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January 01-31, 2017

  • Date:05ThursdayJanuary 2017

    Gamma-ray astronomy - observing the extreme places in the Universe

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    Time
    11:15 - 12:30
    Location
    Edna and K.B. Weissman Building of Physical Sciences
    LecturerChristian Stegmann
    DESY
    Organizer
    Faculty of Physics
    Contact
    AbstractShow 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.

    Colloquia
  • Date:05ThursdayJanuary 2017

    Immunology Departmental Student Seminar

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    Time
    14:00 - 15:00
    Location
    Wolfson Building for Biological Research
    LecturerAdi Sharbi Yunger & Masha Kolesnikov
    Organizer
    Department of Systems Immunology
    Contact
    Lecture
  • Date:05ThursdayJanuary 2017

    Shirat Hamada

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    Time
    19:30 - 21:30
    Location
    Michael Sela Auditorium
    Contact
    Lecture
  • Date:08SundayJanuary 2017

    New CRISPR-Cas systems from uncultivated microbes

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    Time
    09:00 - 09:00
    Location
    Arthur and Rochelle Belfer Building for Biomedical Research
    LecturerDr. David Burstein
    Department of Earth and Planetary Sciences, University of California, Berkeley
    Organizer
    Department of Molecular Genetics
    Contact
    Lecture
  • Date:08SundayJanuary 2017

    The Snowball Bifurcation on Exoplanets

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    Time
    11:00 - 11:00
    Location
    Sussman Family Building for Environmental Sciences
    LecturerDr. Dorian Abbot
    Department of the Geophysical Sciences The University of Chicago
    Organizer
    Department of Earth and Planetary Sciences
    Contact
    AbstractShow 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.

    Lecture
  • Date:08SundayJanuary 2017

    Protein and Cell Therapeutics using Polymeric Hydrogel Carriers

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    Time
    11:00 - 12:00
    Location
    Perlman Chemical Sciences Building
    LecturerProf. Dror Seliktar
    Faculty of Biomedical Engineering, Technion
    Organizer
    Department of Molecular Chemistry and Materials Science
    Contact
    Lecture
  • Date:08SundayJanuary 2017

    GeneHancer: genome-wide integration of enhancers and target genes in GeneCards

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    Time
    13:00 - 13:00
    Location
    Arthur and Rochelle Belfer Building for Biomedical Research
    LecturerDr. Simon Fishilevich
    Doron Lancet's group, Dept. of Molecular Genetics, WIS
    Organizer
    Department of Molecular Genetics
    Contact
    Lecture
  • Date:08SundayJanuary 2017

    Acute and long term response to bariatric surgery

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    Time
    15:00 - 16:00
    Location
    Arthur and Rochelle Belfer Building for Biomedical Research
    LecturerDr. Danny Ben-Zvi
    Contact
    Lecture
  • Date:09MondayJanuary 2017

    "Application of novel in vitro single-molecule approaches to the studies of chromatin, replication, and transcription"

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    Time
    11:00 - 12:15
    Location
    Gerhard M.J. Schmidt Lecture Hall
    LecturerProf. Nynke Dekker
    Kavli Institute of Nanoscience, TU Delft
    Organizer
    Faculty of Chemistry
    Contact
    AbstractShow 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
    Colloquia
  • Date:09MondayJanuary 2017

    Heterogeneity landscapes of breast cancer- communities of clones and communities of cells

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    Time
    14:00 - 14:00
    Title
    Cancer Research Club
    Location
    Max and Lillian Candiotty Building
    LecturerProf. Carlos Caldas
    UK Cambridge Research Institute Director, Cambridge Breast Cancer Research Unit,UK
    Organizer
    Department of Immunology and Regenerative Biology
    Contact
    AbstractShow 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.
    Lecture
  • Date:09MondayJanuary 2017

    Kidnapped - Tragic Yeman story

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    Time
    20:30 - 20:30
    Location
    Michael Sela Auditorium
    Contact
    Cultural Events
  • Date:10TuesdayJanuary 2017

    Faculty Day - Chemistry

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    Time
    08:30 - 17:00
    Location
    Gerhard M.J. Schmidt Lecture Hall
    Lecturerall Senior Scientists
    Organizer
    Faculty of Chemistry
    Contact
    Lecture
  • Date:10TuesdayJanuary 2017

    Cardiolipin - mitochondrial phospholipid at the epicenter of energy metabolism

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    Time
    10:00 - 11:00
    Location
    Wolfson Building for Biological Research
    LecturerProf. Miriam-Leba Greenberg
    Department of Biological Sciences, Wayne State Univ., Detroit, MI, USA
    Organizer
    Department of Biomolecular Sciences
    Contact
    AbstractShow 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.
    Lecture
  • Date:11WednesdayJanuary 2017

    "High precision flavor sum rules"

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    Time
    11:00 - 11:00
    Location
    Weismann Aquarium
    LecturerProf Yuval Grossman
    cornell
    Organizer
    Department of Particle Physics and Astrophysics
    Contact
    Lecture
  • Date:11WednesdayJanuary 2017

    "The Top quark as a window for new physics at the LHC".

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    Time
    13:00 - 13:00
    Location
    Weismann Aquarium
    LecturerDr. Ofir Gabizon
    Technion
    Organizer
    Department of Particle Physics and Astrophysics
    Contact
    Lecture
  • Date:11WednesdayJanuary 2017

    Special seminar Prof. Aprahamian Ivan

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    Time
    14:00 - 14:00
    Title
    “Hydrazone-Based Functional Materials”
    Location
    Helen and Milton A. Kimmelman Building
    Organizer
    Department of Molecular Chemistry and Materials Science
    Contact
    Lecture
  • Date:12ThursdayJanuary 2017

    Magnetic Resonance Seminar

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    Time
    09:30 - 09:30
    Title
    NMR Characterization of CO2 Adsorbtion on 3-Aminopropylsilyl-modified SBA15 Mesoporous Silica
    Location
    Gerhard M.J. Schmidt Lecture Hall
    LecturerDr. Daphna Shimon
    Department of Chemistry Washington University in St. Louis
    Organizer
    Department of Chemical and Biological Physics
    Contact
    Lecture
  • Date:12ThursdayJanuary 2017

    Bacterial Farming of Microalgae - An Interdisciplinary View

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    Time
    10:30 - 10:30
    Location
    Ullmann Building of Life Sciences
    LecturerDr. Einat Segev
    Organizer
    Department of Plant and Environmental Sciences
    Contact
    Lecture
  • Date:12ThursdayJanuary 2017

    Hot gas in clusters of galaxies, cosmic microwave background radiation and cosmology

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    Time
    11:15 - 12:30
    Location
    Edna and K.B. Weissman Building of Physical Sciences
    LecturerRashid Sunyaev
    MPI
    Organizer
    Faculty of Physics
    Contact
    AbstractShow 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.
    Colloquia
  • Date:12ThursdayJanuary 2017

    Pelletron meeting - by invitation only

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    Time
    16:00 - 17:45
    Contact
    Lecture

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