... galaxy within the 2 arc second error region of a GRB x-ray afterglow is identified as a host galaxy; however confusion can rise due to the facts that 1. the edge of a galaxy is diffused, 2. multiple sources could exist within 2 arc second error region, 3 ...
... The AstroStat Slog . [ArXiv] SVM and galaxy morphological classification, Sept. 10, 2007 . Leave a comment . Admin . ... A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. ...
... galaxy within the 2 arc second error region of a GRB x-ray afterglow is identified as a host galaxy; however confusion can rise due to the facts that 1. the edge of a galaxy is diffused, 2. multiple sources could exist within 2 arc second error region, 3 ...
... galaxy within the 2 arc second error region of a GRB x-ray afterglow is identified as a host galaxy; however confusion can rise due to the facts that 1. the edge of a galaxy is diffused, 2. multiple sources could exist within 2 arc second error region, 3 ...
... galaxy within the 2 arc second error region of a GRB x-ray afterglow is identified as a host galaxy; however confusion can rise due to the facts that 1. the edge of a galaxy is diffused, 2. multiple sources could exist within 2 arc second error region, 3 ...
... Galaxy Photometry Data Zach Clayto , Peter Capa , Dan Maste 1 1 r 2 k 2 rs Ohio ... In essence, highz galaxies are lost to low-z regions, and low-z galaxies contaminate ... galaxies that scatter will depend on the number of galaxies in each cell (i.e ...
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Ссылки http://hea-www.harvard.edu/AstroStat/aas227_2016/Zachary_Claytor_Summer_Poster.pdf -- 840.5 Кб -- 06.01.2016 Похожие документы