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a new machine learning technique developed at cornell university allows astronomers to find the location of asteroids and other objects in space that are moving through the solar system. the technique, which is based on deep learning algorithms, is called deep virtual telescope, or d-vast.

the webb telescope will be more precise than hubble and will also examine the abundance of elements in distant stars, which, like earth, might contain a record of the chemical reactions that occurred in the early universe. the telescope will be capable of detecting very faint light, at the limit of what human eyes can see, and will be able to look through clouds of gas and dust in deep space, to explore the evolution of the universe back to the beginning.

the webb telescope will focus on a tiny region of the sky, the hubble ultra deep field, to study the cosmos in detail. the telescope will be able to examine the universe for the first time in infrared wavelengths and for the first time in ultraviolet wavelengths.

the new model is not only a breakthrough in terms of the spatial resolution and the number of parameters considered, but also a major advance in terms of the physical understanding of the fault structures. the model is able to reproduce well the observation (additional file 4 : fig. s4). the dip of the fault beneath mashiki town is determined to be southward-dipping. additional file 5 ; fig. s5 shows the best solution when the dip is assumed to be north-dipping(table 3 ). the north-dipping fault also can account for the displacement field well. the root mean squares (rmss) are estimated to be 1.2 and 1.3cm for the south- and north-dipping faults, respectively. there is no significant visible difference in fitting between the south- and north-dipping faults, but the akaikes information criterion (aic) (akaike 1974 ) values support the south-dipping model (aic=153.8) rather than the north-dipping one (aic=212.7). according to nied ( 2016 ) and kyushu university ( 2016 ), the hypocenters align along a west-dipping orientation in the central part of the hinagu fault, while in the northern part, where the hypocenter of m j 6.5 is located, the distribution extends slightly deeper toward the east rather than to the west. although there is no decisive evidence, the south-dipping fault seems to be the favorable solution.


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