Deep-learnt classification of light curves

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dc.contributor.author Mahabal, Ashish
dc.contributor.author Sheth, Kshiteej
dc.contributor.author Gieseke, Fabian
dc.contributor.author Pai, Akshay
dc.contributor.author George Djorgovski, S.
dc.contributor.author Drake, Andrew
dc.contributor.author Graham, Matthew
dc.contributor.other 2017 IEEE Symposium Series on Computational Intelligence (SSCI)
dc.coverage.spatial Honolulu, US
dc.date.accessioned 2018-05-15T10:39:53Z
dc.date.available 2018-05-15T10:39:53Z
dc.date.issued 2017-11-27
dc.identifier.citation Mahabal, Ashish; Sheth, Kshiteej; Gieseke, Fabian; Pai, Akshay; George Djorgovski, S.; Drake, Andrew and Graham, Matthew, "Deep-learnt classification of light curves", in the 2017 IEEE Symposium Series on Computational Intelligence (SSCI), Honolulu, US, Nov. 27 - Dec. 1, 2017. en_US
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/3660
dc.description.abstract A small variation in the elemental composition of a chemical compound can cause the formation of additional electronic defect states in the material, thereby altering the overall microstructure and thus induced properties. In this work, we observed chemical constitution-induced modification in the morphology and optoelectronic properties of SnS. To this end, SnS particles were prepared using the solution chemical route and were characterized using a wide range of experimental techniques, such as x-ray diffractometry, field emission scanning electron microscopy, high resolution transmission electron microscopy, energy dispersive spectroscopy (EDS), x-ray photoelectron spectroscopy (XPS), UV-Vis spectrophotometry, and scanning tunneling spectroscopy (STS). All these SnS particles are found to be Sn-rich and p-type. However, distinctly different morphologies (i.e., flower-like and aggregated ones) are observed. These are then correlated with the electronic defect states, which are induced because of the presence of Sn vacancies, Sn antisites, and/or Sn interstitials. A combination of EDS, XPS, and STS data confirmed the presence of a higher concentration of Sn vacancies along with lower quantities of Sn interstitials and/or antisites in the SnS particles with flower-like morphologies giving rise to higher hole concentration, which subsequently leads to reduced transport, optical band gaps, and barrier heights
dc.description.statementofresponsibility by Ashish Mahabal, Kshiteej Sheth, Fabian Gieseke, Akshay Pai, Djorgovski S. George, Andrew Drake and Matthew Graham
dc.language.iso en en_US
dc.title Deep-learnt classification of light curves en_US
dc.type Article en_US


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