0000000000787960

AUTHOR

C. Blumer

showing 2 related works from this author

LrhA as a new transcriptional key regulator of flagella, motility and chemotaxis genes in Escherichia coli

2002

The function of the LysR-type regulator LrhA of Escherichia coli was defined by comparing whole-genome mRNA profiles from wild-type E. coli and an isogenic lrhA mutant on a DNA microarray. In the lrhA mutant, a large number (48) of genes involved in flagellation, motility and chemotaxis showed relative mRNA abundances increased by factors between 3 and 80. When a representative set of five flagellar, motility and chemotaxis genes was tested in lacZ reporter gene fusions, similar factors for derepression were found in the lrhA mutant. In gel retardation experiments, the LrhA protein bound specifically to flhD and lrhA promoter DNA (apparent K-D approximate to 20 nM), whereas the promoters of…

DNA BacterialbindingTranscription GeneticRecombinant Fusion ProteinsMolecular Sequence DataMutantacetyl phosphatelac operonBiologymedicine.disease_causeMicrobiologyh-ns proteink-12lysr homologBacterial ProteinsGenes ReporterTranscription (biology)expressionEscherichia colimedicinernaRNA MessengerPromoter Regions GeneticMolecular BiologyGeneEscherichia coliDerepressionOligonucleotide Array Sequence AnalysisBase SequenceChemotaxisEscherichia coli ProteinsGene Expression ProfilingPromoterChemotaxisGene Expression Regulation BacterialMolecular biologyco2 fixationmaster operonDNA-Binding ProteinsRNA BacterialLac OperonFlagellaTrans-ActivatorssignalTranscription Factors
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The rapid atmospheric monitoring system of the Pierre Auger Observatory

2012

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 1017 eV. During clear nights with a low illuminated moon fraction, the UV fluorescence light produced by air showers is recorded by optical telescopes at the Observatory. To correct the observations for variations in atmospheric conditions, atmospheric monitoring is performed at regular intervals ranging from several minutes (for cloud identification) to several hours (for aerosol conditions) to several days (for vertical profiles of temperature, pressure, and humidity). In 2009, the monitoring program was upgraded to allow for additional targeted measurements of atmospheric conditions shor…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyFOS: Physical sciencesCosmic rayReal-time monitoring01 natural sciencesLarge detector systems for particle and astroparticle physics Real-time monitoring Control and monitor systems onlineOptical telescopeObservatory0103 physical sciencesSHOWERSLarge detector systems for particle and astroparticle physics; Real-time monitoring; Control and monitor systems onlineFLUORESCENCE010303 astronomy & astrophysicsInstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORMathematical PhysicsRemote sensingEvent reconstructionPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsControl and monitor systems online[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaENERGY-SPECTRUMMonitoring programControl and monitor systems online; Large detector systems for particle and astroparticle physics; Real-time monitoringAerosolATMOSFERA (MONITORAMENTO)Air showerExperimental High Energy PhysicsFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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