I am an Instrument Project Scientist/Astronomer at the UK Astronomy Technology Centre (ATC) in Edinburgh.
I am currently one of the Instrument Scientist for Multi-Object Optical and Near-IR Spectrograph (MOONS), the next generation spectrograph for the Very Large Telescope (VLT). I am also part of the UKATC technical team developing the IR subsystem of ELT-HIRES and science Team of ELT-HARMONI.
I am leading the design of the inner Milky Way survey with VLT-MOONS, a member of the Vista Variables in the Via Lactea (VVV) photometric survey and its extension (VVV-X), member of the WEAVE low-resolution survey of the Galactic disk, and an Affiliated Principal Investigator of LSST:UK .
My research is focused on mapping the stellar population and structure of the inner Galaxy. I am currently leading several projects to place the properties of the Milky Way bulge in the general context of bulge formation by observing nearby edge-on galaxies.
I am also a strength training/powerlifting enthusiast and strong proponent of a plant-based nutrition for performance, the environment and animal welfare.
Dr. Oscar A Gonzalez
Instrument Project Scientist/Astronomer
UK Astronomy Technology Centre
Galactic Archaeology: the history of the Milky Way
The formation and evolution of X-shaped bulges
Dust extinction and the reddening law of the inner Milky Way
UK ASTRONOMY TECHNOLOGY CENTRE
As part of STFC’s National Laboratories, the UKATC is the UK’s national laboratory for the design and development of astronomical instrumentation. My primary role is to support the instrumentation projects undertaken by the lab and pursue my own research programmes.
IfA Edinburgh Visiting Fellow
UNIVERSITY OF EDINBURGH
During the 4th year of the ESO fellowship, I was hosted by the Institute for Astronomy at the University of Edinburgh with 100% research time.
ESO Postdoctoral Fellow
EUROPEAN SOUTHERN OBSERVATORY, Chile
Paranal support astronomer of UT1 (FORS2, CRIRES, KMOS, and NACO), Instrument Scientist of VIRCAM@VISTA, and Instrument Fellow of FORS2. I completed 240 nights as UT1 Support Astronomer and 40 nights as Night Shift Coordinator at the VLT
PhD in Astronomy
LUDWIG-MAXIMILIANS UNIVERSITY, Munich, Germany
Thesis title: “Unfolding the Galactic Bulge”
Advisors: Prof. Dr. Ortwin Gerhard (LMU) and Dr. Marina Rejkuba
Thesis title: “Unfolding the Galactic Bulge” (ESO)
Degree: PhD in Astronomy, Magna Cum Laude
Licenciatura (diploma) in Astronomy
P. UNIVERSIDAD CATOLICA DE CHILE
Thesis title: "Lithium rich RGB stars in the Galactic Bulge”
Advisor: Prof. Dr. Manuela Zoccali
Degree: Licenciatura (Diploma) in Astronomy, Maximum Distinction
High-resolution spectroscopy and spectral synthesis
Integral Field Unit Spectroscopy
Photometry and Image processing
IDL, R, C#, Python - Advanced
Spanish - Mother Tongue
English - Fluent
The structure behind the Galactic bar traced by red clump stars in the VVV survey
Gonzalez et al. 2018, MNRAS, 481L, 130G
We show that a secondary, fainter clump seen in the luminosity function of the galactic at low latitudes (|b|<2°) traces a spiral arm structure behind the galactic bar. This result suggests that studies aiming to characterise the bulge red-giant branch bump should avoid these low galactic latitudes and it highlights the need to include this structural component in future modelling of the Galactic bar
First stellar spectroscopy in Leo P
Evans et al. 2019, A&A, 622A, 129E
The low oxygen abundance (3% solar) and relative proximity ( 1.6 Mpc) of Leo P, a low-luminosity dwarf galaxy discovered in 2013, provides a tantalising opportunity to investigate massive stars with near-primordial compositions. Here we introduce observations of Leo P with the Multi Unit Spectroscopic Explorer (MUSE) instrument on the VLT, which have revealed its spectroscopic content for the first time.
Formation, vertex deviation and age of the Milky Way's bulge: input from a cosmological simulation with a late-forming bar
Debattista et al. 2019, submitted to MNRAS
We present the late-time evolution of m12m, a cosmological simulation of a Milky Way-like galaxy from the FIRE project. We show that the evolution of the model exhibits behaviours typical of kinematic fractionation, with a bar weaker in older populations, an X-shape traced by the younger, metal-rich populations and a prominent X-shape in the edge-on mean metallicity map, as seen in the Milky Way.