2022MNRAS.514.1335S

We explore indirect methods to detect polycyclic aromatic hydrocarbons (PAHs) in gas-rich, absorption-selected galaxies at high redshift. We look at the optical X-Shooter observations of an intervening, extremely strong damped Lyman α absorber (or ESDLA, with log [N(H I) >= 21.7)] towards QSO SDSS J1143+1420 at redshift, z_ESDLA = 2.323. Literature studies have shown that this ESDLA contains signatures of dust and diffuse molecular hydrogen and it was specifically chosen for our study due to its close spatial proximity (impact parameter, ρ= 0.6 ±0.3 kpc) with its associated galaxy. There is no direct detection of PAHs emission in the limited observations of infrared spectra along this sightline. Hence, we use CLOUDY numerical simulation modelling to indirectly probe the presence of PAHs in the ESDLA. We note that PAHs need to be included in the models to reproduce the observed column densities of warm H₂ and C I. Thus, we infer the presence of PAHs indirectly in our ESDLA, with an abundance of PAH/H = 10^–7.046. We also measure a low 2175 Å bump strength (E_bump ∼0.03 - 0.19 mag) relative to star-forming galaxies by modelling extinction of quasar QSO spectra by dust at the absorber rest frame. This is consistent with the low PAH abundance obtained indirectly using CLOUDY modelling. Our study highlights the usage of CLOUDY modelling to indirectly detect PAH in high-redshift gas-rich absorption-selected galaxies.