ESO Scientific Staff in Garching
Find out more about the Key Research Areas in Garching:
| (1) Planets and Star Formation (3) Stellar Populations (5) Cosmology and the Early Universe |
(2) Stellar Structure and Evolution (4) Evolution of Galaxies and the ISM |
See also the PhD Thesis Topics offered by ESO Faculty Members (Garching and Chile) and the ESO Santiago Staff and Research page for scientific staff in Chile.
- Planetary nebulae populations: their luminosity functions, specific frequencies and stellar progenitors
- Diffuse stellar population in galaxy clusters & intracluster Planetary Nebulae
- Dynamics of late and early-type galaxies, mass content of galaxies, polar-rings, properties of dark matter haloes
- Galaxy and galaxy cluster formation and evolution
- Near field cosmology and hierarchical mass assembly of galaxy halos
- Star formation and young stellar evolution
- Magnetic fields on young stars
- Infrared instrumentation
- Galactic kinematics and dynamics
- Stellar galaxy halos
- Intracluster light
- Stellar populations
- Kinematic decoupling in galaxies
- Extragalactic Planetary Nebulae
- 3D spectroscopy
- Supermassive black holes
- High redshift radio galaxies
- Radio and millimetre interferometry
- Radio surveys
- Optical spectropolarimetry
- Formation, structure and dynamics of galaxies, including the Galaxy
- Star clusters and OB associations
- Galactic dynamics
- Early-type galaxies
- Stellar populations
- 3D spectroscopy
- Numerical simulations
- Data analysis softwares
- Observational cosmology
- High-redshift galaxies and quasars
- Active Galactic Nuclei (AGNs)
- Large Scale Structure and peculiar motion of galaxies
- Comets, asteroids, trans-neptunian objects
- Surface properties and evolution of icy bodies
- Cometary activity at large heliocentric distances
- Ultra-deep imaging
- Dwarf galaxies in galaxy clusters
- Extragalactic globular clusters
- Stellar populations
- Element abundances of galactic globular clusters
- Transiting exoplanets
- Nearby brown dwarfs and low mass stars
- Milky Way structure and star clusters
- Optical and near-IR interferometry
- Double stars and stellar evolution
- Star formation
- Pre-main Sequence Stars in massive star-burst Clusters
- Stellar Population in Clusters
- Stellar dynamics in Globular Clusters
- Exotica in Globular Clusters (BSS, MSP, IMBH)
- Resolved stellar populations in dSph
- Central Parsecs of AGN
- High-Mass Star Formation
- Evolved Star Mass Loss
- Millimetre and Submillimetre Astronomy
- Magnetic activity in cool stars and stellar clusters
- Optical, NIR and X-ray spectroscopy of stars and circumstellar environments
- T Tauri and pre-main sequence stars
- Stellar surface imaging
- Evolution of the ISM in galaxies
- Formation of galaxies in the distant Universe
- Dust formation
- Masers
- Proto-Planetary disks
- Exoplanets
- Stellar evolution (post main sequence, RGB, AGB, post-AGB)
- YSOs and Circumstellar Discs
- Planetary and cometary atmospheres
- Very high contrast imaging
- Hi-speed photometry
- Instrumentation
- Planetary nebulae
- Late stages of stellar evolution
- Stellar mass loss and interaction with the interstellar medium
- Galaxy formation and evolution
- Stellar populations of early-type galaxies
- Extragalactic globular clusters
- Integral-field spectroscopy
- Active galaxies, relativistic jets in extragalactic and galactic sources, synchrotron and inverse Compton emission, polarization and extragalactic magnetic fields, Faraday rotation, radio surveys.
- Optical/IR telescopes; telescope control; aperture synthesis at cm, mm and sub-mm wavelengths.
- Isolated neutron stars
- Planet formation
- Stars in the solar neighborhood
- High resolution spectroscopy, precise radial velocity measurements
- Multiwavelength properties of AGN and their SED (X-ray, optical, near-IR, sub-mm, radio)
- Highly obscured (Compton thick) AGN
- AGN properties as a function of the environment: field, groups, clusters of galaxies
- High-redshift X-ray clusters of galaxies: their metallicities and AGN content
- AGN feedback
- 3D spectroscopy (SINFONI)
- X-ray binaries
- Stellar mass black-holes
- Neutron stars
- Disc accretion outflows: winds and jets
- Galactic globular clusters
- Horizontal branch stars
- Late stages of stellar evolution
- Damped Lyman-alpha Absorbers at high redshift
- Dust at high redshift
- Galaxy Formation and Evolution
- Formation of Large Scale Structure
- Absorption and emission scaling relations of DLA galaxies and GRB hosts
- Redshift Evolution of galaxy scaling relations
- Active Galactic Nuclei (AGN), X-ray, gamma-ray emission
- BL Lacertae Objects
- Blazar Surveys
- Deep radio surveys
- AGN - starburst connection
- Neutrino and cosmic-ray astronomy
- Precision Spectroscopy, direct measurement of the cosmic acceleration
- Light Element Abundances (Li and Be): Primordial Nucleosynthesis, Galactic Enrichment, Stellar Mixing
- Globular Clusters: light elements anti-correlations
- Chemical Abundance of stars in the local group, in clusters and in the field
- Exo-Planets, planets around evolved stars
- Spectroscopic Survey Facility
- Supernovae
- Statistical Data Analysis
- Polarimetry and Spectropolarimetry
- Star formation in this and nearby galaxies
- Cirumstellar matter (disks, outflows)
- Near-infrared spectroscopy (particularly of H2)
- Instrumentaton expertise: IFU spectroscopy, KMOS, ELT instrumentation
- Resolved stellar populations in nearby galaxies
- Extragalactic globular clusters
- Variable stars
- Centaurus A = NGC 5128
- Stellar populations in nearby Galaxies
- Distance measurements
- Star formation and early stellar evolution
- Optical Long Baseline Interferometry
- Stellar magnetic fields
- Star formation and stellar evolution
- Supvernovae, their use as distance indicators
- IR spectroscopy
- High resolution spectroscopy
- Active Galactic Nuclei
- Starburst Galaxies
- Super Star Clusters
- Adaptive Optics/NIR Imaging and Spectroscopy
- High mass star formation
- Young (proto-)stellar clusters
- Young brown dwarfs
- Circumstellar disks and their evolution
- Resolved stellar populations
- Star Clusters
- Galactic Bulge
- Chemical Abundances
- Adaptive optics - NIR Imaging and Spectroscopy
- Star and Planet Formation
- Protoplanetary Disks
- Exoplanets
- Infrared Spectroscopy
- VLT Instruments: CRIRES, FORS2, SPHERE, VISIR, XSHOOTER
- The formation and evolution of galaxies
- High-redshift galaxies and galaxy clusters
- Cosmological simulations
- Gravitational lensing
- Atmospheres and mass-loss of evolved stars
- Fundamental stellar properties
- Optical interferometry and interferometric imaging, mainly with the VLTI instruments PIONIER and GRAVITY
- Synergy of optical and radio interferometry
- Evolution of gas in galaxies
- Radio and millimetre surveys
- QSO absorption lines
- ALMA
- Progenitors of Supernovae
- Radiative Transfer
- Stellar Spectroscopy and Analysis
- Data Mining
- Evolution of protoplanetary disks
- Exoplanet population synthesis from disk dust/ gas composition
- ISM/ molecular cloud chemistry
- Multi-wavelength extragalactic surveys
- Galaxy formation and evolution
- Evolution of the ISM in galaxies
- Simulations of galaxy formation and evolution
- Modelling the ISM in galaxies
- Modelling sub-mm emission from galaxies
- Infrared dark clouds
- Initial conditions of high-mass star formation
- mm/submm/cm interferometry
- Far-IR spectroscopy and photometry with Herschel
- low-mass star formation
- protostellar energetics and dynamics
- chemcial evolution from pre-stellar cores to circumstellar disks
- planetary atmospheres
Sybilska (formerly Rys), Agnieszka
- Formation and evolution of dwarf galaxies in cluster and field environments
- Dynamical modelling of galaxies
- Galaxy scaling laws
- Integral field spectroscopy
- The quenching of star formation in massive galaxies
- Quiescent galaxies at high-redshift: formation & evolution; stellar populations & ISM; structures & dynamics
- Galaxy mergers: observations & simulations
- Strong gravitational lensing
- Formation history of galaxy clusters
- Evolution of galaxy clusters
- Globular clusters and ultra-compact dwarf galaxies in galaxy clusters
- Low mass star formation: cloud cores, protostars, protostellar disks, jets and outflows
- High mass star formation (jets and outflows)
- High-redshift radio galaxies (optical/IR line-emission), AGN's
- Galaxy structure: edge-on galaxies, thin and thick disks
- Optical and infrared instrumentation
- High-redshift radio galaxies
- Radio galaxy evolution
- AGN characteristics
- Radio and mm surveys
- Gamma-ray burst (GRB) afterglows and host galaxies
- Interstellar medium (mainly extragalactic)
- Superluminous supernovae
- Cosmic Dust
- Active Galactic Nuclei (AGN)
- Infrared extragalactic astronomy
- Extragalactic Surveys
- ALMA
- Formation of OB clusters
- Sgr A* accretion
- Accretion outburst young stellar objects
- Type Ia Supernovae
- Spectropolarimetry with VLT/FORS
- Superluminous Supernovae and their host galaxies
- Interstellar medium
- Small Solar System Bodies
- Interacting binaries
- Exoplanets
- Star and planet formation
- Stellar Population in Clusters
- Formation and evolution of galaxies
- High redshift galaxies
- Active Galactic Nuclei (AGN)
- Galaxy formation and evolution
- Circum-galactic medium of quasars
- Detection of large-scale structure in emission
- Lyman Alpha Blobs (LABs)
- Star formation in the Magellanic Clouds
- Pre-main-sequence and young stellar evolution
- Near infrared surveys
- Physical properties of HII regions through analysis of nebular emission lines
- High-redshift Lyman-alpha emitters and Lyman break galaxies
- Sources of cosmic reionization
- Evolution of the ISM in galaxies
- High-redshift galaxies
- Cosmic microwave background
- Molecular gas excitation conditions
- Extremely metal poor galaxies
- Supernova remnants
- Millimeter/ Submillimeter Instrumentation
- Formation and Evolution of Galaxy Clusters
- Sunyaev-Zel´dovich (SZ) Effect and X-ray Observations of Galaxy Clusters
- Cosmic Microwave Background
- Low-mass star formation: magnetic field, gas kinematics, disks
- Protoplanetary disks: structures and kinematics
- Polarization of starlight
- Dust grains
- Interstellar and galactic magnetic fields
- Galaxy formation and evolution
- High-redshift galaxies
- Multi-wavelength properties of distant galaxies
- 3D spectroscopy
- heavily obscured AGN, X-ray surveys
- BH-galaxy co-evolution
- properties of AGN and their hosts (study of multiwavelength SEDs: X-ray, optical, near-IR, sub-mm, radio)
- AGN feedback
- Galaxy formation and evolution
- Nuclear star clusters formation and evolution
- The interplay between baryons and dark matter in galaxies
- Near-IR properties of stellar populations
- Stellar spectral libraries
- Galaxy formation and evolution
- Dynamics and star formation in galaxies
- Galaxy mergers
- Radio and millimetre astronomy
- Galaxy formation and evolution
- Star-forming galaxies at high redshifts: star-forming giant clumps, ISM properties, morphology, molecular gas content
- Quiescent galaxies at high redshift: structure, dynamics, and quenching
- Galaxy formation and evolution
- AGN feedback
- Galaxy kinematics and dynamics
- Multi-wavelength properties of distant galaxies
- 3D spectroscopy
- Dark Matter in Galaxies
- Galaxy Scaling Relations
- Gas and Star Formation
- Low-mass Galaxies
Grid Item Title
- Galaxy formation and evolution
- AGN feedback
- 3D spectroscopy
- Stellar populations in galaxies
- High precision stellar parameters determination using multi-observations modelling
- Cepheid pulsating stars
- Distance indicators
- Spectroscopy and spectropolarimetry of Supernovae
- Progenitors and explosion models of Type Ia Supernovae
- Supernovae as distance indicators
- Galactic Centre
- Astronomical images analysis and reduction
- Extinction maps and star population
- Stars at low metallicity
- High-resolution spectroscopy
- Galactic chemical evolution
- Exoplanets by direct imaging
Ubeira Gabellini, Maria Giulia
- Planet formation
- Disk evolution and accretion
- Brown dwarfs
- Fluid dynamics
- Molecular cloud IMF
- Star formation
- The formation and evolution of galaxies
- Star clusters and associated black holes
- Astrobiology, exo-planets and life beyond the Solar System
- Instrumentation (VIMOS, SINFONI, HAWK-I, KMOS)
- Active Galactic Nuclei: structure, populations
- Galaxy - supermassive black hole coevolution
- Observational cosmology
- Formation and evolution of galaxies and QSOs
- Far infrared and submillimetric extragalactic backgrounds
- Stellar astrophysics: variability, multiplicity, evolution
- Cosmology: distance scale
- Protoplanetary disk evolution and formation of planets
- Accretion and ejection processes in young stars
- Photospheric and chromospheric properties of pre-main sequence stars
- Kinematic properties of young stellar clusters
- Galactic chemical evolution
- Chemical abundances in metal-poor stars
- High resolution spectroscopy
- Galaxy formation and evolution
- Gravitational lensing, stellar dynamics
- Object classification and rare-object searches
- Quasars and their host galaxies
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