28 research outputs found

    Observation of the TeV gamma-ray source MGRO J1908+06 with ARGO-YBJ

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    The extended gamma ray source MGRO J1908+06, discovered by the Milagro air shower detector in 2007, has been observed for about 4 years by the ARGO-YBJ experiment at TeV energies, with a statistical significance of 6.2 standard deviations. The peak of the signal is found at a position consistent with the pulsar PSR J1907+0602. Parametrizing the source shape with a two-dimensional Gauss function we estimate an extension \sigma = 0.49 \pm 0.22 degrees, consistent with a previous measurement by the Cherenkov Array H.E.S.S.. The observed energy spectrum is dN/dE = 6.1 \pm 1.4 \times 10^-13 (E/4 TeV)^{-2.54 \pm 0.36} photons cm^-2 s^-1 TeV^-1, in the energy range 1-20 TeV. The measured gamma ray flux is consistent with the results of the Milagro detector, but is 2-3 times larger than the flux previously derived by H.E.S.S. at energies of a few TeV. The continuity of the Milagro and ARGO-YBJ observations and the stable excess rate observed by ARGO-YBJ along 4 years of data taking support the identification of MGRO J1908+06 as the steady powerful TeV pulsar wind nebula of PSR J1907+0602, with an integrated luminosity above 1 TeV about 1.8 times the Crab Nebula luminosity.Comment: 6 pages, accepted for pubblication by ApJ. Replaced to correct the author lis

    Long-term Monitoring on Mrk 501 for Its VHE gamma Emission and a Flare in October 2011

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    As one of the brightest active blazars in both X-ray and very high energy Îł\gamma-ray bands, Mrk 501 is very useful for physics associated with jets from AGNs. The ARGO-YBJ experiment is monitoring it for Îł\gamma-rays above 0.3 TeV since November 2007. Starting from October 2011 the largest flare since 2005 is observed, which lasts to about April 2012. In this paper, a detailed analysis is reported. During the brightest Îł\gamma-rays flaring episodes from October 17 to November 22, 2011, an excess of the event rate over 6 σ\sigma is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the Îł\gamma-ray flux above 1 TeV by a factor of 6.6±\pm2.2 from its steady emission. In particular, the Îł\gamma-ray flux above 8 TeV is detected with a significance better than 4 σ\sigma. Based on time-dependent synchrotron self-Compton (SSC) processes, the broad-band energy spectrum is interpreted as the emission from an electron energy distribution parameterized with a single power-law function with an exponential cutoff at its high energy end. The average spectral energy distribution for the steady emission is well described by this simple one-zone SSC model. However, the detection of Îł\gamma-rays above 8 TeV during the flare challenges this model due to the hardness of the spectra. Correlations between X-rays and Îł\gamma-rays are also investigated.Comment: have been accepted for publication at Ap

    ISTITUTO NAZIONALE DI FISICA NUCLEARE GLUE SCHEMA IMPLEMENTATION FOR THE LDAP DATA MODEL *

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    Abstract An important aspect of the interoperability among different Grid systems is the definition of a common schema for the representation of Grid resources. This is vital for sharing the status and availability of resources at the virtual level. The GLUE schema is designed to fulfil this need by providing a conceptual schema of the relevant resources. This paper presents a mapping of this schema into the LDAP data model. It is used in the Globus MDS version 2. Published by SIS-Pubblicazioni Laboratori Nazionali di Frascat

    Top cross section measurement at CDF

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    This paper describes the latest measurements of the t{bar t} pair production cross section performed by the CDF Collaboration analyzing p{bar p} collisions at a center-of-mass energy of 1.96 TeV from Fermilab Tevatron, as presented at the XVIII International Workshop on Deep-Inelastic Scattering and Related Subjects. In order to test Standard Model predictions, several analysis methods are explored and all the top decay channels are considered, to better constrain the properties of the top quark and to search for possible sources of new physics affecting the pair production mechanism. Experimental results using an integrated luminosity up to 5.1 fb{sup -1} are presented

    Familles, migrations et solidarités intergénérationnelles : enjeux politiques et sociétaux

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    La globalisation et l’accĂ©lĂ©ration des flux migratoires conduisent un nombre grandissant de personnes Ă  vivre leurs relations familiales par-delĂ  les frontiĂšres gĂ©ographiques, dans un contexte de dĂ©mocratisation relative des transports et d’un accĂšs accru Ă  des technologies de la communication de plus en plus sophistiquĂ©es. Cette prĂ©sentation s’appuie sur un programme de recherche (TRANSFAM) qui s’inscrit dans le champ d’étude des familles dites ‘transnationales’, qui comptent en leur sein des membres vivant dans diffĂ©rents pays et qui maintiennent vivants leurs liens familiaux, notamment via des pratiques d’entraide familiale dĂ©sormais transnationales. De nos jours, les migrants Ă©changent Ă  des degrĂ©s divers du soutien matĂ©riel, financier, pratique et Ă©motionnel avec leurs enfants, leurs frĂšres et sƓurs, et leurs parents vieillissants, parfois quotidiennement. Ces diffĂ©rents protagonistes se dĂ©placent Ă©galement pour prendre soin de, ou ĂȘtre pris en charge par les leurs. Articuler vie familiale et professionnelle dans un tel contexte pose de rĂ©els dĂ©fis. Cette prĂ©sentation passera notamment en revue les ressources dont ces familles ont besoin pour participer Ă  ces solidaritĂ©s, et identifiera les politiques qui facilitent, ou au contraire font obstacle au maintien de ces solidaritĂ©s
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