Group Members & Collaborators
Joseph Caruana (Group leader)
Joseph’s research interests lie in galaxy formation and evolution, reionisation, galactic dynamics, light pollution, and applications of physics to hyperbaric medicine.
Karl Fiteni (PhD student)
Karl read for a B.Sc. (Hons.) in Physics and Mathematics at the University of Malta. For his final year project Karl carried out photometric measurements of variable stars. Following this, he pursued an M.Sc. in Galactic Dynamics with the Institute of Space Sciences and Astronomy (ISSA) at the University of Malta. Karl is currently working on his PhD in Galactic Dynamics at ISSA.
Ryan Vella (PhD student)
Ryan Vella read for a B.Sc. (Hons.) in Physics and Mathematics at the University of Malta. His final year project involved the mapping of the night sky brightness (NSB) over the Maltese Islands. The first ground-based high-resolution map of the NSB over the Maltese archipelago was presented in Caruana et al. (2020). In 2019, Ryan completed his M.Sc. in Geosciences (UM). Ryan is now working for the European Space Agency (ESA) as a Maltese National Trainee. He is about to start his PhD at the Max Planck Institute for Chemistry in Mainz, Germany. Ryan continues to work with our group on projects relating to dark skies and light pollution.
Victor Debattista (Collaborator at UCLan)
We closely collaborate with the research group of Prof Victor Debattista at the University of Central Lancashire. Click here to visit the website of Prof Debattista’s group.
Lisa-Marie Aquilina (student)
Lisa Maria is an undergraduate student, currently engaged in a project in astrophysics with our group.
Former Group Members
Christina Julia Pisani (2019-2020)
Daniel Spiteri (2019-2020)
Galaxy Formation & Evolution and Reionization
One of my main research interests lies in galaxy formation and evolution, in particular the observational study of galaxies in the early universe (z > 7). A lot of my work has involved designing, undertaking and analysing follow-up spectroscopic surveys of high-redshift candidate galaxies.
At such high redshifts, a particularly useful emission line is Lyman alpha. This emission line can be used to gain a lot of information about these objects, including confirmation of their redshift.
For objects lying at such large distances, the Lyman-alpha line is redshifted to the infrared region of the electromagnetic spectrum. In analysing this data, where any potential signal is very faint and the infrared background sky varies a lot over short time-scales, a lot of effort goes into developing optimal data reduction techniques.
These galaxies are viewed at a time before the “fog” of neutral hydrogen has been cleared, so these galaxies are used as probes of the ionization state of the universe during its infancy. Of particular interest is the question of whether these first objects provided sufficient photons to reionize the universe.
Some of our inferences about the universe at high redshift base upon extrapolations from lower redshifts, such as the fraction of Lyman alpha emitters in the z=3-5 universe; to this end I have also carried out work studying galaxies in this redshift range.
The observatories I use for this work are both space-based, e.g. the NASA/ESA Hubble Space Telescope, and ground-based. For my spectroscopic studies, I have been using various spectrographs installed on ground-based observatories to carry out long-slit, cross-dispersed, multiple-slit, and multi-object IFU spectroscopy. These instruments include:
We use computer simulations to understand various processes in galaxies, and compare these to data obtained with the ESA space-observatory Gaia. Data from Gaia enables astronomers to create a 3D map map of the Milky Way via highly accurate positions and radial velocities for a billion stars.
I serve as a management committee member representing Malta on the MW-Gaia COST Action.
I have a strong interest in the study of light pollution. Beside the obvious implications for astronomy, I am interested in its effects upon ecology and human health.
The night sky brightness resulting from anthropogenic lighting is a global problem that is under increasing scrutiny, as a clearer picture is emerging of artificial lighting’s pollutant attributes, revealing that it can be harmful and disruptive in myriad ways.
For a number of years I have been leading a research effort into mapping the night sky brightness of the Maltese Islands, recently publishing one of the highest resolution maps ever undertaken in a study of this kind.
In addition to my research in astrophysics, I am also interested in topics of hyperbaric medicine, an interest that stems from my own technical diving with SCUBA and rebreathers. In particular, I employ mathematical models and statistical methods in applications to decompression theory and prevalence of decompression illness. For this work, I collaborate with the Hyperbaric Unit at Mater Dei hospital (Malta’s acute general teaching hospital).