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.

Marco Berton is an Operations Staff Astronomer at Paranal Observatory, where he is currently involved in the instrument operations teams of HAWK-I and MUSE. He obtained his PhD from the University of Padova (Italy) in 2016, where he worked on the class of active galactic nuclei (AGN) known as narrow-line Seyfert 1 (NLS1) galaxies. In particular, he studied the parent population of gamma-ray emitting NLS1s, and he developed an orientation-based unification model for AGN in an early evolutionary stage. After a first postdoctoral position in Padova, he moved to Finland, working for the Finnish Centre for Astronomy with ESO at the Aalto University Metsähovi Radio Observatory. There he continued his research on the radio, optical, and X-ray properties of NLS1s. In 2021 he joined ESO at first as a fellow on UT4, working on the MUSE and ERIS instruments, before moving to his current role in 2023. 

Scientific interests: 

• AGN life cycle and feedback
• Narrow-line Seyfert 1 galaxies and their role in the unified model of AGN
• Blazars and relativistic jets

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.

Jesús Corral-Santana 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:

• X-ray binaries in optical and infrared wavelengths
• Stellar-mass black holes in transient systems
• Interacting binaries, accretion disks and black holes in general
• Stellar structure  and evolution

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: 

• Star, planets, and brown dwarfs formation
• Protoplanetary disks formation and evolution
• Jets and molecular outflows
• Astrophysical masers
• Centimeter, Millimeter and Submillimeter Astronomy: Interferometry and Single Dish techniques

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.

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 main interest lies in galaxy formation and evolution, especially how galaxies transform from the blue cloud of star-forming (disk-dominated) galaxies into the red & spheroid-dominated galaxies that populate the red sequence today. He is a member of several large collaborations (CANDELS, GAMA, VIDEO) to explore this transformation over a large fraction of cosmic time.
He is also one of the authors and the current keeper of the public GALAPAGOS code, which runs galaxy profile fitting on a large galaxy sample automatically.
This code uses GalfitM, an extended Galfit version that uses multiple images at different wavelengths simultaneously in order to improve the quality of the fits and produce more stable results, allowing the extension of galaxy samples to fainter magnitudes. GALAPAGOS/GalfitM also enable more accurate bulge-disk-decompositions, and the derivation of colour-magnitude or magnitude-size-relations for the individual galaxy components.

His research interests are:

• Galaxy formation and evolution
• Galaxy transformation from blue, star-forming disks to red, "dead" ellipticals
• Build-up of the red sequence
• Bulge/Disc decomposition of galaxies both at low and high redshift (redshift, not km/s)
• Evolution of galaxies
  

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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:

• Evolved stars
• The Galactic Center
• Be stars
• Optical Interferometry and high angular resolution imaging
• Stellar Structure and Evolution
  

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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 is the Deputy Director of La Silla Paranal Observatory. 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.            

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

• Cosmic Microwave Background
• Galaxy Clusters via the Sunyaev-Zel'dovich Effect
  
• High-Redshift Dusty Galaxies
• Cosmology and the Early Universe

Aaron Labdon, is an Operations Staff Astronomer at Paranal Observatory, where he is currently involved in the instrument operations team of GRAVITY. He obtained his PhD from the University of Exeter (UK) in 2021, with a thesis titled ‘The Inner Astronomical Unit of Protoplanetary Disks’. During this time he worked as part of the MIRCX instrument team, an interferometric beam combiner at CHARA. In 2021 he joined ESO as a fellow working with the VLTI, specifically as the GRAVITY instrument fellow, before moving the his current role in 2023. His current research interests focus on optical interferometry of young stellar objects and variable accretors with interferometry and spectroscopy.

Scientific interests: 

• Optical Interferometry
• Young stellar objects and protoplanetary disks
• Variable accretion and FU Orionis objects

Cédric Ledoux is a Faculty astronomer supporting the science operations of the Very Large Telescope. He obtained his PhD in Astrophysics at the University of Lyon I in 1999. His research includes the properties and evolution of galaxies revealed by high-redshift QSO absorption-line systems, the study of metals, dust, and molecules, in the interstellar medium of galaxies, and the distribution and physical properties of the gas in and around the host galaxies of Gamma-Ray Bursts. He is involved in the operations of the Ultraviolet and Visual Echelle Spectrograph (UVES) and the Echelle Spectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO).

His main research interests are:

• Evolution of Galaxies and the ISM; Cosmology and the Early Universe

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.

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:

• Globular Clusters
• Open Clusters
• Chemical Abundances of stars in the Local Group
• Star Formation and Chemical Evolution History of Dwarf Galaxies in the Local Group
• X-rays Binaries
• Neutron Stars
• Stellar populations; Evolution of Galaxies and ISM

Jorge Melnick was the VLT Programme Scientist.  His research interests include violent star formation, galactic and extragalactic starbursts and the evolution of  massive stars. 
He is now retired as astronomer emeritus at ESO.

Hugo Messias is an Astronomer at ALMA’s Department of Science Operations since January 2020. 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. He was then a FCT Fellow at Institute of Astrophysics and Space Science (IA, Portugal) since 2014, where he was also the Lead Scientist of the Portuguese ALMA Centre of Expertise. That led to his moving back to Chile as an ALMA Fellow from 2016 and 2019. After a short period at IA at the end of 2019, he was back again to ALMA as a DSO Astronomer. His scientific interests are mostly related to extra-galactic astronomy: galaxy and super-massive black-hole (co-)evolution; gas content and dynamics in galaxies; galaxy growth mechanisms; IR-selected AGN; distant (sub-)millimeter/radio-selected galaxies.

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.

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Lars-Åke Nyman received his Ph.D. in 1985 at Onsala Space Observatory in Sweden. In 1989 he joined ESO to be in charge of operations of the SEST (Swedish-ESO Submm Telescope) on La Silla. From 2002 he participated in the startup of APEX and in 2003 he became its first Station Manager. From 1995 to 2000 he was involved in the site testing for the precursors to ALMA, and from 2000 responsible for the European part of the ALMA site characterization. He joined the ALMA project in July 2007 as Head of Science Operations during construction and first years of full operations. In 2018 he returned to APEX as Station Manager during the upgrades of the telescope, instrumentation and infrastructure, and stayed until May 2020 when he retired.

Scientific interests:

• Circumstellar envelopes around evolved stars
• Star formation
• The distribution of molecular gas and star forming regions in the Milky Way
• Millimeter and submillimeter astronomy and techniques

Angel Otarola is a member of the ESO Science Operations team  in the position of Atmosphere Scientist, responsible for the Astronomical Site Monitor (ASM) system. Holds a PhD in atmospheric sciences from the University of Arizona, with a minor in planetary sciences. Has participated in worldwide site testing studies intended for the identification of the best location for the deployment of astronomical projects such as the Atacama Large Millimeter and Submillimeter Array (ALMA) and the Thirty-Meter Telescope (TMT) Project. Conducts research on the atmospheric properties of best sites for the location of astronomical observatories and their operation. More recently, Dr. Otarola has participated in various initiatives for the preservation of the natural brightness of the night-sky. Is an organizing committee member of IAU’s inter-Division B-C Commission for the protection of existing and potential observatory sites, member of the Chilean Astronomy Society’s light pollution working group,  and the Chilean low-earth orbits satellite group.

Scientific interests:

• Atmospheric water vapour (PWV): monitoring, understanding of its temporal and spatial variability, and forecast.
• Atmospheric turbulence (seeing):  understanding of its temporal and spatial variability, and forecast.
• Use of Machine Learning methods for the modelling of atmospheric seeing and PWV
• Active remote sensing of the Earth's atmosphere
• Imaging and characterization of satellites in low-earth orbits

Claudia Paladini is Operations Staff astronomer at the Paranal Observatory.
She obtained her PhD in 2011 at the University of Vienna (Austria) with a thesis on carbon-rich evolved stars using spectroscopy, interferometry, and model atmospheres. After one additional year as Post-Doc in Vienna, in 2013 she moved to the Université Libre de Bruxelles (Belgium) as PRODEX fellow to work on her ESO/VLT(I) Large Program targeting evolved stars observed with MIDI, VISIR, and previously with the HERSCHEL/PACS  instrument. While in Brussels she was awarded the FRS-FNRS fellowship and continued her investigation on the atmospheres of evolved stars and mass-loss using high angular resolution techniques. Claudia joined ESO in August 2017, she supports observations with the VLTI, and in particular PIONIER and MATISSE instruments.

Scientific Interests:

• Evolved Stars
• Stellar Atmospheres
• Mass Loss, Dust Formation
  
• Binaries
• High angular resolution techniques, imaging, spectroscopy
• Image Reconstruction

Rodrigo Parra is the Head of Science Operations Group APEX. 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.
He is interested in the study of possible evolutionary connections between AGN and starburst activity. He also collaborates in several research projects whose topics include interstellar masers, dense molecular gas in star-forming regions and theoretical models of propagation of radiation in clumpy media.

Scientific interests:

• AGN/Starburst Activity
• Interferometry
• Type II Supernovae
• Radiative Transfer Models
• Evolution of Galaxies and the ISM

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.
Her research interests center on the dynamics and chemical evolution of galaxies, on compact groups and clusters of galaxies, as probes of the formation and evolution of large scale structures.
She is a member of the XXL and VANDELS consortia.

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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.

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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.
His main research interest - exoplanet atmospheres - is ultimately driven by the hunt for life on other worlds. Their atmospheres bear the key to reveal life forms, as they may produce gases that alter the atmospheric composition. With the upcoming technology of the extremely large telescopes, we astronomers will finally be able to answer one of the most fundamental questions: Are we alone in the universe?
Florian is currently working on projects that are aiming to refine the observational techniques for inspecting exoplanet atmospheres. He is an expert on spectroscopy in the visual and near-infrared.

His work interests are:

• Exoplanet Atmospheres
• Astrobiology
• Pulsating Stars
• Public Outreach

Eleonora Sani joined ESO as a Staff Astronomer in March 2015. In 2009 Eleonora obtained her PhD degree at the University of Firenze, Italy, in collaboration with the Max Planck Institute fuer Extraterrestrische Phisik in Munich, Germany. Her scientific research focuses on supermassive black holes and their (co)-evolution with their host galaxies. For her investigations Eleonora  adopts an holistic multiwavelength approach, spanning from the X-rays to the sub-mm frequencies, with the development of diagnostic diagrams and analytical models. Her technical background starts back in 2012 as a fellow at the Large Binocular Telescope with duties on schedule optimization, user support and observatory work and she broadens her competences at ESO being part of various instrument. and operations teams. Currently she is Deputy Head of the Paranal Science operations department with duties as Instrument Operations Team Coordinator.

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 scheme 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.
Ivo obtained his Masters degree in Astronomy from the University of Padova in 1991 with work based on colour-magnitude diagrams of three Galactic globular clusters, under the supervision of Prof. M. Capaccioli and Dr. G. Piotto. He received his Ph.D. in Astronomy from the same university in 1997.

Luca Sbordone joined ESO in June 2016 as a Staff Astronomer and is currently UVES instrument scientist, X-Shooter second instrument scientist and support astronomer for UT1, UT2, and UT3. 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. Observationally his main tools are intermediate- and high-resolution optical and infrared spectroscopy.

Linda Schmidtobreick is currently the deputy Head of the Office for Science at Chile. She is also working on Paranal as support astronomer.
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.

Elyar Sedaghati is an ESO Staff Astronomer at the Paranal Observatory since July 2022. After studying natural sciences at Cambridge University in the UK, he obtained his Master’s degree in physics and astronomy from Freie Universität Berlin. He obtained his PhD in 2017 from the Technische Universität Berlin and the German Space Agency (DLR), including a two-year studentship at ESO, under the joint supervision of Heike Rauer (DLR) and Henri Boffin (ESO). His PhD work focused on the detection and characterisation of exoplanetary atmospheres through low resolution transmission spectroscopy, using data mainly obtained with the VLT. He then spent 3 years at Paranal as an ESO fellow working in the instrument operations teams of FORS2 and ESPRESSO. He spent the 4th year of his fellowship at the Instituto de Astrofísica de Andalucía in Granada, working in the CARMENES consortium; the high resolution visible and near-IR spectrograph at CAHA observatory. After a short post-doc at the Universidad Adolfo Ibáñez in Santiago, he returned to ESO, currently working in the FORS2 and ESPRESSO operation teams.

He is currently involved in several scientific and instrumental projects, answering questions such as 1) what planet formation theories describe best the currently observed exoplanetary systems; 2) how to best interpret three dimensional, disequilibrium and dynamic pictures emerging from high resolution spectroscopic observations of exoplanetary atmospheres; 3) how to best improve and optimize current and future high resolution spectrographs in order to facilitate detailed characterisation of smaller exoplanetary atmospheres; and 4) how to optimize telluric correction of spectra using the radiometers installed at Paranal.

His scientific interests include:

• Exoplanet Atmospheres
• Planet formation theories & orbital architectures
• High resolution spectroscopy
• Computational techniques

Elyar Sedaghati (esedagha.github.io) & sc.eso.org/~esedagha

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.
He has previously worked at the University "La Sapienza" of Rome, Italy, (Experimental Cosmology Group) and at the Max Planck Institute for Radio Astronomy (MPIfR) of Bonn, Germany (Mm/Submmm Astronomy and Bolometer Development Group).
He received his Ph.D. in Astronomy in 2003 from the University of Bonn with a thesis on a polarimeter for bolometer cameras.
He has a strong background in observational astronomy at mm/submm wavelengths and also in technology design and development.
His main research interests are:

• Cosmology and Early Universe: high-z submm galaxies, anisotropies and polarization of the Cosmic Background Radiation; mm/submm sensitive continuum detection
• the role of the magnetic field in the star formation process, dust polarization and magnetic fields in molecular clouds; mm/submm spectro-polarimetry
• AGN variability and polarization at mm/submm wavelengths; mm/submm interferometry and VLBI

Alain Smette is a VLT operations Staff Astronomer since 2004. Following studentships at ESO-Garching and La Silla, he received his PhD from the Universite de Liège, Belgium, in 1994. He was then a Post-Doc at Kapteyn Institute, Groningen. He became  a research associate at the NASA-Goddard Space Flight Center, in the STIS team, in 1997, then came back to Liège in 2001. 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. In addition, together with several colleagues, he develops Molecfit, a tool to correct telluric absorption lines. As member of the Science Operations Department until December 2021,  he was successively the instrument scientist for VISIR, then CRIRES and Instrument Operations Team coordinator.  He is currently System Scientist in the Paranal System Engineering group, within the Director’s office.

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.

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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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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:

• active galactic nuclei
• supermassive black holes
• nearby active galaxies
• very high angular resolution imaging and spectroscopy
• optical and infrared interferometry

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Baltasar Vila Vilaro, is a System Astronomer in ALMA (Array Performance Group). PhD in Astrophysics at the Universidad de La Laguna/Instituto de Astrofisica de Canarias (Spain) in 1993. Moved to Japan as a post-Doc for 6 years at the Nobeyama Radio Observatory. In 1999 moved to Arizona (USA) to work at the SMTO (Sub-millimeter Observatory) of the Steward Observatory. In 2004 moved back to Japan as Instrument Scientist for the Atacama Compact Array (part of ALMA), and since 2009 is a System Astronomer at the Joint ALMA Office in Chile.

• Science Interests: Nuclear activity in galaxies, lenticular and elliptical galaxies, molecular and atomic gas properties along the Hubble Sequence, Milky Way structure.
• Technical interests: mm/submm. interferometry, calibration.

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.

Enrico Congiu is an ESO fellow with duties in Paranal since November 2022. He obtained his Ph.D. at the University of Padova, with a thesis on the properties of extended structures in nearby AGN. After his Ph.D. he moved to Chile to the Las Campanas Observatory where he started studying the properties of ionized nebulae in nearby galaxies as part of the PHANGS collaboration. After this first experience he moved to Universidad de Chile as a CATA/DAS fellow, continuing his work on the identification and classification of ionized nebulae, and joining the Local Volume Mapper Science team.

Scientific interests:

• Interstellar medium
• Ionized nebulae
• Star-forming galaxies
• Integral-field Spectroscopy

Evgenia Koumpia is an ESO fellow with ALMA duties since December 2021. She obtained her PhD from the University of Groningen (NL) and in 2017 she moved to the University of Leeds (UK) as a Research Fellow in the field of Star Formation. 

Her scientific interests include:

• High and low mass star formation
• Close binaries
• Dense cores
• Massive stellar evolution. 

For her research she uses high angular and spectral resolution observational techniques from near-infrared to sub-mm wavelengths.

Rob van Holstein is an ESO fellow since November 2021 with duties at Paranal. He obtained his MSc in Aerospace Engineering from the Delft University of Technology in 2016. He received his PhD from the Leiden University in October 2021 on high-contrast imaging polarimetry of exoplanets and circumstellar disks, in particular using the instrument SPHERE-IRDIS at the Very Large Telescope. His main research interests are:

• Formation of planets and brown dwarf companions
• Protoplanetary and debris disks
• High-contrast imaging polarimetry
• Novel observing techniques
• Instrumentation, calibration, and data reduction