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January 01-31, 2017
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Date:05ThursdayJanuary 2017Colloquia
Gamma-ray astronomy - observing the extreme places in the Universe
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer Christian Stegmann
DESYOrganizer Faculty of PhysicsContact Abstract Show full text abstract about Astronomy with gamma rays at energies above some 10 GeV has ...» Astronomy with gamma rays at energies above some 10 GeV has opened in the last decade a new window to the cosmos. Gamma rays allows us to take a look at the extreme places in our Universe. They are produced in Supernova remains, Black holes and active galaxies - cosmic particle accelerators, in which atomic nuclei and electrons are accelerated to vast energies.
Contrary to expectations high-energy phenomena are no exception in the cosmos, but occur in many galactic and extragalactic objects during their life cycle. There are currently over 2000 sources of GeV radiation and over 150 sources of TeV radiation. Thus the results of gamma astronomy are an important building block to the understanding of the development of the Milky Way and our Universe.
So far, gamma-ray astronomy in the TeV range, however, is performed with experiments that are only accessible to a limited circle of users.
With the Cherenkov Telescope Array CTA an international consortium of more than 1000 scientists and engineers aims for an open observatory.
Starting from the current findings of gamma-ray astronomy I will in the presentation date to look into the future to what we will be able to learn with CTA.
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Date:05ThursdayJanuary 2017Lecture
Immunology Departmental Student Seminar
More information Time 14:00 - 15:00Location Wolfson Building for Biological ResearchLecturer Adi Sharbi Yunger & Masha Kolesnikov Organizer Department of Systems ImmunologyContact -
Date:05ThursdayJanuary 2017Lecture
Shirat Hamada
More information Time 19:30 - 21:30Location Michael Sela AuditoriumContact -
Date:08SundayJanuary 2017Lecture
New CRISPR-Cas systems from uncultivated microbes
More information Time 09:00 - 09:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Dr. David Burstein
Department of Earth and Planetary Sciences, University of California, BerkeleyOrganizer Department of Molecular GeneticsContact -
Date:08SundayJanuary 2017Lecture
The Snowball Bifurcation on Exoplanets
More information Time 11:00 - 11:00Location Sussman Family Building for Environmental SciencesLecturer Dr. Dorian Abbot
Department of the Geophysical Sciences The University of ChicagoOrganizer Department of Earth and Planetary SciencesContact Abstract Show full text abstract about The Snowball Earth episodes may have affected the developmen...» The Snowball Earth episodes may have affected the development of life on Earth through increasing atmospheric oxygen and spurring evolution. Considering the habitability and increase in complexity of life on other planets therefore requires thought about Snowball climate states. Using an energy balance model and global climate model, I will show that it is unlikely a tidally locked planet could experience a Snowball Earth bifurcation. Instead the planet would smoothly transition to global ice coverage. This is due to the difference in the shape of the insolation, which increases strongly toward the substellar point on a tidally locked planet. I will then change focus slightly and explain how climate oscillations between a warm state and a Snowball state can occur on a planet within the habitable zone that has a small CO2 outgassing rate. I will develop analytical relations to understand these cycles and outline scalings in variables such as the cycle period as a function of important climatic and weathering parameters. Work of this type should help us understand the context of planetary habitability and focus on appropriate targets as we seek to find the first inhabited exoplanet.
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Date:08SundayJanuary 2017Lecture
Protein and Cell Therapeutics using Polymeric Hydrogel Carriers
More information Time 11:00 - 12:00Location Perlman Chemical Sciences BuildingLecturer Prof. Dror Seliktar
Faculty of Biomedical Engineering, TechnionOrganizer Department of Molecular Chemistry and Materials ScienceContact -
Date:08SundayJanuary 2017Lecture
GeneHancer: genome-wide integration of enhancers and target genes in GeneCards
More information Time 13:00 - 13:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Dr. Simon Fishilevich
Doron Lancet's group, Dept. of Molecular Genetics, WISOrganizer Department of Molecular GeneticsContact -
Date:08SundayJanuary 2017Lecture
Acute and long term response to bariatric surgery
More information Time 15:00 - 16:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Dr. Danny Ben-Zvi Contact -
Date:09MondayJanuary 2017Colloquia
"Application of novel in vitro single-molecule approaches to the studies of chromatin, replication, and transcription"
More information Time 11:00 - 12:15Location Gerhard M.J. Schmidt Lecture HallLecturer Prof. Nynke Dekker
Kavli Institute of Nanoscience, TU DelftOrganizer Faculty of ChemistryContact Abstract Show full text abstract about Over the past few decades, there has been steady progress in...» Over the past few decades, there has been steady progress in both our ability to produce biological material and in our ability to manipute matter at small length scales. These two developments merge in a fascinating area of confluence called single-molecule biophysics in which an understanding of biological matter from physical principles becomes possible. I will illustrate the development of this interdisciplinary field and show how several newly-developed techniques allow us to shed light on genomic processes such as DNA compaction, replication, and transcription.
For example, by measuring the twist and length of single DNA molecules, we are able to learn about DNA compaction into chromatin. We monitor the real-time loading of tetramers or complete histone octamers onto DNA and find, remarkably, that tetrasomes exhibit spontaneous flipping between a preferentially occupied left-handed state and a right-handed state, separated by free energy difference of 2.3 kBT (1.5 kcal/mol). The application of weak positive torque converts left-handed tetrasomes into right-handed tetrasomes, whereas nucleosomes display more gradual conformational changes. These findings reveal unexpected dynamical rearrangements of the nucleosomal structure, suggesting that chromatin can serve as a ‘‘twist reservoir,’’ offering a mechanistic explanation for the regulation of DNA supercoiling in chromatin.
By making use of high-throughput single-molecule techniques, we are able to gain new insights into the termination of DNA replication. In Escherichia coli, replisome progression beyond the termination site is prevented by Tus proteins bound to asymmetric Ter sites. Structural evidence indicates that strand separation on the blocking (non-permissive) side of Tus–Ter triggers roadblock formation, but biochemical evidence also suggests roles for protein- protein interactions. We perform DNA unzipping experiments which demonstrate that nonpermissively oriented Tus–Ter forms a tight lock in the absence of replicative proteins, whereas permissively oriented Tus–Ter allows nearly unhindered strand separation. Quantifying the lock strength reveals the existence of several intermediate lock states that are impacted by mutations in the lock domain but not by mutations in the DNA-binding domain. Lock formation is highly specific and exceeds reported in vivo efficiencies. We therefore postulate that protein-protein interactions may actually hinder, rather than promote, proper lock formation.
I will conclude by describing how such types of biophysical measurements should complement biochemical investigations in the coming few years -
Date:09MondayJanuary 2017Lecture
Heterogeneity landscapes of breast cancer- communities of clones and communities of cells
More information Time 14:00 - 14:00Title Cancer Research ClubLocation Max and Lillian Candiotty BuildingLecturer Prof. Carlos Caldas
UK Cambridge Research Institute Director, Cambridge Breast Cancer Research Unit,UKOrganizer Department of Immunology and Regenerative BiologyContact Abstract Show full text abstract about We redefined the molecular taxonomy of breast cancer identif...» We redefined the molecular taxonomy of breast cancer identifying the genomic driver-based subtypes. We have recently shown these subtypes have prototypical clonal and TME architectures. These observations have profound biological and clinical implications which we are now exploring. These include insights into clonal evolution and cancer-immune system interactions. -
Date:09MondayJanuary 2017Cultural Events
Kidnapped - Tragic Yeman story
More information Time 20:30 - 20:30Location Michael Sela AuditoriumContact -
Date:10TuesdayJanuary 2017Lecture
Faculty Day - Chemistry
More information Time 08:30 - 17:00Location Gerhard M.J. Schmidt Lecture HallLecturer all Senior Scientists Organizer Faculty of ChemistryContact -
Date:10TuesdayJanuary 2017Lecture
Cardiolipin - mitochondrial phospholipid at the epicenter of energy metabolism
More information Time 10:00 - 11:00Location Wolfson Building for Biological ResearchLecturer Prof. Miriam-Leba Greenberg
Department of Biological Sciences, Wayne State Univ., Detroit, MI, USAOrganizer Department of Biomolecular SciencesContact Abstract Show full text abstract about The proteins that mediate the three pillars of energy metabo...» The proteins that mediate the three pillars of energy metabolism – synthesis of acetyl CoA, oxidation of acetyl CoA via the TCA cycle to generate NADH, and utilization of NADH by the electron transport chain to generate ATP – have long been the focus of investigation. In contrast, much less is known about the role of lipids in the production of energy. Recent studies show that cardiolipin, the signature lipid of the mitochondrial membrane, plays a key role in all three pathways of energy metabolism. This knowledge is expected to provide insight into the mechanisms underlying cardiomyopathy in Barth syndrome, a life-threatening genetic disorder of cardiolipin metabolism. -
Date:11WednesdayJanuary 2017Lecture
"High precision flavor sum rules"
More information Time 11:00 - 11:00Location Weismann AquariumLecturer Prof Yuval Grossman
cornellOrganizer Department of Particle Physics and AstrophysicsContact -
Date:11WednesdayJanuary 2017Lecture
"The Top quark as a window for new physics at the LHC".
More information Time 13:00 - 13:00Location Weismann AquariumLecturer Dr. Ofir Gabizon
TechnionOrganizer Department of Particle Physics and AstrophysicsContact -
Date:11WednesdayJanuary 2017Lecture
Special seminar Prof. Aprahamian Ivan
More information Time 14:00 - 14:00Title “Hydrazone-Based Functional Materials”Location Helen and Milton A. Kimmelman BuildingOrganizer Department of Molecular Chemistry and Materials ScienceContact -
Date:12ThursdayJanuary 2017Lecture
Magnetic Resonance Seminar
More information Time 09:30 - 09:30Title NMR Characterization of CO2 Adsorbtion on 3-Aminopropylsilyl-modified SBA15 Mesoporous SilicaLocation Gerhard M.J. Schmidt Lecture HallLecturer Dr. Daphna Shimon
Department of Chemistry Washington University in St. LouisOrganizer Department of Chemical and Biological PhysicsContact -
Date:12ThursdayJanuary 2017Lecture
Bacterial Farming of Microalgae - An Interdisciplinary View
More information Time 10:30 - 10:30Location Ullmann Building of Life SciencesLecturer Dr. Einat Segev Organizer Department of Plant and Environmental SciencesContact -
Date:12ThursdayJanuary 2017Colloquia
Hot gas in clusters of galaxies, cosmic microwave background radiation and cosmology
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer Rashid Sunyaev
MPIOrganizer Faculty of PhysicsContact Abstract Show full text abstract about Presence of the hot (kTe ~ 3 - 10 KeV) rarefied gas in the c...» Presence of the hot (kTe ~ 3 - 10 KeV) rarefied gas in the clusters of galaxies (most massive gravitationally bound objects in the Universe) leads to the appearance of "shadows" in the angular distribution of the Cosmic Microwave Background (CMB) Radiation and permits to measure the peculiar velocities of these clusters relative to the unique coordinate frame where CMB is isotropic. I plan to describe the physics leading to these observational effects. Planck spacecraft, ground based South Pole and Atacama Cosmology Telescopes discovered recently more than thousand of unknown before Clusters of Galaxies at high redshifts detecting these "shadows" and traces of kinematic effect, demonstrating the correlation of the hot gas velocities with mass concentrations on large scales. Giant ALMA submillimeter interferometer in Atacama desert resolved recently strong shocks between merging clusters of galaxies.
Newly discovered clusters of galaxies permit to study the rate of growth of the large scale structure of the Universe and open an independent way to measure key cosmological parameters of our Universe.
I plan to mention Russian - German Spectrum-X/eRosita space mission under preparation for the launch in the March of 2018. This mission will be able to detect all (hundred thousand !) rich clusters of galaxies in the observable Universe and up to 3 millions of accreting supermassive black holes (in Active Galactic Nuclei) during 4 year long X-Ray sky survey. S3 and S4 ground based CMB research programs promise to reach similar or even higher sensitivities and detect up to a million of clusters and groups of galaxies containing hot gas.
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Date:12ThursdayJanuary 2017Lecture
Pelletron meeting - by invitation only
More information Time 16:00 - 17:45Contact