Scientific areas of interest

Galaxy formation and evolution. Multi-wavelength observations of galaxies in the local and high-redshift Universe. Feedback mechanisms from star formation and accreting super massive black holes. Multi-phase and multi-scale galactic outflows. The circumgalactic and intergalactic medium. Galaxy interactions and mergers. (Sub)-millimetre telescopes and observational techniques. Dual and binary active galactic nuclei. The thermal and kinetic Sunyaev-Zel'dovich (SZ) effect.

Ongoing projects

Towards an Atacama Large Aperture Submillimeter Telescope 

Astrophysical observations at (sub-)mm wavelengths (λ from ~300 μm to ~3mm) allow us to study the cold and dense material in the Universe, hence probing the formation of stars and planets, and the interstellar and circumgalactic medium of galaxies across all cosmic times.  The current generation of 10-m class single dish telescopes delivered the first surveys of the sky at (sub-)mm wavelengths, allowing us to go far beyond the previously optical/IR- biased view of the Universe. Follow-up observations with interferometers then revealed, in exquisite detail, the morphology and kinematics of such (sub-)mm sources, enabling tests and revisions of theoretical models for the formation and evolution of planets, stars, and galaxies.  However, it is now clear that without a step change in the capabilities of single-dish facilities in the 2030s, interferometers (like the ALMA observatory) will soon become source-starved. Current 10-m class single dishes, with their limited field of view, spatial resolution, and sensitivity, can only reveal the ‘tip of the iceberg’ of the (sub-)mm source population, both for Galactic and extragalactic studies. These limitations cannot be compensated for by interferometers, which are all intrinsically affected by a low mapping speed and by the loss of diffuse extended signals. 

The Atacama Large Aperture Submillimeter telescope (AtLAST) is a concept for a 50m -diameter single dish observatory to be built in the Chilean desert. With its extremely large field of view (1- 2 degrees diameter), spatial resolution (up to ~1.5” at 350 μm), and sensitivity to both point sources and large-scale structures, AtLAST will be transformational for all fields of Astronomy in the 2030s.  I am the Coordinator of a collaborative Horizon2020 project which by the end of 2024 will deliver a comprehensive design study for AtLAST.  To know more about the design study, and read relevant articles and publications, visit the AtLAST website.

Selection of AtLAST-related publications (full list available at this link):

Science drivers:

Telescope design:

Properties of cold gas and dust in local (ultra) Luminous Infrared Galaxies

One of my main areas of research is the study of local (U)LIRGs. In these sources, the enhanced star formation and AGN activity generate the most massive, extended and energetic multi-phase outflows known. In addition to outflows, the dislocation of gas due to the gravitational interaction and tidal forces make these galaxies very interesting targets for studying extended circumgalactic medium reservoirs. 

Recent related publications:

ALMA CO(2-1) image and spectra showing the extended and massive molecular outflow in NGC6240 (Cicone et al. 2018, ApJ)

The baryon cycle in high-redshift active galactic nuclei

The SINFONI survey for unveiling the physics and effect of radiative feedback (SUPER, PI: Mainieri) is an ESO large program at the very large telescope (VLT). As part of SUPER, we have  obtained high-resolution, spatially-resolved spectroscopic observations of multiple optical emission lines (Hb, [OIII], Ha) for a statistically-significant sample of ~40 active galactic nuclei at z~2.  The main goal of SUPER is to probe the baryon cycle and the effects of AGN feedback at the peak epoch of AGN activity and cosmic assembly, in a sample probing four orders of magnitude in AGN luminosity. Most of the SUPER sample has been observed also at sub-millimetre and millimeter wavelengths with ALMA and APEX.  For an updated list of publications, check the SUPER website.

Recent publications:


The APEX low-redshift legacy survey for molecular gas (ALLSMOG, PI: Wagg) is a large ESO observing program aimed at constraining the molecular gas content of ~100 nearby star forming galaxies through the carbon monoxide (CO) emission line.  ALLSMOG is the first large systematic extragalactic survey of CO ever conducted with the Atacama pathfinder experiment (APEX) telescope. APEX is located on the Chajnantor plateau at 5000 meters above sea level, in the Chilean Andes. The final data release comprises APEX CO(2-1) emission line observations of 88 low-mass (108.5<M [M] < 1010) star-forming galaxies, and IRAM 30m observations of the CO(1-0) and CO(2-1) emission lines in additional nine galaxies with M< 109M. ALLSMOG allows us to probe the molecular gas content of more typical and lower stellar mass galaxies than have been studied by previous extragalactic CO surveys. The reduced data products are public and can be retrieved through the ESO Phase 3 archive query.  For additional info check the ALLSMOG website

Recent publications:

Scaling relations between the molecular gas content - as traced by Carbon Monoxide emission - and galaxy properties, for a statistically significant sample of local star-forming galaxies from the ALLSMOG and COLDGASS surveys (Cicone et al. 2017, A&A).

From dual to binary super massive black holes

With collaborators from INAF and other Italian institutions we are conducting pilot studies and observations aimed at identifying binary and dual AGN candidates, in preparation for future studies with e.g. MAORY+MICADO (PI: Severgnini). MAORY is the Adaptive Optic (AO) module that will be installed at the E-ELT at the first light of the telescope. The MAORY science cases white book is available at this link.

Selected publications:

Identification of high-redshift radio-loud AGNs 

As members of the Large Synoptic Survey Telescope (LSST) consortium, the Observatory of Brera is developing the skills to exploit the LSST database to perform a statistical study of the quasar population in the first billion years of the Universe. By exploiting the currently available multi-wavelength databases, our group has already successfully identified a large sample of previously unknown radio-loud AGNs at z>5.  We are now in the process of obtaining follow-up observations to confirm the redshifts and constrain the physical properties of these sources.

Recent publications: