncertainties in climate projections as key topics for future research. Dust size distribution in climate models controls the dust-radiation-cloud interactions and is a major contributor to these uncertainties. Observations show that the coarse mode of dust can be sustained during long-range transport, while current understanding fails in explaining why the lifetime of large airborne dust particles is longer than expected from gravitational settling theories. This discrepancy between observations and theory suggests that other processes counterbalance the effect of gravity along transport. D-TECT envisages filling this knowledge gap by studying the contribution of the triboelectrification (contact electrification) on particle removal processes. Our hypothesis is that triboelectric charging generates adequate electric fields to hold large dust particles up in the atmosphere. D-TECT aims to (i) parameterize the physical mechanisms responsible for dust triboelectrification; (ii) assess the impact of electrification on dust settling; (iii) quantify the climatic impacts of the process, particularly the effect on the dust size evolution during transport, on dry deposition and on CCN/IN reservoirs, and the effect of the electric field on particle orientation and on radiative transfer. The approach involves the development of a novel specialized high-power lidar system to detect and characterize aerosol particle orientation and a large-scale field experiment in the Mediterranean Basin using unprecedented ground-based remote sensing and airborne in-situ observation synergies. Considering aerosol-electricity interactions, the observations will be used to improve theoretical understanding and simulations of dust lifecycle. The project will provide new fundamental understanding, able to open new horizons for weather and climate science, including biogeochemistry, volcanic ash and extraterrestrial dust research.
Summary
The recent IPCC report identifies mineral dust and the associated uncertainties in climate projections as key topics for future research. Dust size distribution in climate models controls the dust-radiation-cloud interactions and is a major contributor to these uncertainties. Observations show that the coarse mode of dust can be sustained during long-range transport, while current understanding fails in explaining why the lifetime of large airborne dust particles is longer than expected from gravitational settling theories. This discrepancy between observations and theory suggests that other processes counterbalance the effect of gravity along transport. D-TECT envisages filling this knowledge gap by studying the contribution of the triboelectrification (contact electrification) on particle removal processes. Our hypothesis is that triboelectric charging generates adequate electric fields to hold large dust particles up in the atmosphere. D-TECT aims to (i) parameterize the physical mechanisms responsible for dust triboelectrification; (ii) assess the impact of electrification on dust settling; (iii) quantify the climatic impacts of the process, particularly the effect on the dust size evolution during transport, on dry deposition and on CCN/IN reservoirs, and the effect of the electric field on particle orientation and on radiative transfer. The approach involves the development of a novel specialized high-power lidar system to detect and characterize aerosol particle orientation and a large-scale field experiment in the Mediterranean Basin using unprecedented ground-based remote sensing and airborne in-situ observation synergies. Considering aerosol-electricity interactions, the observations will be used to improve theoretical understanding and simulations of dust lifecycle. The project will provide new fundamental understanding, able to open new horizons for weather and climate science, including biogeochemistry, volcanic ash and extraterrestrial dust research.
Max ERC Funding
1 968 000 €
Duration
Start date: 2017-09-01, End date: 2023-08-31
Project acronym DeFiNER
Project Nucleotide Excision Repair: Decoding its Functional Role in Mammals
Researcher (PI) Georgios Garinis
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Country Greece
Call Details Consolidator Grant (CoG), LS4, ERC-2014-CoG
Summary Genome maintenance, chromatin remodelling and transcription are tightly linked biological processes that are currently poorly understood and vastly unexplored. Nucleotide excision repair (NER) is a major DNA repair pathway that mammalian cells employ to maintain their genome intact and faithfully transmit it into their progeny. Besides cancer and aging, however, defects in NER give rise to developmental disorders whose clinical heterogeneity and varying severity can only insufficiently be explained by the DNA repair defect. Recent work reveals that NER factors play a role, in addition to DNA repair, in transcription and the three-dimensional organization of our genome. Indeed, NER factors are now known to function in the regulation of gene expression, the transcriptional reprogramming of pluripotent stem cells and the fine-tuning of growth hormones during mammalian development. In this regard, the non-random organization of our genome, chromatin and the process of transcription itself are expected to play paramount roles in how NER factors coordinate, prioritize and execute their distinct tasks during development and disease progression. At present, however, no solid evidence exists as to how NER is functionally involved in such complex processes, what are the NER-associated protein complexes and underlying gene networks or how NER factors operate within the complex chromatin architecture. This is primarily due to our difficulties in dissecting the diverse functional contributions of NER proteins in an intact organism. Here, we propose to use a unique series of knock-in, transgenic and NER progeroid mice to decode the functional role of NER in mammals, thus paving the way for understanding how genome maintenance pathways are connected to developmental defects and disease mechanisms in vivo.
Summary
Genome maintenance, chromatin remodelling and transcription are tightly linked biological processes that are currently poorly understood and vastly unexplored. Nucleotide excision repair (NER) is a major DNA repair pathway that mammalian cells employ to maintain their genome intact and faithfully transmit it into their progeny. Besides cancer and aging, however, defects in NER give rise to developmental disorders whose clinical heterogeneity and varying severity can only insufficiently be explained by the DNA repair defect. Recent work reveals that NER factors play a role, in addition to DNA repair, in transcription and the three-dimensional organization of our genome. Indeed, NER factors are now known to function in the regulation of gene expression, the transcriptional reprogramming of pluripotent stem cells and the fine-tuning of growth hormones during mammalian development. In this regard, the non-random organization of our genome, chromatin and the process of transcription itself are expected to play paramount roles in how NER factors coordinate, prioritize and execute their distinct tasks during development and disease progression. At present, however, no solid evidence exists as to how NER is functionally involved in such complex processes, what are the NER-associated protein complexes and underlying gene networks or how NER factors operate within the complex chromatin architecture. This is primarily due to our difficulties in dissecting the diverse functional contributions of NER proteins in an intact organism. Here, we propose to use a unique series of knock-in, transgenic and NER progeroid mice to decode the functional role of NER in mammals, thus paving the way for understanding how genome maintenance pathways are connected to developmental defects and disease mechanisms in vivo.
Max ERC Funding
1 995 000 €
Duration
Start date: 2016-01-01, End date: 2021-06-30
Project acronym GHOST
Project Geographies and Histories of the Ottoman Supernatural Tradition Exploring Magic, the Marvelous, and the Strange in Ottoman Mentalities
Researcher (PI) Marinos SARIGIANNIS
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Country Greece
Call Details Consolidator Grant (CoG), SH6, ERC-2017-COG
Summary The project aims to explore Ottoman notions and belief systems concerning the supernatural. Its major objectives will be to explore the meaning and content of the perceptions of the “supernatural”, to localize such beliefs in the various Ottoman systems of thought, to analyze the changes that took place and to associate them with emerging or declining layers of culture and specific social groups. The project will address larger debates in recent historiography about the relevance of the “disenchantment” and “enlightenment” paradigms, integrating Ottoman intellectual history into the broader early modern cultural history.
The research team, composed of the PI, three post-doctoral fellows, four collaborating researchers, five post-graduate students and a technical assistant, will explore these objectives and produce a web portal (containing crowd-sourced dictionaries and bibliographies, open access papers and other material), three international meetings, monographs and papers, and an annual open-access periodical journal. Specific research modules will study the rationalist trends in Ottoman science, various aspects of the Ottoman occult and magic, and the formation and development of the Ottoman cosmological culture. A monograph will be written by the PI and dwell in: the various conceptions of the supernatural/preternatural and their development, the presence of spirits/jinn in Ottoman world image, theory and practice of Ottoman magic, attitudes toward folklore traditions, saintly miracles, and “marvelous geographies”. Monographs will also be produced by the post-doctoral fellows.
The project proposes an innovative approach in many ways, in a subject very much in the frontiers of the field; by exploring the supernatural and the occult in the context of the Ottoman Weltanschauung, the project will address a wider problématique on the Ottoman culture and its place in early modernity, especially as it will focus to the role of different cultural and social layers.
Summary
The project aims to explore Ottoman notions and belief systems concerning the supernatural. Its major objectives will be to explore the meaning and content of the perceptions of the “supernatural”, to localize such beliefs in the various Ottoman systems of thought, to analyze the changes that took place and to associate them with emerging or declining layers of culture and specific social groups. The project will address larger debates in recent historiography about the relevance of the “disenchantment” and “enlightenment” paradigms, integrating Ottoman intellectual history into the broader early modern cultural history.
The research team, composed of the PI, three post-doctoral fellows, four collaborating researchers, five post-graduate students and a technical assistant, will explore these objectives and produce a web portal (containing crowd-sourced dictionaries and bibliographies, open access papers and other material), three international meetings, monographs and papers, and an annual open-access periodical journal. Specific research modules will study the rationalist trends in Ottoman science, various aspects of the Ottoman occult and magic, and the formation and development of the Ottoman cosmological culture. A monograph will be written by the PI and dwell in: the various conceptions of the supernatural/preternatural and their development, the presence of spirits/jinn in Ottoman world image, theory and practice of Ottoman magic, attitudes toward folklore traditions, saintly miracles, and “marvelous geographies”. Monographs will also be produced by the post-doctoral fellows.
The project proposes an innovative approach in many ways, in a subject very much in the frontiers of the field; by exploring the supernatural and the occult in the context of the Ottoman Weltanschauung, the project will address a wider problématique on the Ottoman culture and its place in early modernity, especially as it will focus to the role of different cultural and social layers.
Max ERC Funding
1 289 824 €
Duration
Start date: 2018-03-01, End date: 2023-02-28
Project acronym HETEROPOLITICS
Project Refiguring the Common and the Political
Researcher (PI) Alexandros KIOUPKIOLIS
Host Institution (HI) ARISTOTELIO PANEPISTIMIO THESSALONIKIS
Country Greece
Call Details Consolidator Grant (CoG), SH5, ERC-2016-COG
Summary Heteropolitics is a project in contemporary political theory which purports to contribute to the renewal of political thought on the ‘common’ (communities and the commons) and the political in tandem. The common implies a variable interaction between differences which communicate and collaborate in and through their differences, converging partially on practices and particular pursuits. The political pertains to processes through which plural communities manage themselves in ways which enable mutual challenges, deliberation, and creative agency.
Since the dawn of the 21st century, a growing interest in rethinking and reconfiguring community has spread among theorists, citizens and social movements (see e.g. Esposito 2013; Dardot & Laval 2014; Amin & Roberts 2008). This has been triggered by a complex tangle of social, economic and political conditions. Climate change, economic crises, globalization, increasing migration flows and the malaise of liberal democracies loom large among them.
These issues are essentially political. Rethinking and refiguring communities goes hand in hand thus with rethinking and reinventing politics. Hence ‘hetero-politics’, the quest for another politics, which can establish bonds of commonality across differences and can enable action in common without re-enacting the closures of ‘organic’ community or the violence of transformative politics in the past.
Heteropolitics will seek to break new ground by combining an extended re-elaboration of contemporary political theory with a more empirically grounded research into alternative and incipient practices of community building and self-governance in: education; the social economy; art; new modes of civic engagement by young people; new platforms of citizens’ participation in municipal politics; network communities, and other social fields (Relevant cases include Sardex, a community currency in Sardinia; Barcelona en Comú, a citizens’ platform governing the city of Barcelona, etc.)
Summary
Heteropolitics is a project in contemporary political theory which purports to contribute to the renewal of political thought on the ‘common’ (communities and the commons) and the political in tandem. The common implies a variable interaction between differences which communicate and collaborate in and through their differences, converging partially on practices and particular pursuits. The political pertains to processes through which plural communities manage themselves in ways which enable mutual challenges, deliberation, and creative agency.
Since the dawn of the 21st century, a growing interest in rethinking and reconfiguring community has spread among theorists, citizens and social movements (see e.g. Esposito 2013; Dardot & Laval 2014; Amin & Roberts 2008). This has been triggered by a complex tangle of social, economic and political conditions. Climate change, economic crises, globalization, increasing migration flows and the malaise of liberal democracies loom large among them.
These issues are essentially political. Rethinking and refiguring communities goes hand in hand thus with rethinking and reinventing politics. Hence ‘hetero-politics’, the quest for another politics, which can establish bonds of commonality across differences and can enable action in common without re-enacting the closures of ‘organic’ community or the violence of transformative politics in the past.
Heteropolitics will seek to break new ground by combining an extended re-elaboration of contemporary political theory with a more empirically grounded research into alternative and incipient practices of community building and self-governance in: education; the social economy; art; new modes of civic engagement by young people; new platforms of citizens’ participation in municipal politics; network communities, and other social fields (Relevant cases include Sardex, a community currency in Sardinia; Barcelona en Comú, a citizens’ platform governing the city of Barcelona, etc.)
Max ERC Funding
758 031 €
Duration
Start date: 2017-04-01, End date: 2020-12-31
Project acronym iMAC-FUN
Project Dissecting novel mechanisms of iron regulation during macrophage-fungal interplay
Researcher (PI) Georgios Chamilos
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Country Greece
Call Details Consolidator Grant (CoG), LS6, ERC-2019-COG
Summary Airborne filamentous fungi (molds) are major causes of respiratory diseases in an expanding population of patients with complex immune and metabolic defects. Invasive mold infections (IMI) are associated with substantial mortality and enormous economic impact. Understanding pathogenesis of IMI is an unmet need for design of better therapies. We have put forward a novel mechanism for the pathogenesis of IMI, according to which development of IMI requires two discrete mechanisms (a) phagosome maturation arrest via inhibition of LC3-associated phagocytosis (LAP), which allows intracellular persistence of fungal conidia (spores), and (b) alteration in iron homeostasis, resulting in invasive fungal growth and lysis of the macrophage. On the pathogen site, fungal melanin targets LAP and affects macrophage metal homeostasis. On the macrophage site, iron distribution in subcellular compartments of all eukaryotic cells is controlled by ferric reductases and divalent cation transporters, in a process that remains molecularly unexplored. During mold infection a group of ferric reductases represent the most prominently transcriptionally modulated iron regulatory genes in macrophages. Thus, iron regulation is the critical determinant of macrophage-fungal interplay and is the focus of this project. We will use molds as model pathogens to (i) dissect the role of selected ferric reductases in infection, (ii) identify novel iron transporters implicated in host defense (iii) and explore mechanisms of melanin interference with iron regulation in macrophages. To this end, we will employ a robust, unbiased, approach combining transcriptomics, metalloproteomics, in vivo RNAi screening in Drosophila model of IMI, and validation studies in transgenic mice and eventually in human patients ex vivo. Dissecting the function of novel iron regulators in the macrophage will have profound impact on iron biology and is likely to have direct therapeutic implications for the management of IMI.
Summary
Airborne filamentous fungi (molds) are major causes of respiratory diseases in an expanding population of patients with complex immune and metabolic defects. Invasive mold infections (IMI) are associated with substantial mortality and enormous economic impact. Understanding pathogenesis of IMI is an unmet need for design of better therapies. We have put forward a novel mechanism for the pathogenesis of IMI, according to which development of IMI requires two discrete mechanisms (a) phagosome maturation arrest via inhibition of LC3-associated phagocytosis (LAP), which allows intracellular persistence of fungal conidia (spores), and (b) alteration in iron homeostasis, resulting in invasive fungal growth and lysis of the macrophage. On the pathogen site, fungal melanin targets LAP and affects macrophage metal homeostasis. On the macrophage site, iron distribution in subcellular compartments of all eukaryotic cells is controlled by ferric reductases and divalent cation transporters, in a process that remains molecularly unexplored. During mold infection a group of ferric reductases represent the most prominently transcriptionally modulated iron regulatory genes in macrophages. Thus, iron regulation is the critical determinant of macrophage-fungal interplay and is the focus of this project. We will use molds as model pathogens to (i) dissect the role of selected ferric reductases in infection, (ii) identify novel iron transporters implicated in host defense (iii) and explore mechanisms of melanin interference with iron regulation in macrophages. To this end, we will employ a robust, unbiased, approach combining transcriptomics, metalloproteomics, in vivo RNAi screening in Drosophila model of IMI, and validation studies in transgenic mice and eventually in human patients ex vivo. Dissecting the function of novel iron regulators in the macrophage will have profound impact on iron biology and is likely to have direct therapeutic implications for the management of IMI.
Max ERC Funding
2 000 000 €
Duration
Start date: 2020-09-01, End date: 2025-08-31
Project acronym MIX2FIX
Project Hybrid, organic-inorganic chalcogenide optoelectronics
Researcher (PI) Thomas STERGIOPOULOS
Host Institution (HI) ARISTOTELIO PANEPISTIMIO THESSALONIKIS
Country Greece
Call Details Consolidator Grant (CoG), PE8, ERC-2018-COG
Summary The new generation of optoelectronics seeks for emerging semiconductors which combine high performance with low cost. Lead halide organic-inorganic perovskites manifest as excellent optoelectronic materials for this purpose, but at the expense of robustness and environmental compatibility. This presents a major challenge which this research addresses directly. Viable alternatives have to be identified. To tackle this challenge, MIX2FIX proposes to develop a new class of solution-processable optoelectronic devices based on air-stable, non-toxic metal chalcogenides endowed with an organic part, which will facilitate solution-processing and potentially enrich the compounds with the spectacular properties of halide perovskites. To achieve this, the CoG project has set the following objectives: (i) designing and developing optoelectronically-active, organic-inorganic chalcogenide thin films that have never been explored before, by mimicking strategies from established perovskite technology, (ii) devising means to improve their optoelectronic quality so as to be comparable with the best single-crystal semiconductors and (iii) implementing optimized materials into boundary-pushing PV and LED devices. Addressing these objectives will enable the development of novel functional hybrids at the boundaries of perovskite and chalcogenide thin films. With this, optoelectronics with efficiency and stability, comparable or higher than those of lead halide perovskite or chalcopyrite devices, will be demonstrated. This project will therefore permit the transition for emerging optoelectronic materials from toxic lead halide perovskites to green hybrid chalcogenides. Consolidating this unproven but disruptive technology will secure sustainable future for other areas of interest beyond photovoltaics, displays and lighting such as in X-Rays detectors and phototransistors or even beyond optoelectronics, in systems such as batteries and supercapacitors.
Summary
The new generation of optoelectronics seeks for emerging semiconductors which combine high performance with low cost. Lead halide organic-inorganic perovskites manifest as excellent optoelectronic materials for this purpose, but at the expense of robustness and environmental compatibility. This presents a major challenge which this research addresses directly. Viable alternatives have to be identified. To tackle this challenge, MIX2FIX proposes to develop a new class of solution-processable optoelectronic devices based on air-stable, non-toxic metal chalcogenides endowed with an organic part, which will facilitate solution-processing and potentially enrich the compounds with the spectacular properties of halide perovskites. To achieve this, the CoG project has set the following objectives: (i) designing and developing optoelectronically-active, organic-inorganic chalcogenide thin films that have never been explored before, by mimicking strategies from established perovskite technology, (ii) devising means to improve their optoelectronic quality so as to be comparable with the best single-crystal semiconductors and (iii) implementing optimized materials into boundary-pushing PV and LED devices. Addressing these objectives will enable the development of novel functional hybrids at the boundaries of perovskite and chalcogenide thin films. With this, optoelectronics with efficiency and stability, comparable or higher than those of lead halide perovskite or chalcopyrite devices, will be demonstrated. This project will therefore permit the transition for emerging optoelectronic materials from toxic lead halide perovskites to green hybrid chalcogenides. Consolidating this unproven but disruptive technology will secure sustainable future for other areas of interest beyond photovoltaics, displays and lighting such as in X-Rays detectors and phototransistors or even beyond optoelectronics, in systems such as batteries and supercapacitors.
Max ERC Funding
2 731 250 €
Duration
Start date: 2019-09-01, End date: 2024-08-31
Project acronym PASIPHAE
Project Overcoming the Dominant Foreground of Inflationary B-modes: Tomography of Galactic Magnetic Dust via Measurements of Starlight Polarization
Researcher (PI) Konstantinos TASSIS
Host Institution (HI) IDRYMA TECHNOLOGIAS KAI EREVNAS
Country Greece
Call Details Consolidator Grant (CoG), PE9, ERC-2017-COG
Summary An inflation-probing B-mode signal in the polarization of the cosmic microwave background (CMB) would be a discovery of utmost importance in physics. While such a signal is aggressively pursued by experiments around the world, recent Planck results have showed that this breakthrough is still out of reach, because of contamination from Galactic dust. To get to the primordial B-modes, we need to subtract polarized emission of magnetized interstellar dust with high accuracy. A critical piece of this puzzle is the 3D structure of the magnetic field threading dust clouds, which cannot be accessed through microwave observations alone, since they record integrated emission along the line of sight. Instead, observations of a large number of stars at known distances in optical polarization, tracing the same CMB-obscuring dust, can map the magnetic field between them. The Gaia mission is measuring distances to a billion stars, providing an opportunity to produce, the first-ever tomographic map of the Galactic magnetic field, using optical polarization of starlight. Such a map would not only boost CMB polarization foreground removal, but it would also have a profound impact in a wide range of astrophysical research, including interstellar medium physics, high-energy astrophysics, and galactic evolution. Taking advantage of our privately-funded, novel-technology, high-accuracy WALOP optopolarimeters currently under construction, we propose an ambitious optopolarimetric program of unprecedented scale that can meet this challenge: a survey of both northern and southern Galactic polar regions targeted by CMB experiments, covering >10,000 square degrees, which will measure linear optical polarization at 0.2% accuracy of over 360 stars per square degree (over 3.5M stars, a 1000-fold increase over the state of the art), combining wide-field-optimized instruments and an extraordinary commitment of observing time by Skinakas Observatory and the South African Astronomical Observatory.
Summary
An inflation-probing B-mode signal in the polarization of the cosmic microwave background (CMB) would be a discovery of utmost importance in physics. While such a signal is aggressively pursued by experiments around the world, recent Planck results have showed that this breakthrough is still out of reach, because of contamination from Galactic dust. To get to the primordial B-modes, we need to subtract polarized emission of magnetized interstellar dust with high accuracy. A critical piece of this puzzle is the 3D structure of the magnetic field threading dust clouds, which cannot be accessed through microwave observations alone, since they record integrated emission along the line of sight. Instead, observations of a large number of stars at known distances in optical polarization, tracing the same CMB-obscuring dust, can map the magnetic field between them. The Gaia mission is measuring distances to a billion stars, providing an opportunity to produce, the first-ever tomographic map of the Galactic magnetic field, using optical polarization of starlight. Such a map would not only boost CMB polarization foreground removal, but it would also have a profound impact in a wide range of astrophysical research, including interstellar medium physics, high-energy astrophysics, and galactic evolution. Taking advantage of our privately-funded, novel-technology, high-accuracy WALOP optopolarimeters currently under construction, we propose an ambitious optopolarimetric program of unprecedented scale that can meet this challenge: a survey of both northern and southern Galactic polar regions targeted by CMB experiments, covering >10,000 square degrees, which will measure linear optical polarization at 0.2% accuracy of over 360 stars per square degree (over 3.5M stars, a 1000-fold increase over the state of the art), combining wide-field-optimized instruments and an extraordinary commitment of observing time by Skinakas Observatory and the South African Astronomical Observatory.
Max ERC Funding
1 887 500 €
Duration
Start date: 2018-06-01, End date: 2023-05-31
