A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies

TL;DR

This study investigates the properties of DLA-galaxies at z~0.6 using VLT/X-Shooter spectroscopy, revealing their star formation rates, metallicities, and the relationship with the circum-galactic medium, with a high detection success rate.

Contribution

First detailed spectroscopic analysis of DLA-galaxies at z~0.6 linking their properties to the circum-galactic medium and star formation activity.

Findings

78% detection rate of DLA-galaxies in the sample

DLA-galaxies have SFRs from 0.3 to 6.7 M_sun/yr

Metallicities range from 0.2 to 0.9 Z_sun

Abstract

We present the study of a sample of nine QSO fields, with damped-Ly-alpha (DLA) or sub-DLA systems at z~0.6, observed with the X-Shooter spectrograph at the Very Large Telescope. By suitably positioning the X-Shooter slit based on high spatial resolution images of HST/ACS we are able to detect absorbing galaxies in 7 out of 9 fields (~ 78\% success rate) at impact parameters from 10 to 30 kpc. In 5 out of 7 fields the absorbing galaxies are confirmed via detection of multiple emission lines at the redshift of DLAs where only 1 out of 5 also emits a faint continuum. In 2 out of these 5 fields we detect a second galaxy at the DLA redshift. Extinction corrected star formation rates (SFR) of these DLA-galaxies, estimated using their H-alpha fluxes, are in the range 0.3-6.7 M_sun yr^-1. The emission metallicities of these five DLA-galaxies are estimated to be from 0.2 to 0.9 Z_sun. Based on the Voigt profile fits to absorption lines we find the metallicity of the absorbing neutral gas to be in a range of 0.05--0.6 Z_sun. The two remaining DLA-galaxies are quiescent galaxies with SFR < 0.4 M_sun yr^-1 (3-sigma) presenting continuum emission but weak or no emission lines. Using X-Shooter spectrum we estimate i-band absolute magnitude of -19.5+/-0.2 for both these DLA-galaxies that indicates they are sub-L* galaxies. Comparing our results with that of other surveys in the literature we find a possible redshift evolution of the SFR of DLA-galaxies.