Single-Molecule Analysis Reveals the Kinetics and Physiological Relevance of MutL-ssDNA Binding

DNA binding by MutL homologs (MLH/PMS) during mismatch repair (MMR) has been considered based on biochemical and genetic studies. Bulk studies with MutL and its yeast homologs Mlh1-Pms1 have suggested an integral role for a single-stranded DNA (ssDNA) binding activity during MMR. We have developed single-molecule Förster resonance energy transfer (smFRET) and a single-molecule DNA flow-extension assays to examine MutL interaction with ssDNA in real time. The smFRET assay allowed us to observe MutL-ssDNA association and dissociation. We determined that MutL-ssDNA binding required ATP and was the greatest at ionic strength below 25 mM (KD = 29 nM) while it dramatically decreases above 100 mM (KD>2 µM). Single-molecule DNA flow-extension analysis suggests that multiple MutL proteins may bind ssDNA at low ionic strength but this activity does not enhance stability at elevated ionic strengths. These studies are consistent with the conclusion that a stable MutL-ssDNA interaction is unlikely to occur at physiological salt eliminating a number of MMR models. However, the activity may infer some related dynamic DNA transaction process during MMR

Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy

Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray astronomy has a huge potential in astrophysics, particle physics and cosmology. CTA is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100 GeV and above 100 TeV. CTA will consist of two arrays (one in the north, one in the south) for full sky coverage and will be operated as open observatory. The design of CTA is based on currently available technology. This document reports on the status and presents the major design concepts of CTA

Cosmic ray oriented performance studies for the JEM-EUSO first level trigger

JEM-EUSO is a space mission designed to investigate Ultra-High Energy Cosmic Rays and Neutrinos (E > 5 ⋅ 1019 eV) from the International Space Station (ISS). Looking down from above its wide angle telescope is able to observe their air showers and collect such data from a very wide area. Highly specific trigger algorithms are needed to drastically reduce the data load in the presence of both atmospheric and human activity related background light, yet retain the rare cosmic ray events recorded in the telescope. We report the performance in offline testing of the first level trigger algorithm on data from JEM-EUSO prototypes and laboratory measurements observing different light sources: data taken during a high altitude balloon flight over Canada, laser pulses observed from the ground traversing the real atmosphere, and model landscapes reproducing realistic aspect ratios and light conditions as would be seen from the ISS itself. The first level trigger logic successfully kept the trigger rate within the permissible bounds when challenged with artificially produced as well as naturally encountered night sky background fluctuations and while retaining events with general air-shower characteristics

Calorimetric analysis of binding of two consecutive DNA strands to RecA protein illuminates mechanism for recognition of homology

RecA protein recognises two complementary DNA strands for homologous recombination. To gain insight into the molecular mechanism, the thermodynamic parameters of the DNA binding have been characterised by isothermal calorimetry. Specifically, conformational changes of protein and DNA were searched for by measuring variations in enthalpy change, (Delta H) with temperature (heat capacity change, Delta C-p). In the presence of the ATP analogue ATP gamma S, the Delta H for the binding of the first DNA strand depends upon temperature (large Delta C-p) and the type of buffer, in a way that is consistent with the organisation of disordered parts and the protonation of RecA upon complex formation. In contrast, the binding of the second DNA strand occurs without any pronounced Delta C-p, indicating the absence of further reorganisation of the RecA-DNA filament. In agreement with these findings, a significant change in the CD spectrum of RecA was observed only upon the binding of the first DNA strand. In the absence of nucleotide cofactor, the Delta H of DNA binding is almost independent of temperature, indicating a requirement for ATP in the reorganisation of RecA. When the second DNA strand is complementary to the first, the Delta H is larger than that for non-complementary DNA strand, but less than the Delta H of the annealing of the complementary DNA without RecA. This small Delta H could reflect a weak binding that may facilitate the dissociation of only partly complementary DNA and thus speed the search for complementary DNA. The Delta H of binding DNA sequences displaying strong base-base stacking is small for both the first and second binding DNA strand, suggesting that the second is also stretched upon interaction with RecA. These results support the proposal that the RecA protein restructures DNA, preparing it for the recognition of a complementary second DNA strand, and that the recognition is due mainly to direct base-base contacts between DNA strands. (c) 2006 Elsevier Ltd. All rights reserved

Calorimetric analysis of binding of two consecutive DNA strands to RecA protein illuminates mechanism for recognition of homology

RecA protein recognises two complementary DNA strands for homologous recombination. To gain insight into the molecular mechanism, the thermodynamic parameters of the DNA binding have been characterised by isothermal calorimetry. Specifically, conformational changes of protein and DNA were searched for by measuring variations in enthalpy change, (Delta H) with temperature (heat capacity change, Delta C-p). In the presence of the ATP analogue ATP gamma S, the Delta H for the binding of the first DNA strand depends upon temperature (large Delta C-p) and the type of buffer, in a way that is consistent with the organisation of disordered parts and the protonation of RecA upon complex formation. In contrast, the binding of the second DNA strand occurs without any pronounced Delta C-p, indicating the absence of further reorganisation of the RecA-DNA filament. In agreement with these findings, a significant change in the CD spectrum of RecA was observed only upon the binding of the first DNA strand. In the absence of nucleotide cofactor, the Delta H of DNA binding is almost independent of temperature, indicating a requirement for ATP in the reorganisation of RecA. When the second DNA strand is complementary to the first, the Delta H is larger than that for non-complementary DNA strand, but less than the Delta H of the annealing of the complementary DNA without RecA. This small Delta H could reflect a weak binding that may facilitate the dissociation of only partly complementary DNA and thus speed the search for complementary DNA. The Delta H of binding DNA sequences displaying strong base-base stacking is small for both the first and second binding DNA strand, suggesting that the second is also stretched upon interaction with RecA. These results support the proposal that the RecA protein restructures DNA, preparing it for the recognition of a complementary second DNA strand, and that the recognition is due mainly to direct base-base contacts between DNA strands. (c) 2006 Elsevier Ltd. All rights reserved