Staff at DAWN

Johan Peter Uldall Fynbo

Section Leader | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am an astronomy professor based at the Cosmic Dawn Center at the Niels Bohr Institute. I received my master’s degree in 1998 and PhD degree in 2000 from the University of Aarhus advised by Bjarne Thomsen and Palle Møller. Before taking up my current position at the Niels Bohr Institute I worked at the European Southern Observatory headquarters in Germany. My research focuses on the assembly and evolution of galaxies across the history of the Universe, through direct observation with optical and infrared telescopes from both space and the ground. My particular interests are chemical evolution, quasar absorption line systems, and transient sources like gamma-ray bursts, supernovae, gravitational wave sources and fast radio bursts. I am also involved in the development of new instrumentation.

I teach a range of courses in astronomy ranging from introductory astronomy courses to master level courses. In collaboration with colleagues from the University of Aarhus, I also teach a summer course in astronomical observations at the Nordic Optical Observatory on La Palma.

Beyond academia, I am a frequent contributor to public outreach, I am vice chairman of the Danish Astronomical Society and I give many public talks on science.

Helena Baungaard-Sørensen

Secretary| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

My main tasks are to provide with administrative assistance to the DAWN team. I enjoy working with passionate people and dedicated scientists and to be able to support with my administrative skills in order for them to thrive in their important research.

Before onboarding DAWN, I studied and achieved a MSc in Global Marketing & Innovation Management. Afterwards I have worked as a financial assistant in the NGO’s of the Danish Refugee Council of Youth and the National Lung Association.

One of my favorite quotes is: “Keep your eyes on the stars and your feet on the ground".

Peter Daniel Johannsen

Student Helper| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a Master's Student of Physics at the University of Copenhagen, with specialisation in Quantum Mechanics. I am interested in Condensed Matter Physics; specifically the technology and theory required to make the future's Quantum Computers. I am currently writing my thesis about Andreev Bound States.

I started as a student helper at DAWN in March 2021; my role is primarily overseeing the websites, but I will also be helping Guarn and Helena as much as I can, with different administrative tasks. 

In my free time I play disc golf and dedicate many hours to bouldering. I’ve played the piano for about 15 years and enjoy travelling through Europe on my bicycle. 

Flóra Anna Zentai

Student Helper| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a master’s student at the Technical University of Denmark, studying environmental engineering, specializing in environmental chemistry. I am very interested in ecological engineering, which uses tools and principles from ecology to solve environmental engineering problems, so it is practically building with nature.

Starting with the autumn of 2022, I have been working at DAWN as a student helper. I am mainly responsible for helping out Guarn and Helena so everything runs smoothly, carrying out practical and administrative tasks.

Charles Steinhardt

I am an associate professor at the Cosmic Dawn Center working on several topics in galaxy evolution and related problems in computer science.  I am currently PI of the BUFFALO HST survey, a large program awarded in Cycle 25 expanding Hubble coverage of the Frontier Fields.  I have also recently been exploring the tension between observations of high-redshift luminous galaxies and theoretical predictions of galactic assembly (arXiv link) and developing models for cosmic ray-dominated evolution.  In addition, develop novel machine learning and astrostatistical methods for working with large datasets.
Previously, I was a postdoc at Caltech working with Peter Capak and Kavli IPMU working with John Silverman, after getting my PhD from Harvard with Martin Elvis.

Charlotte Mason

Associate Professor | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I obtained my PhD from the University of California, Los Angeles and Santa Barbara, in 2018, after which I moved to the Center for Astrophysics | Harvard & Smithsonian as a NASA Hubble Fellow and CfA Fellow.

I work at the intersection of theory and observations, focusing on galaxy formation and evolution, and the galaxy - dark matter connection, in the early Universe. My research combines theoretical models and simulations with statistical analysis to interpret observations of galaxies. In particular, I have focused on finding new ways to measure the process of hydrogen reionization - the Universe’s final phase transition, which ended approximately one billion years after the Big Bang and was likely caused by the very first stars and galaxies. By understanding how reionization occurred we can infer the properties of the universe’s first galaxies, which are probably too rare and faint to detect directly.

I am involved with (mostly near-IR) observations from our largest telescopes in space and on the ground: Hubble, VLT, Keck, and MMT, and I am excited to be among the first users of the James Webb Space Telescope in a Early Release Science program to observe the earliest galaxies.

Darach Jafar Watson

I am an associate professor based at the Cosmic Dawn Center at the Niels Bohr Institute. I received my PhD degree in 2000 from the UCD in Dublin advised by professor Brian McBreen. Before moving to the Niels Bohr Institute, I worked at the University of Leicester as a post.doc. My research interest span a broad range of topics from interstellar dust, gamma-ray bursts, the first galaxies, and sources of gravitational waves. I am mainly observationally oriented and have of the course of my career applied a wide range of techniques and wavelengths ranging from X-rays (using satellites) to the infrared (using ALMA).

I teach a range of courses in physics and astronomy ranging from experimental quantum mechanics to observational astrophysics. I have supervised a large number of students at all levels from BSc to PhDs.
I am also a keen advocate for increased diversity in academia and have published several papers, including in Nature, on this issue.

Georgios Magdis

I am an Associate Professor of astrophysics at National Space Institute of Denmark (DTU Space) and NBI/KU, a core member of the Cosmic DAWN Center of Excellence, and serve as a chair for the Cosmic DAWN post-doctoral Fellowships.  I received my DPhil in astrophysics from the University of Oxford and I have been a post-doctoral researcher at CEA/Saclay, a Research Fellow at the University of Oxford, and a DARK/Carlsberg Fellow and Assistant Professor at the DARK Cosmology Center, NBI/KU (2015-2018).
As of 2016 I am also the leader of the ISM/Galaxy-Evolution group, funded by a research grant (Gas to stars, stars to dust – Tracing the evolution of star formation activity across Cosmic time) that I was awarded by the Velux Foundation.
My group and I, focus on the study of distant galaxies aiming to shed light on their formation, their growth (mass build-up), and evolution of their interstellar medium throughout cosmic time. For my research, I use multi-wavelength datasets and I specialise in infrared/submm/radio space as well as ground-based observations. You can find more about me and my research here.

Gabriel Brammer

I am an Associate Professor at the Cosmic Dawn Center. I received my PhD degree from Yale University in 2010, and prior to coming to DAWN I was a postdoctoral Fellow at the European Southern Observatory (Chile) then an ESA/AURA Astronomer at the Space Telescope Science Institute in Baltimore, Maryland (USA).

My research involves studying the formation and evolution of galaxies across much of cosmic time, from relatively nearby massive, evolved objects to infant galaxies at the current limit of the observable Universe.  I discover and characterize these objects by and exploiting large imaging and spectroscopic surveys with the Hubble Space Telescope, and I am helping to develop next-generation projects with the Guaranteed Time Observer and Early Release Science programs on the James Webb Space Telescope, due to be launched in 2021.

I also enjoy photography with much smaller glass, including night-sky astrophotography and analog film.

Peter Jakobsen

I received my Masters degree from the University of Copenhagen in 1979 and my PhD from the University of California, Berkeley in 1983. I was with the European Space Agency (ESA) from 1984 to my retirement from ESA at the end of 2011.

While at ESA I served as the Project Scientist for Europe's participation in the Hubble Space Telescope (HST) until 1995. From 1997 to 2011 I held the same position for Europe's contributions to the James Webb Space Telescope (JWST). In the latter capacity I oversaw the design and development of the NIRSpec multi-object spectrograph onboard JWST, an instrument that I am still actively involved in.

My scientific interests include astronomical space instrumentation, applied statistics, and the physics of the early universe with emphasis on quasar absorption lines and reionization. I also engage in scientific evangelism, and periodically give public lectures at high schools and other venues across Denmark.

Allan Hornstrup

My interests are focused on cosmology, including the large scale structure of the universe; on space instrumentation and space research in general.  I also fancy exoplanetary studies, including the search for extraterrestrial life.  I enjoy physics, teaching, public outreach and management.

In cosmology, I have studied clusters of galaxies in general (the content) and in particular worked on using clusters of galaxies for cosmological purposes e.g. through the cluster development with time.

Since 2007, I have been head of astrophysics at DTU Space and later included atmospheric physics.  The group has grown from about a dozen to now almost 60 scientists and technicians.  I hold a MSc in astrophysics, a PhD in technical physics and an executive MBA.

Lise Bech Christensen

I am an associate professor based at the Niels Bohr Institute. I received my PhD degree from the Potsdam University in Germany in 2005. Since then I have worked as a Postdoctoral Fellow at the European Southern Observatory in Chile and at the headquarters in Germany, as well as the Excellence Cluster Universe at the Technical University in Munich. In 2011 I moved to Denmark with a Marie Curie Fellowship and a Carlsberg Fellowship. I have lead a research group with a Freia fellowship grant and an YDUN grant obtained from the Danish Council for Independent Research.

My research topics focus on the nature of gas and stars in and around distant galaxies with observations from the largest telescopes. Specifically, I investigate galaxy chemical evolution through quasar- or gamma-ray burst absorption lines, and via strong gravitational lensing.  On the technical side, I work to facilitate Danish participation in instrumentation projects for the next generation of large astronomical telescopes.

I teach courses in extragalactic astrophysics and data handing at Bachelor and Masters levels at the University, and supervise a number of students at all levels.

Kasper Elm Heintz

Assistant Professor | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am an Assistant Professor of Astrophysics based at the Cosmic Dawn Center (DAWN) at the Niels Bohr Institute. I received my PhD degree from the University of Iceland in 2019, advised by Prof. Páll Jakobsson. My thesis project was primarily focused on using gamma-ray bursts and quasars as cosmic probes to study the interstellar medium in high-redshift galaxies.

Now, I mainly work on the optical counterparts and host galaxies of astronomical transients such as fast radio bursts and gravitational wave events, to better understand these extreme sources. Additionally, I develop new techniques to identity quasars based on the astrometric measurements of the Gaia satellite, to provide a more unbiased census of the quasar population and foreground absorption-line systems. More recently I also started working on characterizing the molecular and neutral atomic gas of high-redshift galaxies observed in absorption and emission, using a combination of VLT and ALMA imaging and spectroscopic data. The overarching goal of these projects is to study and track the evolution and chemical enrichment of galaxies through cosmic time. 

I am further involved in the development of a new instrument for the Nordic Optical Telescope: the NOT Transient Explorer (NTE) as Instrument Scientist. I teach a range of courses in astronomy and have supervised a large number of students at all levels from first-year to MSc.

Francesca Rizzo

DAWN Fellow | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a Dawn fellow at the Cosmic Dawn Center. I received my BSc (2013) and MSc (2016) at the University of Pisa and Bologna, respectively. In 2020, I received my PhD from the Ludwig-Maximilians-Universität in Munich (Germany) under the supervision of Dr. Simona Vegetti and Prof. Simon White at the Max Planck Institute for Astrophysics in Garching (Germany). During my PhD, I developed a tool that allows to use gravitational lensing for studying distant galaxies.

I am interested in the ways in which galaxies form and evolve across cosmic time. In particular, my research focuses on galactic dynamics, which is the analysis of the motion of gas and/or stars within galaxies. Through this kind of study, I learn how different physical processes shaped the variety of galaxies that we observe today. You can find more about my research here.

I have long been committed to diversity and acted to create an academic environment, which is more inclusive and inviting towards different gender, sexual orientation, ethnic, and socioeconomically underprivileged groups. For this reason, I enjoy giving my contribution to public outreach events.

Victoria Strait

DAWN Fellow | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a DAWN Fellow at the Cosmic Dawn Center. I was previously a PhD student working with Maruša Bradač at the University of California, Davis until August 2021. During my PhD studies, I developed lens models of Hubble Frontier clusters, and did stellar population fitting for the Reionization Lensing Cluster Survey (RELICS). 

I am interested in all properties of galaxies at cosmic dawn, including (but not limited to) ionization and escape, age, dust, and size. You can read more about my previous research on my website. 

Aswin P Vijayan

DAWN Fellow | The Cosmic Dawn Center (DAWN)
_{DTU Space, Danmarks Tekniske Universitet} 

I am a DAWN fellow at the Cosmic Dawn Center based at DTU Space. I recently finished my PhD (September 2021) at the University of Sussex, UK working with Prof. Peter Thomas and Dr. Stephen Wilkins. I work mainly on simulations of galaxy formation and evolution to understand the impact dust has on various galaxy observables in the early Universe. 

During my PhD I have worked on developing a self-consistent dust production and destruction model in the L-Galaxies Semi-Analytical Model. I have also done extensive work in the development of FLARES, a suite of zoom resimulations using the EAGLE simulation physics targeting a range of overdensities in the Epoch of Reionisation. I implemented a line-of-sight dust extinction model to obtain the UV to near-IR SEDs of these galaxies as well as the full SEDs using the radiative transfer code SKIRT. You can find more details about it on my personal website.

I wouldn’t say no to a session of squash or badminton and enjoy watching football and making random foods.

Jasleen Kaur Matharu

DAWN Fellow | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a DAWN Fellow at the Niels Bohr Institute, University of Copenhagen. I will be assisting in building the necessary software to process JWST Slitless Spectroscopy and eventually use that Slitless Spectroscopy to conduct spatially resolved studies of starlight, star formation and dust in some of the earliest galaxies ever observed.

Anne Hutter

DAWN Fellow | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a DAWN fellow at the Cosmic Dawn Center. I received my PhD from the Leibniz-Institute for Astrophysics in Potsdam in 2015, after which I moved to the Kapteyn Astronomical Institute in Groningen and the Centre for Astrophysics & Supercomputing at Swinburne University of Technology in Australia as a postdoctoral researcher.

I am interested in the Epoch of Reionisation and investigate questions such as: Which physical processes define the properties of the first galaxies and their evolution? What can we learn about the first galaxies from their footprints in the ionisation state of the intergalactic medium? I seek to answer these questions with semi-numerical simulations, in particular with the Astraeus framework  that I have developed over the last few years. I am also passionate about how higher-order statistical and topological analysis methods of the cosmic 21cm signal can constrain the ionising nature of the first galaxies.

More about my research and simulation tools, you’ll find here.

Steven R. Gillman

Postdoc | The Cosmic Dawn Center (DAWN)
_{DTU Space}

I recently received my PhD from Durham University, England in which I worked on integral field observations of high-redshift (z=1-2) star-forming galaxies obtained using a number of spectrographs including KMOS and SINFONI.  Using rest-frame optical emission lines , I was able to use these observations to trace the dynamical motions of the ionised interstellar medium on ~kpc scales in  high-redshift galaxies. By studying the kinematic properties of the galaxies and their correlation with other  properties, such as galaxy morphology, the aim of my PhD was to understand how star-forming galaxies have evolved from z=1-2 into what we observe in the local Universe.

 Here at DTU Space, and as part of the Cosmic DAWN Center, my work will focus on preparation for the  James Webb Space Telescope (JWST) MIRI GTO observations and the subsequent reduction and analysis of this data in years to come.

Lijie Liu

Postdoc | The Cosmic Dawn Center (DAWN)
_{DTU Space}

Specialised in observational radio/(sub)mm astronomy, interstellar medium, star formation and galaxy evolution. My research focuses on understanding the galaxy-scale and cloud-scale ISM properties and how these properties regulate the star formation in different galactic environments. Specifically, my research fields include the physical properties and dynamics of the ISM in nearby and high-z galaxies, the resolved properties of giant molecular clouds in different types of galaxies, and the SF-law from GMC-scale to galaxy-scale over cosmic time.

Anton Norup Sørensen

Researcher | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I work with instrument design for astronomy.  Development is made in close contact with both astronomers and workshops. Projects include characterisation of in-house built cameras, development, integration and test of the X-Shooter backbone, pre-slit unit for the SONG and test equipment for the Euclid mission. Current project is the NOT Transient Explorer, where I develop the cryogenics, slit viewer and calibration system and help with integration and test.

I received my Masters degree in 1996 from the  University of Aarhus, advised by Bjarne Thomsen.

Bo Milvang-Jensen

Researcher | The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a researcher based at the Cosmic Dawn Center. I received my master's degree from the University of Copenhagen, having carried out the research for my thesis at the University of Texas at Austin. I received my PhD from the University of Nottingham, where my PhD advisor was Alfonso Aragón-Salamanca. Subsequently, I was a postdoc at the Max Planck Institute for Extraterrestrial Physics in Garching, followed by a number of years at the Dark Cosmology Centre in Copenhagen, and now at DAWN.

I work on observational extragalactic astrophysics, using optical and infrared spectroscopy and imaging (including narrow-band imaging). In particular I have contributed to the EDisCS project studying cluster galaxies, and the UltraVISTA project studying high-redshift galaxies. I also work on gamma-ray bursts, including their host galaxies, and follow-up of gravitational-wave events. Additionally I am instrument scientist for the NTE (NOT Transient Explorer) instrument being designed and built by the Niels Bohr Institute (PI Johan Fynbo).

Peter Laursen

Senior Scientific and Communication Coordinator
_{Niels Bohr Institute, University of Copenhagen}

I am an astrophysicist and science communicator.

At DAWN, my tasks include arranging workshops, maintaining  our website, communicating our science to the public, as well as conducting my own research.

My research focuses on galaxies, in particular the light coming from processes that have to do with galaxy formation. I use computer simulations to predict and interpret "real" observations. More specifically, I use hydrodynamical simulations with (Monte Carlo) Lyman α radiative transfer.

After my PhD I was a postdoc at the Oskar Klein Centre (Stockholm), the Dark Cosmology Centre (Copenhagen), and the University of Oslo.

You can find out more about me, my research, and my outreach activities on my personal website. 

Trity Pourbahrami

I am a science communications practitioner and educator with the ultimate goal of supporting scientists to communicate more effectively and to have greater impact.  As a natural boundary spanner I decided to obtain my undergraduate degrees in Physics and Physiology and my graduate degrees in Social Welfare and Public Administration.  I am a strategic thinker, and community builder with over 15 years of experience in strategic communications, public relations, marketing, and advocacy spanning the non-profit, government, higher education, and corporate sectors. I have a proven track record of effectively engaging diverse groups and organizations in transforming strategy into operational goals, objectives, and measurable outcomes.

In addition to being a practitioner of communications I am an educator and have designed and delivered a variety of customized trainings as well as a new graduate course on effective oral, written, and media communications.

I also enjoy building community through serving on various local, national, and international community groups including the Federation of Zoroastrian Associations of North America and Leadership Pasadena.

Claudia Lagos

International Associate | The Cosmic Dawn Center (DAWN)
_{International Centre for Radio Astronomy Research, University of Western Australia}

I am a Senior Research Fellow and Lecturer at the International Centre for Radio Astronomy Research at the University of Western Australia and I am an international Associate at the Cosmic Dawn Center. I received my PhD degree from Durham University in 2013, and prior to coming to my current position I was a Research Fellow at the European Southern Observatory (Germany) and then a Discovery Early Career Researcher at ICRAR/UWA (Australia).

My research involves studying galaxy formation and evolution using state-of-the-art cosmological simulations of galaxy formation and large galaxy surveys. I am the main developer of the new Shark semi-analytic model of galaxy formation and one of the members of the EAGLE Simulations collaboration. I am also a member of several galaxy surveys including several being carried out with the Australian Square Kilometre Array Pathfinder, the Anglo-Australian Telescope and the future 4MOST instrument at Paranal, Chile.

Kate Whitaker

International Associate | The Cosmic Dawn Center (DAWN)
_{University of Massachusetts}

I am an Assistant Professor at the of University of Massachusetts, and Associate Faculty at the Cosmic Dawn Center. I received my PhD degree from Yale University in 2012, after which point I was awarded a NASA Postdoctoral Program Fellowship at Goddard Space Flight Center in Greenbelt, Maryland (USA), then a Hubble Fellowship at the University of Massachusetts Amherst (USA).

As an observational extragalactic astronomer, I study galaxy formation and evolution over the past twelve billion years of cosmic time. My students and I actively collaborate with DAWN, working towards pushing our detection quiescent “read and dead” galaxies even earlier in time (within a billion years of the Big Bang itself!). We would like to understand the detailed physics of the structures and underlying stellar populations of these early massive galaxies. With exquisite Hubble Space Telescope imaging and spectroscopy, we explore the rich uncharted territory of the distant universe and continually piece together an intriguing timeline of the cosmos.

I also enjoy dancing, photography, crafting, and spending time with my family.

Karina Caputi

International Associate | The Cosmic Dawn Center (DAWN)
_{University of Groningen}

I am an Associate Professor at the University of Groningen (Netherlands) and Associate Staff (zero appointment) at the Cosmic Dawn Center. I received my PhD degree from the University of Edinburgh in 2005, and then worked as a Postdoctoral Researcher at the IAS, Orsay, France and the ETH Zurich, Switzerland. Between 2009 and 2011 I was a Leverhulme Trust Early Career Fellow at the University of Edinburgh, just before I joined the University of Groningen in 2012.

My research involves studying the formation and evolution of galaxies in the first half of cosmic time. I mainly work with space infrared telescopes (e.g. Spitzer) and ground-based telescopes (e.g. VLT). In addition, I am part of the European Guaranteed-Time Science Consortium for the MidInfrared Instrument (MIRI) that will be on board the James Webb Space Telescope, due to be launched in 2021.

Kristian Finlator

International Associate | The Cosmic Dawn Center (DAWN)
_{New Mexico State University}

I received my PhD from the University of Arizona in 2009. After this, I held a Hubble Fellowship at UC Santa Barbara from 2009-2012 and a DARK fellowship at the Dark Centre for Cosmology from 2013-2015. Since fall 2015, I have been an Assistant Professor at NMSU.

I am interested in the processes that couple galaxies with their environments. Although I have previously studied the relationship between galactic outflows and the mass-metallicity relation, the research that I lead nowadays is anchored in detailed comparisons between predictions from cosmological simulations and observations of galaxies, the circumgalactic medium, and the intergalactic medium. My goal is always to learn how observations constrain the feedback processes that regulate galaxy growth and reionization.

I enjoy learning Danish, jogging, and playing with my two young children. Long ago (z~10^-9) I also played in orchestras; I’m sure I will get back to that at some point.

Peter Capak

International Associate | The Cosmic Dawn Center (DAWN)
_IPAC/Caltech

Until February 2020 I was a Senior Research Scientist with the Euclid NASA Science Center at the California Institute of Technology where I studied the formation and evolution of structure in the universe. I have since joined the Oculus team at Facebook as Architect of Perception Systems for Augmented and Virtual reality.  I received my BSc (1999) from the University of British Columbia, and my MSc (2002) and PhD (2004) from the University of Hawaii at Manoa.

My research interests focused in two areas: the physical processes that govern the formation and evolution of the most massive galaxies in the early universe (z>2) and large area surveys to measure galaxy properties and probe Dark Energy and Dark Matter. I am a founding member of the Euclid consortia, developed the redshift estimation pipeline and simulations for the NASA SPHEREx mission, and was a member of the WFIRST cosmology science definition teams.  I was also principal investigator of the Spitzer Legacy Survey and the SPLASH Spitzer Exploration Science programs which were two of the largest ever carried out on the Spitzer Space Telescope using a year of time.  Previously I was lead of the COSMOS project, lead of the CCAT high-z science working group, and leading to effort to produce enhanced imaging products and a source list for the Spitzer archive.  I have also been co-organizer of the PHAT project aimed at developing a set of best practices for photometric redshifts and made significant contributions to the GOODS Legacy project including deep imaging of The Hawaii Hubble Deep Field North. 

Desika Narayannan

International Associate | The Cosmic Dawn Center (DAWN)
_{University of Florida}

I’m currently an Assistant Professor at the University of Florida in the US.  Prior to this, I was an Assistant Professor at Haverford College in the Department of Physics and Astronomy.  I grew up in Florida, went to undergrad school at the University of Florida and grad school at the University of Arizona.  I did postdocs at Harvard (CfA Fellowship) and Arizona (Bok Fellowship).  

My research focuses on theoretical models primarily related to cosmological galaxy evolution, star formation, and the interstellar medium (ISM).   I principally develop and utilize large scale numerical simulations to simulate the interplay between small scale star formation, ISM physics, and global galaxy evolution.  

I love (American) college football, surfing, snowboarding, jam bands, hiking, and hockey.

Fabian Walter

International Associate | The Cosmic Dawn Center (DAWN)
_{Max Planck Institute for Astronomy}

I am a Senior Scientist and Group Leader at the Max Planck Institute for Astronomy (MPIA) in Heidelberg, Germany. I received my Master Degree at the University of New Mexico (USA) in 1995, and my PhD in astronomy at Bonn University (Germany). I held a postdoctoral appointment at Caltech (Pasadena, USA) from 1999-2002 in the Owens Valley Radio Observatory group. After that, I received the Jansky Fellowship of the National Radio Astronomy Observatory (NRAO), which I took to the VLA headquarters in Socorro, New Mexico (USA). Since 2004 I am a staff member at the MPIA (tenured in 2008), and am still an Adjunct Associate Astronomer at NRAO. I am also a Scientific Editor for the AAS Journals (American Astronomical Society).

My research focuses on studies of the evolution of galaxies and quasars, from the end of cosmic reionization to today. My particular focus is on the studies of the interstellar medium that is a requirement for star formation to proceed. In my research, I intensively use the ALMA, IRAM NOEMA, and VLA radio/millimeter interferometers. In this context I have led a number of large initiatives, such as the THINGS survey of HI emission in nearby galaxies, the HERACLES survey to map the distribution of molecular gas in nearby galaxies, surveys to characterize the interstellar medium in the most distant quasars, and a large ALMA program that studies the molecular gas and dust content in the Hubble Ultra-Deep Field (ASPECS).

Luis Colina

International Associate | The Cosmic Dawn Center (DAWN)
Spanish Research Council CSIC

I am a senior research scientist of the Spanish National Research Council (CSIC) at the Centro de Astrobiología (CAB) in Madrid (Spain), and International Associate at the Cosmic Dawn Center. I received my Master Degree at the University Complutense of Madrid (Spain) in 1982, and my PhD in Natural Sciences at the University of Goettingen (Germany) in 1987. I have worked as an ESA postdoctoral fellow (1989-1990), and ESA staff astronomer (1993-1998) at the Space Telescope Science Institute (Baltimore, USA). I was Associate Professor at the University of Valencia before joining the Spanish National Research Council in 2000. I have been involved with the James Webb Space Telescope (JWST) as MIRI European coPI and Spanish PI since 2000. I am co-chair of the European MIRI High-redshift GTO team, and coI of the MIRI Nearby Galaxies GTO team since 2010. My research interests focus mostly on the study of the formation and evolution of dusty star-forming galaxies and AGNs at both low- and high redshifts using different multi-wavelength imaging and integral field spectroscopy techniques from the ground (ALMA, VLT), and space (HST, Spitzer, JWST)

Pascal Oesch

International Associate | The Cosmic Dawn Center (DAWN)
Department of Astronomy | University of Geneva

I am currently an Assistant Professor at the University of Geneva, where I lead a research group “Galaxy Build-up at Cosmic Dawn”. Additionally, I am an International Associate of the Cosmic DAWN Centre. I obtained my PhD in 2010 at ETH Zurich, after which I moved to UC Santa Cruz as a Hubble Fellow (2010-2013) and then to Yale as a YCAA Fellow (2013-2016). Already starting from my PhD studies, my research has focused on understanding the build-up and assembly of the first generations of galaxies based on panchromatic observations. In particular, I use very deep imaging and spectroscopy from the Hubble and Spitzer Space Telescopes, in addition to ground-based follow-up with Keck, VLT, ALMA, and NOEMA. This allows us to trace the galaxy mass build-up out to z~11, when the Universe was only ~400 Myr old, where we have found the most distant galaxy known so far: GN-z11.

Meghana Killi

I am a student in the integrated MSc+PhD programme at the Cosmic DAWN Center, advised by Dr. Darach Watson.

Beginning in eighth grade, I underwent intensive training for the prestigious Indian Institute of Technology (IIT) entrance exam. I was accepted into the Mechanical Engineering programme at IIT Kharagpur, but after graduating in 2015, I decided to switch tracks and follow my childhood passion for Astronomy.

In 2016, I moved to the US, and began a second Bachelor’s degree in Astronomy at the University of Texas at Austin, where I worked with Dr. Caitlin Casey on submillimeter galaxy observations, and with Dr. Volker Bromm on dark matter theory. Two intense and transformative years later, I graduated with highest honors, and was accepted to DAWN.

I am currently studying the origin of various elements in the universe. More broadly, my research interests lie in our cosmic origins, first stars and galaxies, and events in the very early universe just after the Big Bang.

Clara Giménez Arteaga

PhD student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a PhD student at the Cosmic Dawn Center, advised by Gabriel Brammer. I am currently working on the effects of having spatial resolution observations when deriving the physical properties of galaxies, using recently obtained photometry from the Hubble Space Telescope. With high-resolution line emission maps of nearby galaxies, we can probe sites of ongoing star formation activity and dust reddening. In the coming future, we expect to extend this study to galaxies at high redshift with JWST.

I obtained my Master's degree from DAWN in 2020, and my Bachelor's degree in Physics in 2018 at the University of Barcelona, where I am originally from.

Malte Brinch

PhD Student| The Cosmic Dawn Center (DAWN)
_{DTU Space}

I am a PhD student at the DAWN DTU who formerly defended my MSc at KU, DAWN NBI. My thesis focuses on reverberation mapping of AGN, so as to use them as Distance measurements. As part of my PhD at DAWN, I will be working with Thomas Greve on characterizing the dense molecular gas content in gravitationally lensed starburst and normal galaxies and relate these results to surveys of the dense interstellar medium in local galaxies. I will also work on GISMO 2mm surveys with the Greenland Telescope. I plan to travel to the Thule air base in the fall of 2020 to observe with the GLT.

Vadim Rusakov

PhD student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

My degree at the Cosmic Dawn Center is centered around topics in galaxy evolution, where I am advised by Charles Steinhardt. I am part of research into mechanisms driving the active and quiescent stages of high-redshift galaxies, which is motivated by a mismatch in theoretical predictions and observations of galaxy assembly in the early universe. I am also keen to work on computational problems in research.

I received a Masters degree from the University of Surrey in 2019 studying galaxy evolution in the Local Group with Carme Gallart & Matteo Monelli, while spending part of my degree at the IAC (Tenerife), and a Masters degree from University College London in 2020 doing a project in computational astrophysics with Thomas Greve.e I am advised by Charles Steinhardt. I am part of research into mechanisms driving the active and quiescent stages of high-redshift galaxies, which is motivated by a mismatch in theoretical predictions and observations of galaxy assembly in the early universe. I am also keen to work on computational problems in research.

Katriona (Kate) Mai Landau Gould

PhD student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a PhD student working at the Cosmic Dawn Center advised by Gabriel Brammer. I currently study the formation and evolution of the most massive galaxies in the universe, using a combination of data from ground and space based telescopes across the entire electromagnetic spectrum. I received my Master’s in Astrophysics in 2020 from the University of St Andrews in Scotland, where I worked with Vivienne Wild on post-starburst galaxies

Before deciding to study galaxies, I was interested in particle and astroparticle physics, and had fantastic opportunities to work on experimental projects relating to both cosmic rays and neutrinos at Jodrell Bank Center for Astrophysics and later CERN. I’ve also been lucky enough to do both cosmology and galaxy summer research projects at the Institute of Cosmology and Gravitation and the University of Oxford.

When I’m not doing research I enjoy powerlifting, astronomy outreach, pursuing creative projects and exploring the wonderful city of Copenhagen.

David Blánquez

PhD student| The Cosmic Dawn Center (DAWN)
_{DTU Space, Danmarks Tekniske Universitet}

I am a PhD student at the Cosmic Dawn Centre working under the supervision of Georgios Magdis. I am currently studying the interstellar medium of galaxies across cosmic time using data from the ALMA telescope. The main goal is to measure the amount of gas left on quiescent/dead galaxies in order to place constraints on the mechanisms that prevent them from forming new stars.

I received my master’s degree in Earth and Space Physics and Engineering at the Technical University of Denmark in 2021, after having completed my Bachelor’s degree in Mechanical Engineering (2019) at Tecnun - Universidad de Navarra in San Sebastian (Spain), where I am originally from.

Ting-Yi Lu

PhD student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a PhD student at the Cosmic Dawn Center advised by Charlotte Mason. I am currently working on measuring the morphology of cosmic reionization using the distribution of galaxy Lya emission equivalent widths. By studying the reionization morphology, we can learn about the properties of early galaxies and reveal the reionization process. I use statistical methods such as Bayesian inference, along with the equivalent width distributions from forward modelling the 21cmFAST simulation and the current observations, to reveal the reionization morphology.

Back in Taiwan, I obtained my Master's degree in Astronomy and Bachelor's degree in Physics at National Tsing Hua University. I also worked as a Summer intern at Academia Sinica Institute of Astronomy and Astrophysics and National Central University.

Gonzalo Prieto

PhD student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

Hello! I am a PhD student at the Cosmic Dawn center. I finished both my MSc and undergrad at my home city, Santiago de Chile, at Pontificia Universidad Católica.

My previous research was focused on young galaxies near the epoch of reionization and the intersection between Lyman Break Galaxies and Lyman Alpha Emitters.

At DAWN, I am working with Charlotte Mason as my advisor on the topics of the timeline of Reionization and the morphology of ionized bubbles during Reionization, all of these through the observation and modeling of Lyman Alpha Emitters.

Natalie Allen

PhD student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a first year PhD student at the Cosmic Dawn Centre. I received a first class honours in my integrated masters (MPhys) in Physics with Astrophysics at the University of Sussex. Here I also undertook three summer research placements/internships, where I worked on a JWST proposal for parallel observations of high redshift galaxies, using NIRCAM. My masters work resulted in developing a pure python source extractor, named Automated Source Extractor and Photometry (ASEP) with the use of Numpy and Photutils. ASEP was then used to create a source catalogue of the sources in the HUDF/XDF. Here I learnt about the basics of source extractors and selection of high redshift galaxies with the use of colour-colour criteria.

During my PhD I hope to further build my knowledge of high redshift galaxies, galaxy evolution and the epoch of reionization. My work will allow me to study the most luminous, massive and rare galaxies in the early universe and their properties, morphologies and contribution to reionization.

The highest density regions of the Universe are expected to be the first to collapse in the early universe, and therefore be the sites for the formation of the first galaxies. The most massive and luminous galaxies are expected to form in these regions, and intense UV radiation from their young stars and from smaller galaxies in their vicinity is expected to carve out the first reionized bubbles in the overall neutral IGM.  Wide area surveys are needed to study these regions, which will hopefully lead me to work on data from Hubble, JWST, Euclid and Subaru/Hypersuprimecam.  I am excited for my next few years as a PhD student at DAWN and I can’t wait for the research I am able to produce.

Simone Vejlgaard Nielsen

MSc Student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a master's student working on my thesis under supervision of prof. Johan Fynbo and postdoc Kasper E. Heintz. My thesis will be focusing on using gamma-ray bursts and quasars as sources to study various properties of the interstellar medium in high-redshift galaxies.

Furthermore, I am also very interested in dust-obscured quasars and how the current selection cuts are biased against these quasars, which means that I have previously been involved in projects using modern, unsupervised machine learning methods to de-bias object classifications.

Guozhen Ma

PhD Student| The Cosmic Dawn Center (DAWN)
Niels Bohr Institute, University of Copenhagen

I am currently a second-year master’s student writing my thesis at the Cosmic Dawn Center, supervised by Prof. Johan Fynbo. My thesis is trying to make a complete census of quasars and determine the fraction of dust-obscured quasars. The quasar surveys nowadays are highly biased by the selection effect, since they are all selecting quasars based on the excess of blue light over that of stellar sources but can neglect those quasars reddened by the dust which is actually not rare. I’m also interested in detached BAL quasars, from which we may find features of quasar outflows.

Albert Bjerregård Sneppen

MSc Student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am 1st year graduate student within physics at the Niels Bohr Institute. Currently, I am working with Prof. Charles Steinhardt on possible temperature dependencies of the stellar IMF. Additionally, I have worked on quantifying the effect of using supernova redshifts instead of host galaxy redshifts for measurements of cosmological parameters. Here we have shown that using the more poorly measured redshift from broad supernova emission lines yields a biased cosmology

Rachel Alice Gledhill

MSc Student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a master’s student working on my thesis under the supervision of Victoria Strait. My research focuses on modeling gravitational lensing in a massive galaxy cluster. We hope to improve our understanding of the matter and magnification distribution in this cluster by incorporating new constraints from JWST data.

Isabella Henum

MSc Student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a master's student working on my thesis under supervision of Victoria Strait.  

In my project I will look at data from the Keck Telescope on Mauna Kea in Hawaii - the instrument is called MOSFIRE and observes spectroscopy in the infrared. In my project I will be working with manipulation of 1-D and 2-D spectra and identification of emission lines. One of the end goals of my project is to create a catalog of galaxies with emission lines matched with Hubble Space Telescope imaging data. 

Cecilie Henneberg

MSc Student| The Cosmic Dawn Center (DAWN)
_{Niels Bohr Institute, University of Copenhagen}

I am a 2nd year master’s student at the Niels Bohr Institute. I am writing my thesis at The Cosmic Dawn Center under the supervision of Prof. Johan Fynbo and in collaboration with the NTE (NOT Transient Explorer) group and Mads Nymann-Lynggaard. We are working on creating an exposure time calculator for this new instrument and generating artificial data for testing the pipeline that has been made for NTE.

I completed my bachelor’s degree at the Niels Bohr Institute in 2021.