Examining HST observations of some active galactic nuclei that detected with Chandra observatory
2016
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Advisor: Prof. Dr. Aysun Akyüz
Abstract (EN)
In the present thesis the properties about various wavelengths of Active Galactic Nuclei which make up a large class of the astrophysical sources have been studied. For this purpose, X-ray (Chandra) and optical (Hubble Space Telescope, HST) archive data are analyzed. Optical counterparts of X-ray sources that are determined from the Chandra Deep Space-South (CDF-S) region observation data, have been identified inside the field of view of HST observations. Characteristic properties such as V and I band magnitudes and their comparison with field sources, Hardness Ratios, Flux values etc. are examined. V-I color diagrams of optical counterparts show that they could be classified as optically faint and bright populations .
Author
Aysun Yaşar
How to Cite
Aysun Yaşar (Master Thesis). Examining HST observations of some active galactic nuclei that detected with Chandra observatory, 2016, Çukurova University.
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