Satellite Gaia of The European Space Agency made its second data release publicly available on April 25, 2018. In this data there are measurements of parallax (distance), motion, intensity and color of more than a billion stars in Milky way galaxy. Among the observed sources, white dwarfs were also detected. White dwarfs are the remants of stars in which there are no ongoing nuclear reactions. They are extremely dense and hot objects that are similar in size to Earth and have a mass between 0.6 and 1.4 masses of the Sun. The hydrostatic equilibrium in these objects is sustained by degenerate electron gas. That is why they slowly cool and dim at the constant size. From a huge data set created by the Gaia satellite, it is possible to extract a handful of objects that show the characteristics of white dwarfs. This can be obtained by drawing an HR-diagram by comparing the absolute magnitude of each object with its color. White dwarfs have a characteristic position on such a graph, away from the main sequence stars. By limiting the measurement error and the noise, $63414$ white dwarf candidated were extracted, which is the largest collection of white dwarfs to date. The main information for these sources is their position, that was precisely determined and then mapped out on the night sky, to gain a basic picture of their distribution in the Milky way galaxy. In the end, through basic physical models, general physical properties were computed, such as luminosity, effective temperature, radius, mass and age, which were then statistically processed.
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