Welcome to the group homepage

The group is part of the Astrogroup within the Department of Physics & Astronomy at the University of Southampton. We study the circumnuclear dusty environment of active galactic nuclei to learn how supermassive black holes grow, how they influence their host galaxies, and how we can use them as cosmological probes.

Overview of the group's research profile

The illustration below highlights our main fields of research.


29 January 2018: Congratulations Daniel!
Daniel Asmus was awarded a prestigious and highly competitive Marie Sklodowsak Curie Fellowship. The fellowship will allow Daniel to continue his successful independent research on the dusty environment of AGN with his project DUSTDEVILS hosted in our group in Southampton. Only 15% of all applications to the scheme were successful.

22 December 2017: Et voila - VOILETTE!
Today we received a major allocation of observing time (453 hours) on ESO's VLT Survey Telescope to perform an optical support survey of the infrared public survey VEILS
. The survey will observe the same fields as VEILS in the optical griz bands with a cadence of 8(r)-14(giz) days during the 2018 and 2019 VEILS observing seasons. The VOILETTE survey (=VEILS OptIcal Lightcurves of Extragalactic TransienT Events; French for "veil") will essentially replace the optical monitoring of the VEILS fields that has been carried out with DES over the last years.

1 September 2017: Welcome Triana!
Triana R. Almeyda joins the group as a new research fellow. She recently completed her PhD at the Rochester Institute for Technology (Rochester, NY, USA) with Prof. Andy Robinson on modelling the optical and infrared variability of AGN. Triana will become responsible for data reduction and analysis of the VEILS survey. In particular, she will extract AGN light curves and determine dust time lags as required to use AGN as standard candles.

31 March 2017: CAT3D-WIND: Reconciling radiative transfer models with the latest developments in infrared observations of AGN
A new model has been published for the infrared emission of AGN. The model is an extension to CAT3D and takes into account the latest developments in infrared observations. Instead of a classical torus, CAT3D-WIND invokes a disk and a wind to reproduce the observed polar emission features in the mid-IR emission of AGN. This way, it is also possible account for the near-IR bumps between 3-5um seen in many type 1 AGN. The paper is available here:
Hoenig & Kishimoto 2017, ApJL 838, L20: Dusty Winds in Active Galactic Nuclei: Reconciling Observations with Models

Model SEDs can be downloaded from this site:

10 January 2017: VEILS -- the VISTA Extragalactic Infrared Legacy Survey
A new ESO Public Survey is currently undergoing its first observations -- and we are part of it! The survey is a 3-year project to monitor 9 sqrdeg of extragalactic fields in the infrared J and K band. This will facilitate research in galaxy evolution, supernova cosmology, and AGN variability. Manda Banerji (Cambridge) and Seb Hoenig are Co-PIs of the survey and we just published our first paper on the AGN science case
Hoenig et al. 2017, MNRAS 464, 1693: Cosmology with AGN dust time lags -- simulating the new VEILS survey

You can read more on the VEILS survey homepage:

08 September 2016: New 2017 job opening
We have an opening for a postdoc position in observational astrophysics. Please check out the jobs page if you are interested. Applications should be submitted by 15 November 2016. The ad will also be posted to the AAS job register in October.

30 August 2016: Welcome David, Marta and James!
David J. Williamson will join our group as a postdoc in September. He is an expert in hydrodynamic simulations and will work on developing a new radiative-hydrodynamical model of the dusty environment around AGN (see DUST-IN-THE-WIND project description). David received his PhD from St. Mary's University (Halifax, CA) in 2013 and spent the last 3 years as a postdoc in Dr Hugo Martel's group at the University of Laval (Quebec, CA).

Marta Venanzi will start as a PhD student at the end of September. She graduated from University of Rome La Sapienza with a Masters in Physics this summer. In the course of her final research project, she spent some time at QMUL. Marta's thesis project will focus on developing and exploiting effective and efficient methods to solve the radiative transfer problem in hydrodynamical simulations of dusty gas around AGN.

James H. Leftley will start a joint PhD project with ESO this October. His first two years will be spent at ESO's Chilean headquarters in Santiago before he returns to Southampton to finish his thesis. James graduates with a Master of Physics degree from the University of Southampton. He will use infrared interferometry to understand more about the mass distribution ad accretion processes around supermassive black holes.