The role of AGN and its obscuration on the position of the host galaxy relative to Main Sequence

We use X-ray Active Galactic Nuclei (AGN) observed by the Chandra X-ray Observatory within the 9.3 deg$^2$ Bo$\rm \ddot{o}$tes field of the NDWFS to study whether there is a correlation between X-ray luminosity (L$_X$) and star formation rate (SFR) of the host galaxy, at $\rm 0.5

Keywords:

• Spectral energy distribution
• Far infrared
• Star formation
• Absorption (logic)
• Galaxy
• Active galactic nucleus
• Redshift
• Astrophysics
• Physics
• Luminosity

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