The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter ΛCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25σ. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations (σ 8 ) derived from CMB data and that derived from Sunyaev-Zeldovich data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak. Analysis of Planck polarization data is not yet mature, therefore polarization results are not released, although the robust detection of E-mode polarization around CMB hot and cold spots is shown graphically.
Saccharomyces cells suffering a DNA double-strand break (DSB) ultimately escape checkpoint-mediated G2/M arrest either by recovery once the lesion is repaired or by adaptation if the lesion proves irreparable. Cells lacking the PP2C-like phosphatases Ptc2 and Ptc3 are unable to adapt to a HO-induced DSB and are also defective in recovering from a repairable DSB. In contrast, overexpression of PTC2 rescues adaptation-defective yku80Delta and cdc5-ad mutants. These effects are not explained by alterations either in the processing of DSB ends or in DSB repair. In vivo and in vitro evidence suggests that phosphorylated forms of Ptc2 and Ptc3 specifically bind to the Rad53 FHA1 domain and inactivate Rad53-dependent pathways during adaptation and recovery by dephosphorylating Rad53.
IntroductionAerobic organisms are exposed to the toxicity of reactive oxygen species (ROS) produced during respiration, the boxidation of fatty acids, the exposure to radiation, light, metals and redox cycling drugs (Storz and Imlay, 1999). To protect against oxidative stress and to maintain a A. Exponential cell cultures grown in yeast extract peptone dextrose (YEPD) were diluted to OD 600 = 0.2 and 3 ml of three serial dilutions (10-fold) were patched on YEPD plates that contained H 2 O 2 at the indicated concentration. Plates were incubated at 30°C for 2 d and analysed. B. Wild-type and isogenic mutant strains cultures (as indicated) that were untreated or pretreated with H 2 O 2 (0.3 mM) were challenged during 2 h with H 2 O 2 at the indicated concentration, as described in Experimental procedures. The multicopy plasmid used for overexpression of PDE2 under its own promoter is pGR103 (Geymonat et al., 1998).
CAST (version 1.0) executable binaries are available to academic users free of charge under license. Web site entry point, server and additional material: http://www.ebi.ac.uk/research/cgg/services/cast/
The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity ( ΔT T ∼ 2 × 10 −6 ) and angular resolution (∼5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30−350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis.
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