The role of AGN and obscuration in the position of the host galaxy relative to the main sequence

We use X-ray active galactic nuclei (AGN) observed by the Chandra X-ray Observatory within the 9.3 deg 2 Boötes 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 0.5 < z

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Bibliographische Detailangaben
Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-09, Vol.653
Hauptverfasser:	Mountrichas, G., Buat, V., Yang, G., Boquien, M., Burgarella, D., Ciesla, L., Malek, K., Shirley, R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Cosmology and Extra-Galactic Astrophysics Sciences of the Universe
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Beschreibung
Zusammenfassung:	We use X-ray active galactic nuclei (AGN) observed by the Chandra X-ray Observatory within the 9.3 deg 2 Boötes 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 0.5 < z
ISSN:	0004-6361 1432-0756
DOI:	10.1051/0004-6361/202140630