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אוקטובר 01, 2009
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Date:19שלישייולי 2011הרצאה
Bak-Sneppen type models and rank-driven Markov processes
More information שעה 11:00 - 11:00מיקום Ziskind Bldg.מרצה Michael Grinfeld
University of Strathclydeמארגן הפקולטה למתמטיקה ומדעי המחשב -
Date:19שלישייולי 2011הרצאה
"The TPP Riboswitch Acts as a Pacesetter to Orchestrate Central Metabolism in Thiamin Autotrophs"
More information שעה 11:15 - 11:15מיקום בניין אולמן למדעי החייםמרצה Dr. Samuel Bocobza
Dr. Asaph Aharoni's lab - Department of Plant Sciences, WISמארגן המחלקה למדעי הצמח והסביבהצרו קשר -
Date:19שלישייולי 2011הרצאה
New vistas on the role of the rodent dopaminergic system in learning and memory
More information שעה 12:30 - 12:30מיקום בניין יעקב זיסקינדמרצה Prof. Jean-Marc Fellous
University of Arizona, Tucsonמארגן המחלקה למדעי המוחצרו קשר תקציר Show full text abstract about Computational and experimental studies of learning and memor...» Computational and experimental studies of learning and memory have traditionally focused on the role of cognitive brain areas such as the cortex and hippocampus. This work has provided invaluable insights in the ways items are learned, stored and consolidated using a variety of neural mechanisms from molecular to network levels. Relatively little has however been done on understanding how and why some items are selected to be memorized while others are not. I will present a set of experimental results in the rodent showing that the dopaminergic neurons of the rodent ventral tegmental area are actively involved in the acquisition and consolidation of positively and negatively valued memories. The experiments will include optimal spatial navigation, memory reactivation and a rodent model of post-traumatic stress disorder. This ongoing work suggests that neuromodulatory centers may have a much more active and selective role in learning and memory than previously thought. -
Date:19שלישייולי 2011הרצאה
"Apoptotic Inducers in Macrophages and DCs: The story behind apoptosis "
More information שעה 13:30 - 13:30מיקום בניין וולפסון למחקר ביולוגימרצה Dr. Harris Perlman
Northwestern University Feinberg School of Medicine Division of Rheumatology Department of Medicineמארגן המחלקה לאימונולוגיה מערכתיתצרו קשר -
Date:20רביעייולי 2011הרצאה
Individualized treatment on multiple sclerosis
More information שעה 12:30 - 12:30מיקום בניין יעקב זיסקינדמרצה Prof. Giancarlo Comi
Department of Neurology Vita-Salute San Raffaele University and Scientific Institute, Milanמארגן המחלקה למדעי המוחצרו קשר -
Date:20רביעייולי 2011אירועי תרבות
"בית אל ג'ירן - שכנים"
More information שעה 20:30 - 20:30כותרת קומדיה בשפה העיראקיתמיקום אודיטוריום מיכאל סלעצרו קשר -
Date:21חמישייולי 2011הרצאה
Geometry of the random interlacement
More information שעה 11:00 - 11:00מיקום Ziskind Bldg.מרצה Eviatar Procaccia
WISמארגן הפקולטה למתמטיקה ומדעי המחשב -
Date:21חמישייולי 2011הרצאה
Presenting TIGM: The largest collection of mutant mouse ES cell resources for the scientific community
More information שעה 14:00 - 14:00מיקום בניין ארתור ורושל בלפר למחקר ביורפואימרצה Dr. Ben Morpurgo
Director, TIGM Business and Operations, Texas A&M Institute for Genomic Medicine, Texas, USAמארגן המחלקה לגנטיקה מולקולריתצרו קשר -
Date:21חמישייולי 2011הרצאה
Some connections between almost periodic and periodic discrete Schroedinger operators with analytic potentials
More information שעה 15:00 - 15:00מיקום Ziskind Bldg.מרצה Mira Shamis
Institute for Advanced Studyמארגן הפקולטה למתמטיקה ומדעי המחשב -
Date:24ראשוןיולי 2011הרצאה
<a href="http://adsabs.harvard.edu/abs/2011arXiv1107.1477M">Herschel Detects a Massive Dust Reservoir in Supernova 1987A</a>
More information שעה 12:30 - 14:00מיקום מעבדה על-שם דני נ. היינמןמרצה Dong Xu מארגן מרכז לאסטרופיסיקה עש נלה וליאון בנוזיוצרו קשר תקציר Show full text abstract about We report far-infrared and submillimeter observations of Sup...» We report far-infrared and submillimeter observations of Supernova 1987A, the star that exploded on February 23, 1987 in the Large Magellanic Cloud, a galaxy located 160,000 lightyears away. The observations reveal the presence of a population of cold dust grains radiating with a temperature of ~17-23 K at a rate of about 220 solar luminosity. The intensity and spectral energy distribution of the emission suggests a dust mass of ~0.4-0.7 solar mass. The radiation must originate from the SN ejecta and requires the efficient precipitation of all refractory material into dust. Our observations imply that supernovae can produce the large dust masses detected in young galaxies at very high redshifts. -
Date:25שנייולי 2011הרצאה
"Molecular Origami: protein folding and misfolding in health and disease"
More information שעה 11:00 - 12:00מיקום בניין הלן ומילטון קימלמןמרצה Prof Judith Frydman
Dept. of Biology Stanford University ,USAמארגן המחלקה לביולוגיה מבנית וכימיתצרו קשר -
Date:25שנייולי 2011הרצאה
An Integrative approach to uncover drivers of cancer
More information שעה 14:00 - 14:00מיקום בניין ע"ש מקס ולילאן קנדיוטימרצה Dr.Dana Peer
Assistant Professor Dept. of Biological Sciences Columbia University NY USAמארגן המחלקה לאימונולוגיה ורגנרציה ביולוגיתצרו קשר -
Date:25שנייולי 2011הרצאה
Determining the stability of genetic switches:
More information שעה 14:15 - 14:15מיקום בניין הפיזיקה ע"ש עדנה וק.ב. וייסמןמרצה Michael Assaf
University of Illinois, Urbanaמארגן המחלקה לפיזיקה של מערכות מורכבותצרו קשר תקציר Show full text abstract about Cells use genetic switches to shift between alternate gene e...» Cells use genetic switches to shift between alternate gene expression states, e.g. to adapt to new environments or to follow a developmental
pathway. Here, we study the dynamics of switching in a generic-feedback
on/off switch. Unlike protein-only models, we explicitly account for stochastic fluctuations of mRNA, which have a dramatic impact on switch dynamics. Employing a semi-classical theory to treat the underlying chemical master equations, we obtain accurate results for the quasi-stationary distributions of mRNA and protein copy numbers and for the mean switching time, starting from either state. Our analytical results agree well with extensive Monte Carlo simulations. Importantly, one can use the approach to study the effect of varying biological parameters on the switch stability.
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Date:25שנייולי 2011אירועי תרבות
"האריה שאהב תות" - תאטרון ילדים
More information שעה 17:30 - 17:30מיקום אודיטוריום מיכאל סלעצרו קשר -
Date:26שלישייולי 2011הרצאה
"Dynamic Proteomics of human cancer cells as they respond to drugs"
More information שעה 11:15 - 11:15מיקום בניין אולמן למדעי החייםמרצה Dr. Naama Geva Zatorsky
Department of Molecular Cell Biology Weizmann Institute of Scienceמארגן המחלקה למדעי הצמח והסביבהצרו קשר -
Date:26שלישייולי 2011הרצאה
Induction of tolerance to BM allografts by central memory CD8+ T cells
More information שעה 13:30 - 13:30מיקום בניין וולפסון למחקר ביולוגימרצה Eran Ophir
Ph.D. Student in the laboratory of Prof. Yair Reisnerמארגן המחלקה לאימונולוגיה מערכתיתצרו קשר -
Date:27רביעייולי 2011הרצאה
"Universal Strain - Temperature Dependence of Dislocation Structures in Deformed FCC Metals"
More information שעה 11:00 - 11:00מיקום בניין פרלמן למדעי הכימיהמרצה Dr. Peri Landau
Department of Physics, Ben Gurion Universityמארגן המחלקה לכימיה מולקולרית ולמדע חומריםצרו קשר תקציר Show full text abstract about This research is aimed to understanding plastic deformation ...» This research is aimed to understanding plastic deformation mechanisms through the systematic analysis of the microstructure and dislocation patterns in deformed metals, mainly by electron microscopy techniques. Dislocation dynamics and microstructural evolution under applied stresses by means of in-situ experiments in the transmission electron microscope was performed in order to explore the mechanism of dislocation pattern formation.
The combined effect of strain and temperature on the microstructural evolution of plastically deformed fcc metals (Aluminum, Copper, Nickel and Gold) was examined systematically. In particular, the detailed nano-scale, internal structure of dislocation boundaries was determined. In all the metals studied, dislocations within the boundaries tend to rearrange themselves sequentially with increasing strain from tangles into dislocation cells with tangled boundaries, followed by the formation of dislocation boundaries consisting of wavy, parallel dislocations and finally into arrays of parallel dislocations. The results were represented by strain-temperature microstructural maps. The topology of the microstructural maps was found to be similar for all metals studied, suggesting a universal strain- temperature dependence in deformed fcc metals.
The experimental strain-temperature maps of dislocation structures at the nano-scale for the studied fcc metals are scaled by the cross-slip activation energy, calculated using an atomistic based elastic model, to form a single universal strain - temperature map. Such a map unifies many observations obtained by different groups over the years and serves to direct further investigations in this fundamental area. These implications for dislocation rearrangement mechanisms are discussed.
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Date:28חמישייולי 2011אירועי תרבות
תערוכת היופי שבמדע
More information שעה 15:00 - 17:00כותרת אירוע פתיחהמיקום המשכן ללימודי מוסמכים על-שם דוד לופאטימארגן בית הספר למחקר - מכון ויצמן למדעדף בית צרו קשר -
Date:28חמישייולי 2011אירועי תרבות
קובי מימון במופע סטנד אפ
More information שעה 21:00 - 21:00מיקום אודיטוריום מיכאל סלעצרו קשר -
Date:31ראשוןיולי 2011הרצאה
A luminous quasar at a redshift of z = 7.085
More information שעה 12:30 - 14:00כותרת <a href="http://adsabs.harvard.edu/abs/2011Natur.474..616M">http://adsabs.harvard.edu/abs/2011Natur.474..616M</a>מיקום מעבדה על-שם דני נ. היינמןמרצה Adam Becker מארגן מרכז לאסטרופיסיקה עש נלה וליאון בנוזיוצרו קשר תקציר Show full text abstract about The intergalactic medium was not completely reionized until ...» The intergalactic medium was not completely reionized until approximately a billion years after the Big Bang, as revealed by observations of quasars with redshifts of less than 6.5. It has been difficult to probe to higher redshifts, however, because quasars have historically been identified in optical surveys, which are insensitive to sources at redshifts exceeding 6.5. Here we report observations of a quasar (ULASJ112001.48+064124.3) at a redshift of 7.085, which is 0.77 billion years after the Big Bang. ULASJ1120+0641 has a luminosity of 6.3×1013Lsolar and hosts a black hole with a mass of 2×109Msolar (where Lsolar and Msolar are the luminosity and mass of the Sun). The measured radius of the ionized near zone around ULASJ1120+0641 is 1.9megaparsecs, a factor of three smaller than is typical for quasars at redshifts between 6.0 and 6.4. The near-zone transmission profile is consistent with a Lyα damping wing, suggesting that the neutral fraction of the intergalactic medium in front of ULASJ1120+0641 exceeded 0.1.
