H-Link simulator

Aquest projecte intenta donar solució al problema amb el qual s'ha trobat la empresa Hitachi Air Conditioning Products SA a la hora de fer probes durant el desenvolupament del seu principal producte, el CSNet Web. El simulador que s'ha realitzat en aquest projecte pretén reproduir la topologia d'una xarxa d'unitats d'aire condicionat per a que el CSNet Web les interpreti com si aquestes màquines fossin reals. Per a aconseguir-ho, el simulador reproduirà les comunicacions entre aquestes màquines i el CSNet Web.Este proyecto intenta dar solución al problema que se ha encontrado la empresa Hitachi Air Conditioning Produtcs Europe SA a la hora de hacer pruebas en el desarrollo de su principal producto de control de máquinas de aire acondicionado, el CSNet Web. El simulador que se ha realizado en este proyecto, pretende reproducir la topología de una red de unidades de aire acondicionado para que el CSNet Web lo interprete como si esas maquinas fueran reales. Para ello, el simulador reproducirá las comunicaciones entre estas máquinas con el CSNet Web.This project tries to solve to the problem that Hitachi Air Conditioning Produtcs Europe SA company found when they makes test during the development of its principal product of air conditionating control machines, called CSNet Web. The simulator created in this project, tries to reproduce the topology of a network of air conditioning machines. CSNet Web interprets this topology as real machines. In order to achieve this goal, this simulator will reproduce the communications between these machines and CSNet Web

H-Link simulator

Aquest projecte intenta donar solució al problema amb el qual s'ha trobat la empresa Hitachi Air Conditioning Products SA a la hora de fer probes durant el desenvolupament del seu principal producte, el CSNet Web. El simulador que s'ha realitzat en aquest projecte pretén reproduir la topologia d'una xarxa d'unitats d'aire condicionat per a que el CSNet Web les interpreti com si aquestes màquines fossin reals. Per a aconseguir-ho, el simulador reproduirà les comunicacions entre aquestes màquines i el CSNet Web.Este proyecto intenta dar solución al problema que se ha encontrado la empresa Hitachi Air Conditioning Produtcs Europe SA a la hora de hacer pruebas en el desarrollo de su principal producto de control de máquinas de aire acondicionado, el CSNet Web. El simulador que se ha realizado en este proyecto, pretende reproducir la topología de una red de unidades de aire acondicionado para que el CSNet Web lo interprete como si esas maquinas fueran reales. Para ello, el simulador reproducirá las comunicaciones entre estas máquinas con el CSNet Web.This project tries to solve to the problem that Hitachi Air Conditioning Produtcs Europe SA company found when they makes test during the development of its principal product of air conditionating control machines, called CSNet Web. The simulator created in this project, tries to reproduce the topology of a network of air conditioning machines. CSNet Web interprets this topology as real machines. In order to achieve this goal, this simulator will reproduce the communications between these machines and CSNet Web

Very high energy gamma-ray observation of the peculiar transient event Swift J1644+57 with the MAGIC telescopes and AGILE

Context. On March 28, 2011, the BAT instrument on board the Swift satellite detected a new transient event that in the very beginning was classified as a gamma ray burst (GRB). However, the unusual X-ray flaring activity observed from a few hours up to days after the onset of the event made a different nature seem to be more likely. The long-lasting activity in the X-ray band, followed by a delayed brightening of the source in infrared and radio activity, suggested that it is better interpreted as a tidal disruption event that triggered a dormant black hole in the nucleus of the host galaxy and generated an outflowing jet of relativistic matter. Aims. Detecting a very high energy emission component from such a peculiar object would be enable us to constrain the dynamic of the emission processes and the jet model by providing information on the Doppler factor of the relativistic ejecta. Methods. The MAGIC telescopes observed the peculiar source Swift J1644+57 during the flaring phase, searching for gamma-ray emission at very-high energy (VHE, E > 100 GeV), starting observations nearly 2.5 days after the trigger time. MAGIC collected a total of 28 h of data during 12 nights. The source was observed in wobble mode during dark time at a mean zenith angle of 35 degrees. Data were reduced using a new image-cleaning algorithm, the so-called sum-cleaning, which guarantees a better noise suppression and a lower energy threshold than the standard analysis procedure. Results. No clear evidence for emission above the energy threshold of 100 GeV was found. MAGIC observations permit one to constrain the emission from the source down to 100 GeV, which favors models that explain the observed lower energy variable emission. Data analysis of simultaneous observations from AGILE, Fermi and VERITAS also provide negative detection, which additionally constrain the self-Compton emission component

MAGIC detection of short-term variability of the high-peaked BL Lac object 1ES 0806+524

ISSN:0035-8711ISSN:1365-2966ISSN:1365-871