# Water masers in Compton-thick AGN II. The high detection rate and EVN observations of IRAS 15480-0344

## TL;DR

This study reports a high detection rate of water masers in heavily absorbed, Compton-thick AGN, including new VLBI observations of IRAS 15480-0344, revealing complex maser components and jet-cloud interactions.

## Contribution

It presents the discovery of a luminous water maser in IRAS 15480-0344 and demonstrates a 50% detection rate in a well-defined Compton-thick AGN sample, with detailed EVN imaging insights.

## Key findings

- High maser detection rate (50%) in Compton-thick AGN sample.
- Discovery of a luminous water maser in IRAS 15480-0344.
- EVN imaging reveals jet knots interacting with molecular clouds.

## Abstract

Investigations of H$_2$O maser galaxies at X-ray energies reveal that most AGN associated with water masers are characterized by high levels of absorption. With the aim of finding new maser sources for possible interferometric follow-ups, we have searched for water maser emission in a well-defined sample of heavily absorbed AGN ($N_{\rm H} > 10^{23}$ cm$^{-2}$), including Compton-thick (CT) sources. All the galaxies in the sample were already searched for 22 GHz water maser emission in previous surveys. With the goal of providing a detection or a stringent upper limit on the H$_2$O luminosity, we re-observed some of the non-detected sources with the Green Bank Telescope. A new luminous H$_2$O maser ($L_{\rm H2O} \sim 200\,$L$_\odot$) was detected in the mid-IR-bright Seyfert 2 galaxy IRAS 15480-0344 and then followed-up with the Very Long Baseline Array. In order to shed light on the origin of the maser (jet/outflow vs. disc), we recently observed the radio continuum emission in IRAS 15480-0344 with the European VLBI network (EVN) at 1.7 and 5.0 GHz. With the newly discovered megamaser in IRAS 15480-0344 revealing a narrow ($\sim$0.6 km s$^{-1}$) and a broad ($\sim$90 km s$^{-1}$) component, the maser detection rate of the CT AGN sample is 50% (18/36), which is one of the highest ever found in maser surveys. The EVN maps show two bright sources (labeled SW and NE) in the nuclear region of IRAS 15480-0344, which we interpret as jet knots tracing regions where the radio plasma impacts dense molecular clouds. [abridged]