Research Fellow

Research Fellow

Kontos

Φωτογραφία Τάκη Κόντου
Education

Takis Kontos obtained a MSc and a PhD in Solid State Physics at the University of Orsay, France, in 1998 and 2002 respectively.

Career

The research of Takis Kontos is mainly based on the implementation of hybrid quantum circuits, aiming to reveal new states of matter or to exploit quantum mechanical properties of circuits. During his thesis at CSNSM, Orsay, France, he studied the interplay of superconductivity and ferromagnetism in multilayers of superconductors and ferromagnetic alloys together with Marco Aprili and Jérôme Lesueur. He moved as a postdoctoral researcher to the University of Basel, Switzerland, in the group of Prof. Christian Schönenberger, where he studied spin transport in carbon nanotubes. Since 2005, he has been permanent CNRS researcher at LPENS, Ecole Normale Supérieure, first as a research associate and, since 2013, as a research director. In collaboration with Audrey Cottet for the theoretical aspects, his research has focused on the implementation of a circuit quantum electrodynamics architecture with carbon nanotubes for which he was awarded an ERC CoG in 2013 (project “CirQys”). He could shed new light on fundamental aspects of condensed matter such as the Kondo effect. He could also develop a synthetic spin-photon interface for single spins trapped in carbon nanotubes. The latter work is at the basis of the technology used by the “quantum” start-up C12 Quantum electronics, which Takis Kontos co-founded in 2020. Takis Kontos is now focusing on the use of quantum sensing techniques with circuits in order to test dark matter paradigms such as axions or to measure radioastronomical signals such as the 21 cm hydrogen line. For the dark matter quantum sensing project, he has been awarded an ERC SyG in 2023 (project “Dark Quantum”). He joined IA-FORTH as a Research Fellow in 2025.

Interests

Quantum circuits with superconductors and/or carbon nanotubes, condensed matter physics, quantum sensing of axion dark matter and of radioastronomical signals.

Email
Affiliation
Name
Takis
University/Institute
École Normale Supérieure & École Supérieure de Physique et Chimie Industrielle, Paris (France)
Past Member
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Director
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Female
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Educational Title TR

Charisi

MariaCharisi
Education

Maria Charisi obtained her BSc in Physics from the Aristotle University of Thessaloniki in 2011. She then completed her PhD in Astronomy in 2017 at Columbia University in the City of New York under the supervision of Zoltan Haiman.

Career

Between 2017-2020, she worked as a NANOGrav (North American Nanohertz Observatory for Gravitational Waves) fellow in the TAPIR group at Caltech. From 2020-2023, she was a VIDA (Vanderbilt Initiative for Data-intensive Astrophysics) fellow at Vanderbilt University and subsequently she joined the Department of Physics and Astronomy at Washington State University as an assistant professor. She is a member of the NANOGrav Collaboration, the International Pulsar Timing Array, the LISA Consortium and the LSST AGN Science Collaboration. In 2023, she was awarded an ERC Starting Grant entitled "MMMonsters: The first multi-messenger detection of a supermassive black hole binary" and she joined IA-FORTH as a research fellow. In 2024 she was the recipient of the “L’Oreal-UNESCO Award for women in science”.

Interests

Supermassive black hole binaries, multi-messenger astrophysics, time-domain and gravitational-wave astrophysics, pulsar timing arrays, big data and machine learning

Email
Department
Dept. of Physics and Astronomy
Affiliation
Name
Maria
University/Institute
Washington State University (USA)
Past Member
Off
Director
Off
Female
On
Educational Title TR

Gilmore

Gilmore
Education

Gerard (Gerry) Gilmore obtained his MA, Sc.D. from Cambridge University, UK and his PhD in Astrophysics from the University of Canterbury, New Zealand.

Career

He spend 5 years (1979-1984) at the Royal Observatory Edinburgh before moving to the Institute of Astronomy at the Univ. of Cambridge, where in 2000 he became Professor of Experimental Philosophy, FRS. He has been Scientific Coordinator of Opticon, the EC Optical Infrared Coordination Committee for Astronomy and more recently the Opticon-Radionet-Pilot. He is the UK PI of the Gaia data processing and analysis consortium; Co-PI of the Gaia-ESO Public Spectroscopic Survey. For his research he was also awarded an ERC Advanced Grant. Professor Gilmore has received numerous awards and recognitions for his contributions to astrophysics including: Fellow of the Royal Society (2013), Fellow of Academia Europaea and Institute of Physics, Honorary Fellow of Royal Astronomical Society NZ (2016), recipient of the Chalonge Medal (2013) and the De Vega medal (2015). As of 2023 he is Emeritus Professor of Experimental Philosophy.

In 2023 he was elected as lifetime Honorary Fellow of the Institute of Astrophysics - FORTH.

Interests

The main interests of Professor Gilmore are related to near-field cosmology. This is the use of precision studies of kinematics, dynamics, stellar populations, chemical abundances, etc. for the oldest systems in the local universe to deduce the fundamental properties of structure formation and the nature of dark matter in the early Universe. He has been intimately involved in the planning and scientific exploitation of the ESA satellite GAIA, which was launched in 2013. Moreover, as a Co-PI of the Gaia-ESO Survey,  a  400+night ESO-VLT Public Spectroscopic Survey -the largest large-telescope high-quality stellar spectroscopic survey - he is leading the effort of the major complementary science to the GAIA.

Email
Department
Institute of Astronomy
Affiliation
Name
Gerard (IA Hononary Fellow)
University/Institute
Cambridge University (UK)
Past Member
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Director
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Female
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Educational Title TR

Starck

Starck
Education

Dr. Jean-Luc Starck studied Physics in the University of Nice, holds a Ph.D from Nice Observatory (1992) and a Habilitation from the University Paris XI.

Career

After a brief postdoctoral appointment at ESO, he joined CEA-Saclay in 1993 as a tenure researcher. Over the years he has been a frequent long term visitor of several institutions including ESO, UCLA, Stanford, the Flatiron Institute, and FORTH. In 2010 he founded and has been leading since, the “CosmoStat Lab” at CEA, an interdisciplinary research group, currently having 16 researchers. His group is performing cutting edge research at the interface between astrophysics, cosmology and statistics, with strong interests in applications for space missions, as well as developing close industry-academia partnerships. He has received the EADS prize of the French Academy of Science in 2011, as well as the 2018 Gruber Prize in Cosmology (as a member of the ESA Planck team) and the Tycho Brahe Medal of the European Astronomical Society in 2022. He is also member of Academia Europae (since 2021). Over the last 10 years, he has been awarded as Co-I or PI ~11MEuros in competitive research funding including an Advanced ERC. He has published over 300 refereed papers in astrophysics, cosmology, signal processing and applied mathematics, which have received more than 98,000 citations (source Google Scholar), and he is also author of three books.

In 2022 he was awarded a highly competitive ERA Chair in "Astroinformatics", in collaboration with the Institute of Computer Science and the Institute of Astrophysics and the Board of Directors of FORTH named him an "Honorary FORTH Fellow".

Interests

Jean-Luc Starck is a pioneer in the field of astrostatistics: Modern telescope facilities produce large amounts of data and require advanced analysis techniques to achieve their scientific goals. Thus astrophysicists have been increasingly relying on statisticians to develop sophisticated and mathematically robust methods to reduce and interpret their data.Currently he is mainly interested in various aspects of cosmology and he is heavily involved in the Euclid space mission of ESA, which was launched on July 1, 2023.

Email
Department
IRFU/DAp-AIM
Affiliation
Name
Jean-Luc (FORTH Honorary Fellow)
University/Institute
CEA-Saclay (France)
Past Member
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Director
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Female
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Educational Title TR

Chatzopoulos

chatzopoulos
Education

Manos Chatzopoulos obtained his BSc in Physics from the University of Crete in 2007. He then completed his Ph.D. in Astronomy in 2013 at the University of Texas at Austin under the supervision of J. Craig Wheeler.
 

Career

Between 2013-2016 he worked as an Enrico Fermi Postdoctoral Research Fellow at the Department of Astronomy at the University of Chicago and the FLASH Center for Computational Science until he joined the Department of Physics & Astronomy at Louisiana State University in 2016 at the rank of Assistant Professor and was promoted to Associated professor in 2022. He joined IA-FORTH as research fellow in 2021.

Interests

Numerical modeling of supernovae and luminous transients. Superluminous supernovae and circumstellar interaction. Massive stellar evolution. Binary star mergers. Monte Carlo radiation transport. 
 

Email
Department
Dept. Physics & Astronomy
Affiliation
Name
Manos
University/Institute
Louisiana State University (USA)
Past Member
Off
Director
Off
Female
Off
Educational Title TR

Readhead

Readhead
Education

Anthony Readhead obtained his B.Sc. in Physics from the  University of Witwatersrand (South Africa) in 1968 and his Ph.D. in Physics from the University of Cambridge (UK) in 1972. His thesis was entitled "The angular structure of radio sources" and was performed under the supervision of Prof. Antony Hewish.

Career

He joined California Institute of Technology as a Research Fellow (1974-75) continuing as Senior Research Fellow (1976-79) and then  Research Associate, 1979-81. He became  Professor of Radio Astronomy in 1981 and Professor of Astronomy from1990 to 2000. He was Rawn Professor, 2000-13 and then Robinson Professor, 2013-15. Since 2015 his is  Robinson Professor, Emeritus. Professor Readhead served in various administrative positions including Director, of the Owens Valley Radio Observatory, 1981-86, 2007-18,  Executive Officer for Astronomy, 1990-92, 2012-13; Director of Chajnantor Observatory, 2006-2011 and  Jet Propulsion Laboratory Senior Research Scientist, 2006-15. He is a member of the US National Academy of Sciences and the American Academy of Arts and Sciences. 

Professor Readhead was elected as the first Honorary Fellow of the Institute of Astrophysics - FORTH in 2021.

Interests

The main areas of interest of Prof. Readhead are observational cosmology, especially the cosmic microwave background radiation, and active galaxies, with special emphasis on the central engines that drive them and the formation of relativistic jets. In carrying out research in both these areas he is particularly interested in developing state-of-the-art instrumentation.

Over the last ten years he led the Cosmic Background Imager (CBI) project in Chile, and this has now been superseded by the QU Imaging ExperimenT (QUIET) project at the same site. In Phase I, his group demonstrated the feasibility of using Monolithic Millimeterwave Integrated Circuits (MMICs) for making very sensitive observations of the cosmic microwave background, and is  now embarking on QUIET Phase II, with which they hope to detect the large-scale B-mode polarization radiation caused by gravitational waves interacting with the CMB. The detection of this signal would prove that the universe did go through an inflationary phase, reveal the energy scale of inflation, possibly pushing the clock back to 10-35 s after the Big Bang. The new radio laboratory in Cahill is working closely with JPL and Northrop Grumman Corporation to improve the sensitivity of the MMIC amplifiers.

The other side of his research involves the engines that drive the activity in active galaxies. His group, in collaboration with several others, developed the Very Long Baseline Interferometry (VLBI) imaging techniques that are in wide use today, and is using VLBI to study a carefully selected sample of blazars that are also being observed with Fermi-GST, and in addition we are observing the TeV sources being monitored by VERITAS. A program of 15 GHz monitoring of the light curves of ~1200 blazars on the Owens Valley Radio Observatory (OVRO) 40m Telescope twice a week is the most comprehensive variability study of active galaxies thus far and is providing key information on these objects.

Email
Department
Astronomy Department
Affiliation
Name
Anthony (IA Hononary Fellow)
University/Institute
California Institute of Technology (USA)
Past Member
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Director
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Female
Off
Educational Title TR

Ramaprakash

ram phot
Education

Anamparambu N. Ramaprakash (Ram) obtained his Bachelors in Electronics from the University of Kerala (India) and his MSc and PhD in Physics from the University of Pune (India) in 1996 and 1998 respectively.

Career

During the last part of his thesis (1997-1998) he was a visiting fellow at the California Institute of Technology  (USA). He was a postdoctoral fellow at the Institute of Astronomy of Cambridge University (UK) for the period 1998-2000 before joining the staff of the Inter-University Centre for Astronomy and Astrophysics (IUCAA) at Pune (India). Since 2010 he is a Professor (Scientist G) at IUCAA, where he heads the instrumentation laboratory. He holds several adjunct faculty appointments in Indias as well as a Visiting Associate Faculty at Caltech (since 2015). He joined IA-FORTH as a Research Fellow in 2019. Prof. Ramaprakash has co-/supervised over 20 PhD students and postdocs.

Interests

Prof. Ramaprakash is an expert in astronomical instrumentation. He was Co-PI for Robopol and Robo-AO and currently Co-PI for the Wide Area Linear Optical Polarimeter (WALOP). He is PI of the Devasthal Optical Telescope Integral Field Spectrograph (DOTIFS) at IUCAA, as well as Associate Program Director for India's involvement in the Thirty Metre Telescope project. He is interested in developing instruments for ground and space based astronomy including adaptive optics, optical fibres, sensors and electronics etc., Developing novel astronomical techniques and technology, physics of the inter-stellar medium, and transients.

Email
Affiliation
Name
Anamparambu
University/Institute
IUCAA, Pune (India)
Past Member
Off
Educational Title
Professor
Director
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Female
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Educational Title TR

Kalas

kalas photo
Education

Paul Kalas studied astronomy and physics at the University of Michigan, Ann Arbor. He earned a Ph.D. in Astronomy in 1996 from the University of Hawaii under the direction of astronomer David Jewitt.

Career

He worked as a postdoctoral scientist at the Max Planck Institute for Astronomy in Heidelberg, Germany, the Space Telescope Science Institute, and the University of California, Berkeley. In 2006, he became an Adjunct Professor of Astronomy at the University of California, Berkeley. He joined IA-FORTH as research fellow in 2019.

Interests

Direct imaging of exoplanets and dusty debris disks, the search for exoplanetary rings and moons, stellar and planetary dynamics, ethics in professional astronomy, and the nature of space and time.
 

Email
Department
Department of Astronomy
Affiliation
Name
Paul
University/Institute
Univ. of California, Berkeley (USA)
Past Member
Off
Educational Title
Professor
Director
Off
Female
Off
Educational Title TR