ERC FUNDED PROJECTS

During an organism’s development it must integrate internal and external information. An example in plants, whose development stretches across their lifetime, is the coordination between environmental stimuli and endogenous cues on regulating the key hormone gibberellin (GA). The present challenge is to understand how these diverse signals influence GA levels and how GA signalling leads to diverse GA responses. This challenge is deepened by a fundamental problem in hormone research: the specific responses directed by a given hormone often depend on the cell-type, timing, and amount of hormone accumulation, but hormone concentrations are most often assessed at the organism or tissue level. Our approach, based on a novel optogenetic biosensor, GA Perception Sensor 1 (GPS1), brings the goal of high-resolution quantification of GA in vivo within reach. In plants expressing GPS1, we observe gradients of GA in elongating root and shoot tissues. We now aim to understand how a series of independently tunable enzymatic and transport activities combine to articulate the GA gradients that we observe. We further aim to discover the mechanisms by which endogenous and environmental signals regulate these GA enzymes and transporters. Finally, we aim to understand how one of these signals, light, regulates GA patterns to influence dynamic cell growth and organ behavior. Our overarching goal is a systems level understanding of the signal integration upstream and growth programming downstream of GA. The groundbreaking aspect of this proposal is our focus at the cellular level, and we are uniquely positioned to carry out our multidisciplinary aims involving biosensor engineering, innovative imaging, and multiscale modelling. We anticipate that the discoveries stemming from this project will provide the detailed understanding necessary to make strategic interventions into GA dynamic patterning in crop plants for specific improvements in growth, development, and environmental responses.

1 499 616 €

Start date: 2018-01-01, End date: 2022-12-31

"Magnetism plays a profound role in stars and planets. In the Sun, magnetic fields are ultimately responsible for solar flares and coronal mass ejections that can impact our technological society. Earth's own magnetic field partly shields us from these events, but solar storms can still interrupt satellite communications, disrupt power grids, and pose a danger to astronauts on spacewalks. More generally, magnetic fields partly control the rotational evolution of stars, likely impact the habitability of extrasolar planets, and may modify the sizes and internal structures of low-mass stars and gaseous planets. In all cases, the magnetism is generally thought to arise from a convective dynamo -- but a detailed theoretical understanding of this process, and its influence on the overall evolution of stars and planets, has remained elusive. Particularly fascinating observational puzzles have recently come from the study of low-mass M-dwarf stars: the most numerous type of stars in our galaxy and perhaps the most likely to host habitable planets. We therefore propose to study how stars and sub-stellar objects build magnetic fields using 3-D magnetohydrodynamic simulations, and to quantify the effects of those fields on stellar structure and evolution. Using the Anelastic Spherical Harmonic (ASH) and Compressible Spherical Segment (CSS) codes, we will examine (a) how global magnetic field generation in these stars depends upon parameters like stellar mass, rotation rate, and the presence of a stable core, and (b) how the deep convection and magnetism imprints through (and is shaped by) the near-surface layers of these objects. We will (c) determine the impact of the resulting fields on the convective transport of heat and angular momentum, incorporate our results into state of the art 1-D evolutionary models of stars, and explore the consequences for stellar evolution. Separately, we will (d) develop and maintain a public database of 3-D convective dynamo models."

1 469 070 €

Start date: 2013-12-01, End date: 2018-11-30

Eukaryotic cells inherit much of their genomic information in the form of chromosomes during cell division. Centimetre-long DNA molecules are packed into micrometer-sized chromosomes to enable this process. How DNA is organised within mitotic chromosomes is still largely unknown. A key structural protein component of mitotic chromosomes, implicated in their compaction, is the condensin complex. In this proposal, we aim to elucidate the molecular architecture of mitotic chromosomes, taking advantage of new genomic techniques and the relatively simple genome organisation of yeast model systems. We will place particular emphasis on elucidating the contribution of the condensin complex, and the cell cycle regulation of its activities, in promoting chromosome condensation. Our previous work has provided genome-wide maps of condensin binding to budding and fission yeast chromosomes. We will continue to decipher the molecular determinants for condensin binding. To investigate how condensin mediates DNA compaction, we propose to generate chromosome-wide DNA/DNA proximity maps. Our approach will be an extension of the chromosome conformation capture (3C) technique. High throughput sequencing of interaction points has provided a first glimpse of the interactions that govern chromosome condensation. The role that condensin plays in promoting these interactions will be investigated. The contribution of condensin s ATP-dependent activities, and cell cycle-dependent post-translational modifications, will be studied. This will be complemented by mathematical modelling of the condensation process. In addition to chromosome condensation, condensin is required for resolution of sister chromatids in anaphase. We will develop an assay to study the catenation status of sister chromatids and how condensin may contribute to their topological resolution.

2 076 126 €

Start date: 2010-04-01, End date: 2015-03-31

"The proposed research is intended to initiate the process of formulating an integrated approach to the evolution and spread of early Christianity in the Eastern Mediterranean, Caucasus and Middle East. Thus far this work has been constrained by geographical, linguistic and denominational boundaries meaning that there has been a plethora of regional studies in the field but no comprehensive overview attempting to develop a coherent picture of wider cultural interaction. By beginning a project that seeks to explore the relationship between the Syrian and Georgian Churches from a variety of different disciplines, this project intends to develop a framework from which to construct a comprehensive overview of the development of Eastern Christianity in late antiquity. This work will open a new phase in the study of late antique Christianity by seeking to place the different denominations that split apart after the Christological and Mariological controversies of the fifth century into a wider context that allows comparative study of their liturgical, architectural and theological development and interaction. It is logical to begin with the Syrian and Georgian traditions as the Georgians wrote in an Aramaic script, known as Armazi, until the evolution of the Georgian alphabet in the fifth century. Syriac, the liturgical language of the Syrian Church tradition, is also an Aramaic dialect that developed in the city of Edessa (now Şanliurfa in south-eastern Turkey). Edessa stood between Syria and Georgia and provided the main conduit for the transmission of culture between the two regions. In addition Georgia historically received monasticism and a renewed evangelical movement through the ""Thirteen Syrian Fathers"", thirteen Syrian monks who were credited with expanding on the work of evangelisation begun in Georgia by St Nino of Cappadocia in the fourth century. Beginning with these two inter-linked traditions this framework can be applied to other traditions in future."

954 523 €

Start date: 2012-11-01, End date: 2017-10-31