Revealing the structure of the lensed quasar Q 0957+561. II. Supermassive black hole mass via gravitational redshift
Aims: We intend to use the impact of microlensing on the Fe III λλ2039−2113 emission line blend along with a measure of its gravitational redshift to estimate the mass of the quasar's central supermassive black hole (SMBH). Methods: We fit the Fe III feature in multiple spectroscopic observations between 2008 and 2016 of the gravitationally lensed
Fian, C. et al.
Fecha de publicación:
11
2022