Low-redshift quasars in the SDSS Stripe 82 – III. MOS observations

Bettoni, D. (ORCID:0000000241586496); Falomo, R. (ORCID:0000000341376541); Paiano, S. (ORCID:0000000222393373); Kotilainen, J. K.; Stone, M. B. (ORCID:0000000229310593)

doi:10.1093/mnras/stac3606

DOE OSTI · 1908252

Low-redshift quasars in the SDSS Stripe 82 – III. MOS observations

Bettoni, D. (ORCID:0000000241586496)·Falomo, R. (ORCID:0000000341376541)·Paiano, S. (ORCID:0000000222393373)·Kotilainen, J. K.·Stone, M. B. (ORCID:0000000229310593)

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Abstract

ABSTRACT We present multi-object optical spectroscopy of the galaxies in the environment of 12 low-redshift (z < 0.5) quasars and of 11 inactive massive galaxies chosen to match the properties of the quasar host galaxies to probe physical association and possible events of recent star formation (SF). The quasars are selected from a sample of QSOs in the Sloan Digital Sky Survey (SDSS) Stripe 82 region for which both the host galaxy and the large-scale environments were previously investigated. The new observations complement those reported in our previous works on close companion galaxies of nearby quasars. For the whole data set, we find that for about half (19 out of 44) of the observed QSOs, there is at least one associated companion galaxy. In addition to the new spectroscopic observations, we add data from the SDSS data base for the full sample of objects. We find that the incidence of companion galaxies in the fields of QSO (17 per cent) is not significantly different from that of inactive galaxies (19 per cent) similar to quasar hosts in redshift and mass. Nevertheless, the companions of quasars exhibit more frequently emission lines than those of inactive galaxies, suggesting a moderate link between the nuclear activity and recent SF in their environments.

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Bettoni, D. (ORCID:0000000241586496), Falomo, R. (ORCID:0000000341376541), Paiano, S. (ORCID:0000000222393373), Kotilainen, J. K., Stone, M. B. (ORCID:0000000229310593). 2022-12-09. Low-redshift quasars in the SDSS Stripe 82 – III. MOS observations. https://doi.org/10.1093/mnras%2Fstac3606

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