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In addition, we have made an all-sky animation from our series of daily all-sky images. This animation shows how the objects on the Galactic plane transiently appear and then disappear, and often vary violently. (Image 2) MAXI has detected several gamma-ray bursts, whose majority is confirmed to be related to supernova explosions. Gamma-ray bursts are the enormous explosions that are thought to be the largest in the Universe, and many of these bursts occur billions-light years away. Their process of X-ray generation is insufficiently understood, and they remain a mystery. Over more than seven months, we observed an X-ray nova of a black hole binary as it appeared near the Galactic center. X-ray nova appeared suddenly like a bright firework, but MAXI succeeded in detecting a rising phase of an X-ray nova before the peak of its burst and following its evolution until it has vanished. Bright X-ray novae with black holes are seen only once or twice per year in the entire sky, so these MAXI data are very valuable, and we have already published the paper on it. (Image 3) A binary X-ray pulsar consists of a neutron star with a strong magnetic field and an ordinary star. The gases from the ordinary star flow into the neutron star, and the brightness alters depending on the amount of gas flow. MAXI observed these X-ray pulsars, and obtained unique data on the structure and evolution of these gases. Additionally, it obtained the X-ray pulsars that had been re-activated after several years, as well as a new, little-known phenomenon; i.e. X-ray pulsars that extremely brighten only for a few hours. MAXI observed active galaxies with producing jets that make variable X-ray intensely, like enormous flares. We obtained valuable data that could explain the conditions under which active galaxies eject jets by simultaneous observation with radio and ultra-high energy gamma-rays. MAXI also detected the jets which were produced from micro-Quasars; i.e. binary active stars accompanying a black hole or a neutron star. MAXI performed the first all-sky soft X-ray observation using the X-ray CCD camera whose CCDs are produced by Japanese company. This allowed us to confirm that there are many soft X-ray objects along the galactic plane, as well as to reveal the existence of high-temperature plasmas surrounding the solar system. If we continue our observation on how much and what kind of elements exist in the hot plasma - such as the distribution of oxygen and neon emission lines - we could get close to solving the mystery of the origin and evolution of the hot plasmas. (Image 4)