ESO Scientific Staff in Santiago/Chile
- Faculty & Scientists
- Fellows
- Fellows Hosted outside ESO
- Paid Associates
- Unpaid Associates
- Students
- Support Staff
GAR = Garching; LS = La Silla; PAO = Paranal; SCV = Science Vitacura
See also the ESO Garching Staff and Research page for scientific staff in Garching.
Also available is a List of the Astronomers and Astronomical Institutes in Chile.
Faculty & Scientists
Joseph Anderson |
Joseph Anderson is an ESO support astronomer and currently FORS2 instrument scientist. He obtained his PhD in astronomy at the Astrophysics Research Institute at Liverpool John Moores University in the UK, in 2009, investigating the parent stellar populations of supernovae under the supervision of Phil James. Joseph then moved to a postdoc position at the Universidad de Chile, Chile, working with Mario Hamuy. He joined ESO at first as a fellow in 2013. Hi main research interests are the study of supernovae of different types, with a focus on investigating the progenitor and explosion characteristics of type II supernovae through analysing their observed diversity. He also spends a significant amount of time analysing supernova host galaxy and environment properties in order to constrain progenitor properties while also learning about star formation processes within galaxies. |
Fuyan Bian |
Scientific interests:
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 Stephane Brillant (PAO/SCV) |
Stephane Brillant is an Operations Astronomer at the Paranal observatory. He received his PhD in physics from the University of Paris XI in 1999. After 2 years as a student in ESO during his PhD he came back in 1999 as a fellow and moved in 2001 to his current position in Paranal. While his PhD was more in theoretical physics, he moved to more observational study and has been working mostly on extrasolar planet using various technics including microlensing. He is now working mostly on the study of the atmosphere of extrasolar planet using in particular CRIRES to study their chemical composition. |
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Itziar de Gregorio-Monsalvo is the Head of the Office for Science in Chile from November 2018. Before she was the Head of the ALMA Program Management group. She did her PhD in the Spanish National Institute for Aerospace Technology, using the NASA Deep Space Network antennas to set up Radio Astronomy observations and perform star formation studies at centimeter wavelengths. She joined ESO in 2006 as an ESO ALMA fellow with duties at the APEX telescope, the Atacama Test Facility (in Socorro, New Mexico), and the Operations Support Facilities near San Pedro de Atacama. She became an ESO Faculty member in 2010, working as an ALMA Science Operations Astronomer. Her main research activities are focused in star and planetary formation, in particular:
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(PAO/SCV) |
Willem-Jan de Wit is a VLTI support astronomer. His scientific interest is star formation and in particular the formation of massive stars. With the VLTI, he studies the harsh environment of the immediate vicinity of massive stars during their assembly process. His research involves the properties of young stellar clusters and how they relate to the character of massive star formation in Galaxies. He received his PhD from the University of Utrecht in 2001. Scientific interests:
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 Bill Dent (JAO/SCV) |
Bill Dent joined ESO in 2008 as a System Astronomer for ALMA. He obtained his PhD from the University of Kent, then worked at NASA MSFC, before moving to the JCMT as a support astronomer. He then alternated between Hawaii and UKATC Edinburgh, working mostly on support of JCMT observers and heterodyne instrumentation. Before moving to ALMA, he worked at the UKATC on studies for new IR & sub-mm instrumentation. His main research interests are in star & planet formation, particularly debris disks, protoplanetary disks and IR/submm spectroscopy. |
Pedro Figueira |
Pedro Figueira is an ESO Staff Astronomer since February 2018. His research focuses on Extrasolar planet detection and characterization, and on the development of dedicated instrumentation for this purpose. He obtained his Ph.D. from University of Geneva in 2010, under the supervision of Michel Mayor and Francesco Pepe. Specializing first on near infra-red spectroscopy and on precise radial velocity measurements in the nIR, Pedro has been working on the characterization of both the stellar signals and the minute signatures of low-mass planets. After having worked at Centro de Astrofísica da Universidade do Porto and Institute of Astrophysics and Space Sciences, in Portugal, Pedro comes to ESO to work with instruments he helped to develop, such as ESPRESSO or NIRPS. He likes Lindy Hop and craft beer. |
Boris Haeussler |
Boris Häußler (Haeussler) is an ESO staff astronomer at Paranal as of November 2015. Born in Karlsruhe, he received his Ph.D. in 2007 from the University of Heidelberg in Germany (PhD thesis at MPIA). He then moved to Nottingham, UK for 2 consecutive 2 postdoc positions and, after another postdoc in Oxford (while also being associated with Hertfordshire), he moved to ESO/Santiago to work at Paranal Observatory. His research interests are:
Evolution of galaxies |
George Hau |
George Hau received his Ph.D. from Cambridge University in 1998. After postdoctoral positions at P.U. Catolica, ESO (as Fellow), Durham and Swinburne, George returned to ESO as Operations Staff Astronomer in 2010, supporting the adaptive optics effort at ESO. George has broad interests on extragalactic astronomy, the topics include:
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Xavier Haubois |
Xavier Haubois is the VLTI System Scientist at Paranal Observatory since December 2016. Xavier was previously a Fellow since October 2014. He got his PhD in 2009 at Observatoire de Paris that was focused on infrared interferometric imaging of evolved stars and the design phase of GRAVITY. After his thesis, he obtained a post-doctoral contract at the University of São Paulo (IAG) to work on the modelling of circumstellar environments and at the University of Sydney to deepen his skills in optical interferometry. His research focuses on mass-loss processes in evolved stars observed at high angular resolution. His research interests are:
Stellar Structure and Evolution |
Pascale Hibon |
Scientific Interests:
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 Andreas Kaufer (PAO/SCV) |
Andreas Kaufer is the Director of the La Silla Paranal Observatory. He received his degree in Physics from Heidelberg University in 1993. In 1996 he graduated with a PhD in Astronomy from the same university. He became ESO staff member in 1999 and joined the VLT Science Operations department. He has been the Paranal instrument scientists of UVES and later FLAMES. In 2003 he became the instrumentation scientist of the La Silla Paranal Observatory. His research activities focus on the fields of stellar astrophysics, galaxy evolution, and state-of-the-art astronomical instrumentation. |
 Thomas Klein (APEX - Scientist) |
Thomas Klein is the Head of the APEX telescope facilities on Chajnantor and Sequitor. In 1996 he received his degree in Physics from the University of Bonn where he also graduated with a PhD in Astronomy in 1999. Since then he was a staff scientist at the Max-Planck Institut fuer Radioastronomie, where he focused his interests on the development of THz instrumentation for astronomy and accumulated a strong background on submillimeter observing techniques at various telescopes. In 2000 he started his involvement in the HERSCHEL/HIFI project as the lead system engineer for the HIFI local oscillator system. Until the end of the HIFI mission, in April 2013, he supported HIFI’s Instrument control center. In 2007 he became the group leader of the MPIfR’s heterodyne submillimeter technology group, developing the institute’s PI instrumentation for APEX and SOFIA. Since 2008, he was a frequent guest scientist at APEX, accompanying the PI instruments of the MPIfR, before he joined ESO and APEX in September 2013. |
Ruediger Kneissl |
Rüdiger Kneissl joined ESO in 2009 as Science Operations Astronomer in the ALMA project. He received his PhD from the University of Munich and the Max-Planck-Institute for Astrophysics in 1997. During appointments at the University of Cambridge, UC Berkeley and MPI for Radio Astronomy in Bonn he worked with various radio interferometers and the APEX telescope. He has also been involved in the Planck satellite mission for many years. His main scientific interest is in
Cosmology and the Early Universe |
 Cédric Ledoux (PAO/SCV) |
Cédric Ledoux is a support astronomer at the Very Large Telescope on Paranal. His main research interests include the properties and evolution of galaxies as revealed by QSO absorption-line systems, the study of metals, dust and molecules in the interstellar medium of high-redshift galaxies, the distribution and physical properties of the gas in and around the host galaxies of Gamma-Ray Bursts, and the detection of galaxies in emission up to the highest redshifts. He is deeply involved in the operations of the Ultraviolet and Visual Echelle Spectrograph (UVES) and is currently the instrument scientist of the Echelle Spectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO). Evolution of Galaxies and the ISM; Cosmology and the Early Universe |
 Stéphane Leon (JAO/SCV) |
Stéphane Leon Tanne is System Astronomer at ALMA. He received his PhD from the University Paris 7 in 1998. His main interests are the effects of the environment on stellar systems. He studied the tidal tails in globular clusters using wide field telescopes and numerical simulations. While he was working at IRAM (Spain) he studied the dynamics of the molecular gas in galaxies using single-dish and interferometer telescopes. Since his post-docs at ASIAA (Taiwan) and at the Instituto de Astrofísica de Andalucía (Spain) he works actively on the ISM content of radio galaxies, barred and isolated galaxies. |
Gaspare Lo Curto |
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 Gianni Marconi(ESO/EASC) |
Gianni Marconi is Commissioning Scientist of the ALMA Observatory (Array Group lead). He received his degree (cum Laude) in Astronomy from Bologna University in 1987. In 1991 he graduated with a PhD in Astronomy from the same university. From 1994 to 2005 he held an assistant professorship and was member of the Director Board at the Observatory of Rome. In 1999 he became ESO staff member and joined the VLT Science Operations department. He has been the Paranal instrument scientists of VIMOS between 2002 and 2005. From 2006 to 2010 he has been the Instrumentation Operation Teams Coordinator of the La Silla Paranal Observatory. From 2010 he has been seconded to the JAO office for the commissioning of ALMA. Starting in June 2010 has been appointed as Commissioning Scientist for the European Alma Support Center (EASC) and in charge of the integration and verification of the development projects for ESO in ALMA. His main research activities focus on the fields of stellar astrophysics, star formation history and chemical evolution of galaxies, and state-of-the-art astronomical instrumentation and telescopes. Scientific interests:
Stellar populations; Evolution of Galaxies and ISM
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Christophe Martayan |
Christophe Martayan joined ESO in 2009 as Paranal support astronomer and will be FLAMES instrument scientist. He received his PhD in Physics-astrophysics from Paris XI University and Meudon Observatory, France in 2005. By after he was employed at the ESO-Garching, the Paris Observatory, and the Royal Observatory of Belgium. He worked as manager of modules for the scientific preparation of the GAIA space mission, and on the analysis of million of spectra taken with the ESO-WFI in its slitless mode. His current research activities concern the stellar evolution of massive and emission-line stars (O, B, Be, LBV, GRB) in different environments of metallicity (Milky Way, Magellanic Clouds, etc). He is also involved in the GAIA space mission about emission-line stars and in the scientific preparation of a multi-object spectrograph for the E-ELT. |
Sergio Martin |
Scientific Interests:
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 Gautier Mathys (JAO/SCV) |
Gautier Mathys is Lead Astronomer of the Proposal Handling Team. He obtained his PhD in Physics in 1983, and his Habilitation in 1990, both at the University of Liege. After 8 years in Switzerland (first at the ETH in Zurich, then at the Geneva Observatory), he moved to ESO-Chile in 1991, where he worked as support astronomer at the La Silla Observatory and, as of 1998, at the Paranal Observatory; in particular he was Head of Science Operations from 1999 to early 2006. From 2006 to 2011, he was Head of ESO's Observing Programmes Office, in charge of the support of the observing proposal selection process. His main research interests are stellar magnetic fields and stellar pulsation, with particular emphasis on the chemically peculiar A- and B-type stars. |
Andrea Mehner |
Stellar Structure and EvolutionScientific interests:
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Jorge Melnick was the VLT Programme Scientist. His research interests include violent star formation, galactic and extragalactic starbursts and the evolution of massive stars. |
Claudio Melo |
Claudio Melo is the ESO Representative in Chile from April 2018. Before he was the Head of the Office for Science in Chile. His main interests focus in finding planets in different environments such as open clusters, metal poor stars and young stars. From the technical point of view, Claudio is familiar with high-precision radial velocity measurements and interested in how to overcome the different sources of noise to reach the 10cm/s precision with ESPRESSO and eventually to find an exo-Earth. For the coming years, he is willing to develop new projects in the field of Astrobiology. |
Steffen Mieske |
Steffen Mieske is the Head of Science Operations at Paranal. He obtained his PhD in astronomy in 2005 from Bonn University. Between 2000 and 2004 he spent about 3 years in Chile at PUC, pursueing research for his Master's and PhD theses. In 2005 he joined ESO as a fellow in Garching and moved to ESO Chile in August 2008 as Staff Astronomer. Steffen has acted as instrument scientist of OmegaCAM and VIMOS, and was Deputy Head of Science Operations between 2014 and 2015 before moving to his current position in July 2015. His scientific interests comprise the high-mass end of the globular cluster population and ultra-compact dwarf galaxies (UCDs), and generally the internal dynamics of compact stellar systems. Recently he has focused in particular on the search for super-massive black holes in UCDs. Steffen is also interested in ensemble properties of dwarf galaxies, such as their scaling relations, luminosity function, internal kinematics and stellar populations. During his PhD time, he studied the shape of the Hubble flow in the "Great Attractor" region. |
Julien Milli |
Julien Milli is the Paranal Adaptive Optics (AO) scientist as of November 2016. He obtained his PhD in 2014 from the Institute of Planetology and Astrophysics of Grenoble (IPAG) after spending 2 years at ESO Santiago with the studentship program. He was a fellow at ESO with duties in Paranal on UT3 from 2014 to 2016. He uses adaptive optics and high-contrast imaging techniques to reveal the circumstellar environment of stars. His main interest focuses on debris disk: their formation, evolution and the characterisation of the dust properties. His main achievements include the characterisation of the debris disk around beta Pictoris and HR4796. He is also interested in instrumentation for adaptive optics and develops algorithms to reduce high-contrast data. |
 Francisco Montenegro (APEX/SCV - Scientist) |
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Juan Carlos Muñoz |
Juan Carlos Muñoz Mateos is a Paranal Operations Staff Astronomer. He is mainly interested in galaxy formation and evolution, as well as the physics of the interstellar medium. He completed his PhD in 2010 at Complutense University in Madrid, Spain. In his thesis he worked extensively with UV, optical, IR and radio data to map the distribution of stars, gas and dust in nearby galaxies, and used that information to constrain the past assembly and evolution of galaxies. He then moved as a postdoc to the National Radio Astronomy Observatory in Charlottesville, USA, where he worked within the Spitzer Survey of Stellar Structure in Galaxies (S4G). He led and developed the S4G surface photometry pipeline, and used the S4G data to investigate how features such as bars and spiral arms can drive stellar migration in galaxies. He now plans to exploit ESO's existing and upcoming instruments to further pursue his research on galaxy assembly at different redshifts. |
 Lars-Åke Nyman (APEX/SCV - Scientist) |
Lars-Åke Nyman is the APEX Station Manager. His research interests include the study of circumstellar envelopes around evolved stars, star formation and the large scale distribution of molecular clouds and star forming regions in the Milky Way. |
Claudia Paladini |
Claudia Paladini is Operations Staff astronomer at the Paranal Observatory. Scientific Interests:
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 Rodrigo Parra (APEX/SCV) |
Rodrigo Parra is a staff astronomer at the APEX project. He obtained an Electrical Engineering Degree at Universidad Tecnica Federico Santa Maria and a MSc in Microwave Digital Communications Systems at Chalmers University. Subsequently, he received a PhD in Radio Astronomy from the Onsala Space Observatory. He has a strong background in both single dish and interferometric observational astronomy at cm/mm/submm wavelengths. He is expert in holographic techniques (used to assess and maintain the APEX main dish surface accuracy) and development and implementation of telescope pointing models. Scientific interests:
Evolution of Galaxies and the ISM |
Juan-Pablo Pérez-Beaupuits |
Juan-Pablo Pérez-Beaupuits is an APEX Staff Astronomer since August 2015. He obtained an Electrical Engineering Degree at Universidad de Chile and a MSc in Space Science and Radio Astronomy at Chalmers University of Technology, Sweden. Subsequently, he received his PhD from the University of Groningen, The Netherlands, in 2010, working on the chemical fingerprints of star-forming regions and active galaxies (https://www.rug.nl/research/portal/publications/chemical-fingerprints-of-star-forming-regions-and-active-galaxies%28116b82be-bff3-4b4c-ae97-d6d7ec15b6b7%29.html). Scientific interests:
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 Emanuela Pompei (PAO/SCV) |
Emanuela Pompei is working as FORS and NACO instrument scientist at the Paranal La Silla Observatory. She obtained her PhD from University of Trieste in Italy in 1999 and joined ESO the same year. She has worked both on La Silla and on Paranal as Boller&Chivens, DFOSC, FEROS, EMMI- NTT, MUSE and HAWK-I instrument scientist, WFI, EFOSC2 , KMOS, SINFONI support astronomer. |
 Thomas Rivinius (PAO/SCV) |
Thomas Rivinius has studied at the University of Heidelberg, where he got his PhD in 1998. After three years of ESO fellowship in Garching he returned to Heidelberg to become "Privatdozent". Since 2005 he's back at ESO, this time in Chile as science operations support astronomer on Paranal at the VLTI. Currently, he's the intrument scientist for MIDI. His research focusses on hot stars and their circumstellar environments, covering stellar pulsation, hot star winds, magnetic O and B-type stars, and Be stars and their disks. |
Florian Rodler |
Florian Rodler is an ESO Staff Astronomer at the Paranal Observatory since September 2016. Already as kid he was fascinated by the stars and the universe; he decided to make his dream come true and studied Astronomy at the University of Vienna, Austria. In 2008, Florian obtained his PhD degree at the University of Vienna with a thesis on atmospheric properties of giant exoplanets. After his PhD he spent five years in Spain, working in Tenerife and Barcelona. In 2013, he joined the Harvard-Smithsonian Center for Astrophysics in Cambridge, USA. In 2014, he was awarded the Alexander-von-Humboldt fellowship at the Max-Planck-Institute for Astronomy in Heidelberg, Germany.
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Eleonora Sani |
Eleonora Sani joined ESO as a Staff Astronomer in March 2015. In 2009 Eleonora obtained her PhD degree at the University of Firenze, Italy, with a thesis on the connection and energetic balance between active galactic nuclei (AGN) and star formation in active galaxies both in the local Universe and at high redshift. For this purposes she adopted a multiwavelenght approach, spanning from the X-rays to the sub-mm frequencies, and developed new diagnostic diagrams. Part of this work was developed at the Max Planck Institute fuer Extraterrestrische Phisik in Munich, Germany, institute that she visited again during her first postdoc. She passed the last 3 years working for the LBT italian community as a support astronomer and executing observations at the telescope. Currently the main research interests span from the feeding/feedback mechanisms in local AGN, to the black hole-bulge scaling relations, till the evolution and role of AGNs on protoclusters. |
 Ivo Saviane (LSO) |
Ivo Saviane has been in its position as La Silla Site Manager officially since October 2013. However, his history at ESO commenced about 12 years ago. That is when he first came to ESO, to join a Fellowship programme at La Silla that lasted three years from 2001 to 2003. Right after that he became an Operations Staff Astronomer at La Silla, starting a steady career closely related with the site. Among other positions at La Silla, he has been at various times Instrument Scientist of FEROS, TIMMI2, EMMI, and EFOSC2, and he became Head of Science Operations in 2008. After moving to Paranal as an Operations Staff Astronomer, he became Instrument Scientist of FORS2 and later KMOS. |
Luca Sbordone |
Luca Sbordone joined ESO in June 2016 as a Staff Astronomer. He obtained his PhD in Astronomy from the University of Rome “Torn Vergata”, Italy, in 2005. Subsequently, he was part of the CIFIST Marie Curie Excellence Team at Paris Observatory, France, and held postdoc positions at Max Planck Institüt für Astrophysik, Munich, Germany, Landessternwarte Heidelberg, Germany, and Pontificia Universidad Catolica de Chile. His main research interests are the chemical analysis of cool stars in the Milky Way and Local Group (LG) galaxies, and the modeling of cool stars atmospheres. He is particularly interested in the chemical composition of LG dwarf Spheroidal galaxies and associated tidal streams, the characterization of multiple populations in globular clusters, the evolution of Lithium, and the search and characterization of extremely metal-poor stars. He is also an expert in the development and deployment of fast automatic codes for the determination of stellar atmospheric parameters and chemical abundances in large spectroscopic samples, and in the production of large libraries of synthetic stellar spectra. He is Second Instrument Scientist for X-Shooter. Observationally his main tools are intermediate- and high-resolution optical and infrared spectroscopy. |
 Linda Schmidtobreick (PAO/SCV) |
Linda Schmidtobreick is currently working on Paranal as instrument scientist for KMOS as well as support astronomer for UT1, UT3, and VLTI. In the past, she has been instrument scientist of EFOSC at La Silla and ISAAC at Paranal and coordinator of the TrainDoc and GenOps groups. During the early years of her career she worked on interplanetary astronomy, studying comets, the Zodiacal light, and the Gegenschein. For her PhD (1997 at the Ruhruniversitaet Bochum, Germany), she studied the Galactic structure in the UV and later expanded that also to other galaxies using surface photometry and stellar population synthesis methods. She took postdoc positions in Bochum, the MPIA in Heidelberg, and the Osservatorio Astronomico di Padua, Italy. In 2001, she started as an ESO fellow on La Silla, and in 2005 got her current staff position. By now, Linda is mainly working on compact binaries, i.e. cataclysmic variables. She is interested in the physical evolution of these systems, the nova-binary connection, and the physics of the accretion disc. In addition, she likes teaching and to work with students and spends a large fraction of her time on public outreach. |
 Fernando Selman (PAO/SCV) |
Fernando Selman's current observational research interests include studies of the nature of the stellar IMF, and the dynamics and binary content in 30 Doradus using SINFONI, and the physics of medusa galaxies studied with MUSE. On a larger scales he iinterested in the intergalactic light in clusters of galaxies. On a theoretical side he is interested in the dynamics of gravitational systems with particular attention to the phenomenon of dynamical friction. As an observatory astronomer, he has been instrument scientist for the Wide Field Imager (WFI) at La Silla, and HAWK-I, VIMOS, and OmegaCam at Paranal. He is currently the instrument scientist for MUSE at Paranal. He started his career as a physics student at the School of Engineering of Universidad de Chile subsequently obtaining his PhD at Caltech in 2004. During his strongly acausal career he was Fulbright Travel fellow, Carnegie-Chile Fellow, and Beatrice Watson Parrent postdoctoral fellow. |
Karleyne Silva |
Scientific Interests:
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Giorgio Siringo |
Giorgio Siringo joined ESO in September 2009 as Operations Staff Astronomer at APEX. In June 2012 he moved to the Joint ALMA Observatory (JAO) as Test Scientist. Since September 2013 he works at JAO as Senior RF Engineer and Front-End Technical Lead within the Engineering Services Group.
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 Alain Smette (PAO/SCV) |
Alain Smette is a VLT operations Staff Astronomer. Following studentships at ESO-Garching and La Silla, he received his PhD from the Universite de Liege, Belgium, in 1994. He was a Post-Doc at Kapteyn Institute, Groningen, and a research associate first at the NASA-Goddard Space Flight Center, in the STIS team, then back in Liege. His research interests mainly include the study of absorption lines in the spectra of quasars and gamma-ray burst optical afterglows, gravitational lensing and AGN. He is the instrument scientist of CRIRES. |
Jonathan Smoker
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Jonathan Smoker is a VLT Operations Staff Astronomer and the instrument scientist for CRIRES (previously FLAMES and UVES). He obtained his PhD from Manchester University (Jodrell Bank), England in 1993 studying low surface brightness dwarf galaxies in HI and the optical, before moving on to be a computer systems administrator at the Royal Greenwich Observatory and IoA, Cambridge. After that came a 4-year stint as a postdoc at Queen's University, Belfast, Ireland, then 3 years at ESO Chile which he left in 2005. He is now back at the VLT, working on high velocity clouds, tiny-scale structure in the interstellar medium, the Magellanic system and some work on supernovae, B-type and Post-AGB stars. |
 Thomas Szeifert (PAO/SCV) |
Thomas Szeifert is support astronomer at the VLT since 1999. Before he was working for the FORS instrument consortium at the observatory in Heidelberg. He has been instrument scientist at Paranal for the FORS optical multi-mode instrument and the SINFONI near-IR adaptive optics integral field spectrograph. His primary fields of research are the study of long-term wind variability of Luminous Blue Variables and other massive hot stars and stellar abundance studies in the Galaxy and local group galaxies. He obtained his PhD in 1995 at the Heidelberg University for his work on Luminous Blue Variable Stars in the Magellanic clouds, M31 and M33. |
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Astronomer Emeritus |
Karl Torstensson |
Scientific interests:
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Konrad Tristram |
Konrad Tristram is an operations staff astronomer at Paranal. He received his PhD in 2007 from the University of Heidelberg, Germany, where he started his investigation of active galactic nuclei (AGN) at highest angular resolutions. After his PhD he moved to Bonn becoming an interferometry specialist. He joined ESO in April 2014 in order to support the interferometric effort at Paranal. He continues working on the dust and gas surrounding the supermassive black holes in AGN. Driven by his science, he holds a special interest in high angular resolution imaging and spectroscopy as well as in infrared & submm interferometry. Since 2015, he is the instrument scientist of VISIR. His research interests are:
Evolution of Galaxies and the ISM |
Eric Villard |
Eric Villard is a System Astronomer on ALMA. He joined ESO in January 2010, after obtaining his PhD at Service d'Aéronomie du CNRS (near Paris) in 2008. While at Service d'Aéronomie, he also worked on the science operations of the European Venus Express mission, in particular the SPICAV instrument. His main research interest is the study of planetary atmospheres at various wavelengths. Other research interests include astrometry, the study of comets, exoplanets and galaxy evolution (bars).
Planets and Star Formation
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Zahed Wahhaj |
Zahed Wahhaj joined ESO as a VLT astronomer in 2012, as one of the instrument scientists for the exoplanet imager, SPHERE. He is interested in the direct-imaging and characterization of exoplanets, brown dwarfs and circumstellar debris disks. Before joining ESO, he was a core team member of the Gemini NICI Planet-Finding Campaign, a direct-imaging search for giant planets around 300 nearby young stars, at the University of Hawaii. He was also involved in the Cores-to-Disks Spitzer Legacy Program (2003-2006), where he worked on understanding weak-line TT stars, through the evolution of their mid-infrared (MIR) disk emission. His dissertation work was on planetary signatures in debris disks. This involved Keck high-resolution MIR imaging and Bayesian modeling of the dust disks around Beta Pictoris, HR 4796A and 49 Ceti. Zahed Wahhaj received his PhD in Physics and Astronomy from the University of Pennsylvania, Philadelphia in 2005.
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Bin Yang |
Bin Yang is an ESO staff Astronomer with duties at the VLT since December 2016. She received her PhD from the University of Hawaii in 2009, where she studied the physical properties of Solar System small bodies (e.g. asteroids and comets) using various facilities atop Mauna Kea. She joined ESO at first as a science fellow in 2013. She is interested in the formation of planetary systems, particularly the formation and evolution of our own solar system. Her other interests include Extreme Adaptive Optics, High-contrast Imaging and Astrobiology. |
Trystyn Berg |
Scientific Interests:
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Jesus M. Corral-Santana |
Jesús Corral-Santana is an ESO Fellow with duties in Paranal since October 2016. Jesús received his PhD in Astrophysics at the Instituto de Astrofísica de Canarias (IAC) and the University of La Laguna (ULL) in the Canary Islands (Spain) in 2012, working in the X-ray binaries group leaded by Jorge Casares. After his thesis, he moved to Chile as a FONDECYT Fellow at the Pontificia Universidad Católica de Chile where he worked with Franz E. Bauer. His main research topic is the study of stellar-mass black holes in X-ray binaries and, in particular, those found in X-ray transients. One of his main goals is to dynamically confirm the presence of black holes (using optical and near-infrared photometry and spectroscopy) in order to increase the currently scarce sample of black hole transients, which is essential to understand several aspects of physics and astrophysics such as, for instance, the final stages of stellar evolution, supernovae explosions and the formation of compact objects. In addition, he is a member of the VVV and EGAPS (IPHAS, UVEX and VPHAS+) surveys performed, among others, with the VISTA and VST telescopes. Scientific interests:
Stellar structure and evolution |
Bruno Dias |
Bruno Dias is an ESO fellow with duties in Paranal since July 2015. He is the instrument fellow of FORS2 and operates UT1, that includes FORS2, KMOS, and NACO. He received his PhD from IAG - Universidade de São Paulo, in Brazil in 2014, with a prize of best thesis of the year from the same institute. During the PhD he was granted an ESO studentship for one year in Chile. Before coming back to ESO he was a post-doc at Durham University, UK. His main science interests involves stellar clusters and stellar populations to understand stellar and galaxy evolution in the Milky Way and Magellanic Clouds. He has experience on spectroscopy and photometry that is applied to his work on FORS2. He is also a member of the spectroscopic survey GOTHAM and the photometric surveys VVV and VISCACHA. Scientific Interests:
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Alexandre Gallenne |
Scientific Interests:
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Marie-Lou Gendron-Marsolais |
Scientific Interests:
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Johanna Hartke |
Scientific Interests:
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Ruben Herrero-Illana |
Rubén Herrero-Illana is an ESO fellow with duties at ALMA. He obtained his PhD in 2014 at the Instituto de Astrofísica de Andalucía (IAA-CSIC), in Granada, Spain. He is mainly interested in luminous and ultraluminous infrared galaxies from a multi-wavelength perspective. He studies them at different spatial scales, from their overall gas structure as traced by mm observations, to their innermost regions using high-resolution NIR data and radio interferometric observations. In particular, he is focused on their star formation properties and on the connection between the AGN and the starburst processes. After his first postoc, also at the IAA-CSIC, he started to work at ESO in September 2016. |
Matias Jones |
Scientific Interests:
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Darshan Kakkad |
Scientific Interests:
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Chiara Mazzucchelli |
Scientific Interests:
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Hugo Messias |
Hugo Messias is an ALMA Fellow since September 2016. He obtained his PhD in 2011 at the Universidade de Lisboa, in Portugal. He went on to Universidad de Concepción, in Chile, as an ALMA-CONICyT postdoc. Before coming to ALMA, he was a FCT Fellow at Institute of Astrophysics and Space Science (Portugal) since 2014, where he was also the Lead Scientist of the Portuguese ALMA Centre of Expertise. His scientific interest are mostly related to extra-galactic astronomy: galaxy and super-massive black-hole (co-)evolution; gas content and dynamics; galaxy growth mechanisms; IR-selected AGN; distant (sub-)millimeter/radio-selected galaxies; fundamental couplings variation. |
Camila Navarrete |
Camila Navarrete is an ESO Fellow with duties in Paranal since May 2019. PhD in Astrophysics at the Instituto de Astrofísica - Pontificia Universidad Católica de Chile, in 2018, with a thesis on stellar substructures and streams in the Milky Way and Magellanic Clouds, observed from the southern Galactic hemisphere. Part of this work was developed at the Institute of Astronomy of the University of Cambridge, United Kingdom. During her PhD, she was awarded with the L'Oréal-UNESCO For Women in Science Chile Fellowship 2017. Her main research interests includes stellar substructures in the form of tidal tails and stellar streams to understand the Milky Way formation history and the role of the Magellanic Clouds, as well as the contribution from globular clusters to the assembly of the Milky Way halo. She has experience on time series observations applied in the detection of variable stars, optical and near-infrared photometry as well as low resolution spectroscopy. |
Cyrielle Opitom |
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Andrés Pérez Sánchez |
Andrés F. Pérez-Sánchez is an ESO fellow with duties at ALMA since June 2016. He graduated in Physics from the University of Antioquia, Colombia. Andrés earned his MSc in Astronomy from the Valongo Observatory-UFRJ, Brazil, and his PhD in Astronomy from the Argelander-Institute für Astronomie - Universität Bonn, Germany. His main research interests are:
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Alvaro Ribas |
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Elyar Sedaghati |
Elyar Sedaghati is an ESO Fellow with duties at Paranal since August 2017, mostly responsible for observations with UT1 of the VLT. Elyar received his PhD from Technische Universität Berlin, however the entire work was done under the supervision of Prof. Heike Rauer at DLR Berlin and Dr. Henri Boffin at ESO. His doctoral research focused on detection and characterization of Exoplanetary atmospheres with the FORS2 instrument at the VLT. His current research is in the same field of exoplanetary atmospheric studies, utilizing a variety of techniques afforded by the presence of a multitude of second generation instruments at the VLT, suited to exoplanet follow-up observations, such as ESPRESSO and CRIRES+. Additionally he works with data from space-based observatories such as the HST, as well as preparation for exoplanetary observations with the JWST. Scientific interests:
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Romain Thomas |
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Frederic Vogt |
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Chentao Yang |
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Jorge Lillo Box |
4th year at the Center for Astrobiology (CAB), Spain |
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Paulo Garcia |
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Javier Abril |
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Valentin Le Gouellec |
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Javier Minniti |
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Youssef Moulane |
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Alessandro Razza |
Alessandro Razza earned a bachelor’s degree in astrophysics from Sapienza University of Rome and completed his master’s degree studies in astronomy at Stockholm University. He is currently a PhD student at Universidad de Chile, working at ESO for a 2-year studentship since August 2017. His research focuses on the interstellar medium in supernova host galaxies, in particular on dust properties at supernovae explosion sites, from AMUSING survey of galaxies observed with IFU data from MUSE. Working on:
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Alejandra Rojas |
Alejandra Rojas Lilayú obtained her Bachelor in Astronomy and MSc in Astrophysics degrees at the Pontificia Universidad Católica de Chile (PUC), studying the nature of hard X-ray sources through optical spectroscopy and using the VVV near-IR survey. She is currently a Ph.D. Student at the Universidad Andrés Bello (UNAB, Chile), and joined ESO for a 2-year studentship since February 2017. Her research focused on the hard X-ray selected AGN properties, specifically on AGN outflows and the connection between the AGN activity and the star formation in the host galaxy. |
Cristian Romero |
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Rob Van Holstein |
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Marion Villenave |
Marion Villenave is a PhD student at Institut de Planétologie et d'Astrophysique de Grenoble (IPAG, Grenoble, France) and ESO. She is currently working at ESO Santiago with a 2-year studentship since October 2017. She graduated from ISAE-Supaéro (Toulouse, France) and holds a Master in Astrophysics from Université Paul Sabatier (Toulouse, France). Her research focuses on the evolution of protoplanetary disks with time, in order to constrain mechanisms at play.
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Sebastian Zúñiga F. |
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| Maria Eugenia Gomez Librarian |
Paulina Jiron Science Office Assistant |
Helpdesk Linux support |