960 resultados para Type-1 Fimbriae


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Quasars and AGN play an important role in many aspects of the modern cosmology. Of particular interest is the issue of the interplay between AGN activity and formation and evolution of galaxies and structures. Studies on nearby galaxies revealed that most (and possibly all) galaxy nuclei contain a super-massive black hole (SMBH) and that between a third and half of them are showing some evidence of activity (Kormendy and Richstone, 1995). The discovery of a tight relation between black holes mass and velocity dispersion of their host galaxy suggests that the evolution of the growth of SMBH and their host galaxy are linked together. In this context, studying the evolution of AGN, through the luminosity function (LF), is fundamental to constrain the theories of galaxy and SMBH formation and evolution. Recently, many theories have been developed to describe physical processes possibly responsible of a common formation scenario for galaxies and their central black hole (Volonteri et al., 2003; Springel et al., 2005a; Vittorini et al., 2005; Hopkins et al., 2006a) and an increasing number of observations in different bands are focused on collecting larger and larger quasar samples. Many issues remain however not yet fully understood. In the context of the VVDS (VIMOS-VLT Deep Survey), we collected and studied an unbiased sample of spectroscopically selected faint type-1 AGN with a unique and straightforward selection function. Indeed, the VVDS is a large, purely magnitude limited spectroscopic survey of faint objects, free of any morphological and/or color preselection. We studied the statistical properties of this sample and its evolution up to redshift z 4. Because of the contamination of the AGN light by their host galaxies at the faint magnitudes explored by our sample, we observed that a significant fraction of AGN in our sample would be missed by the UV excess and morphological criteria usually adopted for the pre-selection of optical QSO candidates. If not properly taken into account, this failure in selecting particular sub-classes of AGN could, in principle, affect some of the conclusions drawn from samples of AGN based on these selection criteria. The absence of any pre-selection in the VVDS leads us to have a very complete sample of AGN, including also objects with unusual colors and continuum shape. The VVDS AGN sample shows in fact redder colors than those expected by comparing it, for example, with the color track derived from the SDSS composite spectrum. In particular, the faintest objects have on average redder colors than the brightest ones. This can be attributed to both a large fraction of dust-reddened objects and a significant contamination from the host galaxy. We have tested these possibilities by examining the global spectral energy distribution of each object using, in addition to the U, B, V, R and I-band magnitudes, also the UV-Galex and the IR-Spitzer bands, and fitting it with a combination of AGN and galaxy emission, allowing also for the possibility of extinction of the AGN flux. We found that for 44% of our objects the contamination from the host galaxy is not negligible and this fraction decreases to 21% if we restrict the analysis to a bright subsample (M1450 <-22.15). Our estimated integral surface density at IAB < 24.0 is 500 AGN per square degree, which represents the highest surface density of a spectroscopically confirmed sample of optically selected AGN. We derived the luminosity function in B-band for 1.0 < z < 3.6 using the 1/Vmax estimator. Our data, more than one magnitude fainter than previous optical surveys, allow us to constrain the faint part of the luminosity function up to high redshift. A comparison of our data with the 2dF sample at low redshift (1 < z < 2.1) shows that the VDDS data can not be well fitted with the pure luminosity evolution (PLE) models derived by previous optically selected samples. Qualitatively, this appears to be due to the fact that our data suggest the presence of an excess of faint objects at low redshift (1.0 < z < 1.5) with respect to these models. By combining our faint VVDS sample with the large sample of bright AGN extracted from the SDSS DR3 (Richards et al., 2006b) and testing a number of different evolutionary models, we find that the model which better represents the combined luminosity functions, over a wide range of redshift and luminosity, is a luminosity dependent density evolution (LDDE) model, similar to those derived from the major Xsurveys. Such a parameterization allows the redshift of the AGN density peak to change as a function of luminosity, thus fitting the excess of faint AGN that we find at 1.0 < z < 1.5. On the basis of this model we find, for the first time from the analysis of optically selected samples, that the peak of the AGN space density shifts significantly towards lower redshift going to lower luminosity objects. The position of this peak moves from z 2.0 for MB <-26.0 to z 0.65 for -22< MB <-20. This result, already found in a number of X-ray selected samples of AGN, is consistent with a scenario of “AGN cosmic downsizing”, in which the density of more luminous AGN, possibly associated to more massive black holes, peaks earlier in the history of the Universe (i.e. at higher redshift), than that of low luminosity ones, which reaches its maximum later (i.e. at lower redshift). This behavior has since long been claimed to be present in elliptical galaxies and it is not easy to reproduce it in the hierarchical cosmogonic scenario, where more massive Dark Matter Halos (DMH) form on average later by merging of less massive halos.

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Das lrhA-Gen von E. coli kodiert für einen Transkriptionsregulator der LysR-Familie. Die Funktion von LrhA war ungeklärt und sollte durch Vergleich der Gesamt-mRNA aus einem E. coli-Wildtyp und einer isogenen lrhA-Mutante mit Hilfe von Genomanalysen untersucht werden. In der lrhA-Mutante war der mRNA-Gehalt vieler Gene um den Faktor 3 bis 80 erhöht. Es handelt sich um Flagellen-, Motilitäts- und Chemotaxisgene, bzw. um Gene der Typ 1 Fimbrien. Diese Ergebnisse wurden in Expressionsmessungen bestätigt. LrhA war in der Lage an den Promotor von flhDC zu binden, aber nicht an die Promotoren der übrigen Gene für Motilität und Chemotaxis. FlhDC kodiert für den übergeordneten Regulator FlhD2C2 der Fagellensynthese.LrhA war außerdem in der Lage an die Promotoren der Gene für Typ 1 Fimbrien fimA und fimE zu binden. Typ 1 Fimbrien stellen in E. coli Virulenzfaktoren dar. Eine Regulation weiterer Virulenzfaktoren durch LrhA konnte in DNA-Pathoarrays ausgeschlossen werden.LrhA ist damit ein wichtiger Transkriptionsregulator, der die Expression der Gene für Flagellen, Motilität, Chemotaxis und Typ 1 Fimbrien reguliert. FlhDC, fimA und fimE stellen dabei direkte Zielgene von LrhA dar. Außerdem konnte eine positive Autoregulation von LrhA nachgewiesen werden.

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"Silent mating type information regulation 2 Type" 1 (SIRT1), das humane Homolog der NAD+-abhängigen Histondeacetylase Sir2 aus Hefe, besitzt Schlüsselfunktionen in der Regulation des Metabolismus, der Zellalterung und Apoptose. Letztere wird vor allem durch die Deacetylierung von p53 an Lys382 und der dadurch verringerten Transkription proapoptotischer Zielgene vermittelt. Im Rahmen der vorliegenden Arbeit wurde die SIRT1 Regulation im Zusammenhang mit der DNA-Schadensantwort untersucht.rnIn der Apoptoseregulation übernimmt die Serin/Threonin-Kinase "Homeodomain interacting protein kinase" 2 (HIPK2) eine zentrale Rolle und daher wurde die SIRT1 Modifikation und Regulation durch HIPK2 betrachtet. Durch Phosphorylierung des Tumorsuppressorproteins p53 an Ser46 aktiviert HIPK2 das Zielprotein und induziert die Transkription proapoptotischer Zielgene von p53. Es wurde beschrieben, dass HIPK2 nach DNA-Schädigung über einen bisher unbekannten Mechnismus die Acetylierung von p53 potenzieren kann.rnIn der vorliegenden Arbeit konnte gezeigt werden, dass SIRT1 von HIPK2 in vitro und in Zellen an Serin 27 und 682 phosphoryliert wird. Weiterhin ist die Interaktion von SIRT1 mit HIPK2 sowie die SIRT1 Phosphorylierung an Serin 682 durch DNA-schädigende Adriamycinbehandlung erhöht. Es gibt Hinweise, dass HIPK2 die Expression von SIRT1 reguliert, da HIPK2 RNA-Interferenz zur Erniedrigung der SIRT1 Protein- und mRNA-Mengen führt.rnEin weiterer interessanter Aspekt liegt in der Beobachtung, dass Ko-Expression von PML-IV, welches SIRT1 sowie HIPK2 in PML-Kernkörper rekrutiert, die SIRT1 Phosphorylierung an Serin 682 verstärkt. Phosphorylierung von SIRT1 an Serin 682 interferiert wiederum mit der SUMO-1 Modifikation, welche für die Lokalisation in PML-Kernkörpen wichtig ist.rnBemerkenswerterweise reduziert die DNA-schadendsinduzierte SIRT1 Phosphorylierung die Bindung des SIRT1 Ko-Aktivators AROS, beeinflusst aber nicht diejenige des Inhibitors DBC1. Dies führt zur Reduktion der enzymatischen Aktivität von SIRT1 und der darausfolgenden weniger effizienten Deacetylierung des Zielproteins p53.rnDurch die von mir in der vorliegenden Promotionsarbeit erzielten Ergebnisse konnte ein neuer molekularer Mechanismus entschlüsselt werden, welcher die durch HIPK2 modulierte Acetylierung von p53 und die daran anschließende Induktion der Apoptose beschreibt.rnHIPK2-vermittelte SIRT1 Phosphorylierung resultiert in einer verminderten Deacetylasefunktion von SIRT1 und führt so zu einer verstärkten acetylierungsinduzierten Expression proapoptotischer p53 Zielgene.

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In type 1 diabetes (T1DM), a good metabolic control is important to reduce and/or postpone complications. Guidelines regarding how to achieve this goal are published by the American Diabetes Association (ADA) and the International Society of Paediatric and Adolescence Diabetes (ISPAD). The aims of this study were to determine the current level of metabolic control in T1DM patients on different treatment regimens, followed at the diabetes outpatient unit of the University Children's Hospital Bern, Switzerland, and to compare it with both the reported data from ten years ago (1998) and with the current guidelines of the ADA and ISPAD.

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To compare exercise-induced growth hormone (GH) response in patients with Type 1 diabetes during stable euglycaemic and hyperglycaemic conditions.

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The aim of this randomized, single-blinded cross-over study was to investigate the response of interleukin-6 (IL-6) during moderate aerobic exercise in stable euglycaemia and hyperglycaemia in seven male patients with type 1 diabetes mellitus. IL-6 increased significantly over the entire study period in euglycaemia, but not in hyperglycaemia.

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To compare gingival crevicular fluid (GCF) biomarker levels and microbial distribution in plaque biofilm (SP) samples for subjects with type 1 diabetes (T1DM) versus healthy subjects without diabetes during experimental gingivitis (EG).

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Intramyocellular acetylcarnitine (IMAC) is involved in exercise-related fuel metabolism. It is not known whether levels of systemic glucose influence IMAC levels in type 1 diabetes.

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Sequence data from resistance testing offer unique opportunities to characterize the structure of human immunodeficiency virus (HIV) infection epidemics.

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Episodic ataxia type 1 is a neuronal channelopathy caused by mutations in the KCNA1 gene encoding the fast K(+) channel subunit K(v)1.1. Episodic ataxia type 1 presents with brief episodes of cerebellar dysfunction and persistent neuromyotonia and is associated with an increased incidence of epilepsy. In myelinated peripheral nerve, K(v)1.1 is highly expressed in the juxtaparanodal axon, where potassium channels limit the depolarizing afterpotential and the effects of depolarizing currents. Axonal excitability studies were performed on patients with genetically confirmed episodic ataxia type 1 to characterize the effects of K(v)1.1 dysfunction on motor axons in vivo. The median nerve was stimulated at the wrist and compound muscle action potentials were recorded from abductor pollicis brevis. Threshold tracking techniques were used to record strength-duration time constant, threshold electrotonus, current/threshold relationship and the recovery cycle. Recordings from 20 patients from eight kindreds with different KCNA1 point mutations were compared with those from 30 normal controls. All 20 patients had a history of episodic ataxia and 19 had neuromyotonia. All patients had similar, distinctive abnormalities: superexcitability was on average 100% higher in the patients than in controls (P < 0.00001) and, in threshold electrotonus, the increase in excitability due to a depolarizing current (20% of threshold) was 31% higher (P < 0.00001). Using these two parameters, the patients with episodic ataxia type 1 and controls could be clearly separated into two non-overlapping groups. Differences between the different KCNA1 mutations were not statistically significant. Studies of nerve excitability can identify K(v)1.1 dysfunction in patients with episodic ataxia type 1. The simple 15 min test may be useful in diagnosis, since it can differentiate patients with episodic ataxia type 1 from normal controls with high sensitivity and specificity.

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To investigate the efficacy of sensor-augmented pump therapy vs. multiple daily injection therapy in patients with suboptimally controlled Type 1 diabetes.

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SMARTDIAB is a platform designed to support the monitoring, management, and treatment of patients with type 1 diabetes mellitus (T1DM), by combining state-of-the-art approaches in the fields of database (DB) technologies, communications, simulation algorithms, and data mining. SMARTDIAB consists mainly of two units: 1) the patient unit (PU); and 2) the patient management unit (PMU), which communicate with each other for data exchange. The PMU can be accessed by the PU through the internet using devices, such as PCs/laptops with direct internet access or mobile phones via a Wi-Fi/General Packet Radio Service access network. The PU consists of an insulin pump for subcutaneous insulin infusion to the patient and a continuous glucose measurement system. The aforementioned devices running a user-friendly application gather patient's related information and transmit it to the PMU. The PMU consists of a diabetes data management system (DDMS), a decision support system (DSS) that provides risk assessment for long-term diabetes complications, and an insulin infusion advisory system (IIAS), which reside on a Web server. The DDMS can be accessed from both medical personnel and patients, with appropriate security access rights and front-end interfaces. The DDMS, apart from being used for data storage/retrieval, provides also advanced tools for the intelligent processing of the patient's data, supporting the physician in decision making, regarding the patient's treatment. The IIAS is used to close the loop between the insulin pump and the continuous glucose monitoring system, by providing the pump with the appropriate insulin infusion rate in order to keep the patient's glucose levels within predefined limits. The pilot version of the SMARTDIAB has already been implemented, while the platform's evaluation in clinical environment is being in progress.

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Optic pathway gliomas, which occur in 15-20% of paediatric patients with neurofibromatosis type 1, are the most common central nervous system tumour associated with this neurocutaneous disorder. The detection of optic pathway gliomas is essential for further management but is often delayed in infancy due to oligosymptomatic progression and difficulties in clinical detection. Therefore, the aim of our study was to find a clinical indicator for the presence of optic pathway gliomas in children with neurofibromatosis type 1 in order to facilitate early diagnosis and initiate further ophthalmological and neuroimaging investigations.