Oliver Müller

University of Strasbourg, Observatoire Astronomique de Strasbourg · France · oliver.muller@astro.unistra.fr

Keystone/Gaëtan Bally.

I am a Swiss astronomer...

... working on dwarf galaxies and near-field cosmology. My Alma Mater is the University of Basel, where I studied physics and astronomy under the supervision of Prof. Bruno Binggeli. I am especially interested in the search for and characterization of dwarf galaxies in nearby galaxy groups. For that purpose I use several different optical telescopes like the Dark Energy Camera, the Very Large Telescope, the Hubble Space Telescope, and the Sloan Digital Sky Survey telescope.

Experience and Education

Working experience

PostDoc as SNF Fellow

University of Strasbourg
since November 2018

PhD in Astronomy

University of Basel
September 2014 - September 2018

Software Developer

match my color, LLC
May 2013 - August 2014

Scientific Assistant

University of Applied Science, Nordwestschweiz
August 2012 - April 2013


University of Basel

Master of Science in Physics
August 2012 - August 2014

University of Basel

Bachelor of Science in Physics
August 2008 - August 2012

Gymnasium Münchenstein

August 2004 - December 2007


WLM galaxy. Captured by ESO’s OmegaCAM on the VLT.

Why studying dwarf galaxies?

Dwarf galaxies are the most abundant and most elusive type of galaxy. And more, they are thought to be the most dark matter-dominated objects in the Universe. They are also quite distinct in size, shape and mass from other galaxies, such as elliptical or spiral galaxies. The barely visible dwarf galaxies are a major puzzle to our understanding of structure formation in the Universe, described by the cosmological dark energy + cold dark matter model. The many discrepancies for dwarf galaxies between theory and observations in small-scale cosmology have now standing names like the Too-Big-Too-Fail problem, the cusp/core problem, or the planes-of-satellites problem.

I have published several papers on the discovery of new dwarf galaxies in our local galactic neighbourhood, the so-called Local Volume, which is a sphere of 10 Mpc (= 33 million light years) around our point of view on Earth. In total these discoveries add up to roughly 10 percent of the known nearby galaxies.

Near-field cosmology with southern group dwarf galaxies

In this project we are carrying out a search for very faint, hitherto undetected dwarf galaxy members of the southern groups of galaxies in Sculptor and Centaurus. The search, done in collaboration with my PhD co-supervisor Prof. Helmut Jerjen of the Australian National University in Canberra, is based on dedicated observations with the wide-field CCD camera of the SkyMapper telescope in Siding Spring, Australia, and the DECam (Dark Energy Camera) at Cerro Tololo Observatory in Chile.

A sky area of totally 750 square degrees covering essential parts of the two groups is being imaged down to significantly fainter magnitudes than previously reached by photographic surveys. Drawing on direct inspection of the deep CCD frames, backed by the application of special filtering techniques which are currently being developed. Multicolor surface photometry and profile modelling for the new, as well as the previously known dwarf members will yield a complete set of structural parameters for the galaxies.

The main scientific questions addressed in collaboration with Dr. Marcel Pawlowski are the following: We will trace the luminosity function of galaxies to very faint magnitudes and use its faint end to put constraints on the processes of baryon settlement in the dark matter minihalos. Furthermore, we will search for anisotropies in the spatial distribution of the new and old dwarfs in the groups; such anisotropies are known to exist in the dwarf satellite members of the Local Group, constituting a major challenge to the standard ΛCDM scenario of structure formation. Last but not least, the newly discovered dwarfs will also provide important targets for follow-up studies. This project is almost done and lead to the six publications: Müller et al. (2015, 2016, 2017a, 2018a, 2018b, 2018c), of which one appeared in Science.

TRGB distance measurements of Cen A dwarf galaxies

To study our newly discovered dwarf galaxies follow-up measurements are conducted with the Very Large Telescope (VLT) at Cerro Paranal, the largest optical telescope in the southern hemisphere. This work, in collaboration with Dr. Marina Rejkuba of the European Southern Observatory (ESO), will give better statistics on the existence of the discovered planes of satellites in the Centaurus Group. Are there two almost parallel planes of dwarf galaxies as suggested by Tully et al. (2015) or is one of the two planes just an artifact from low number statistics as we proposed (Müller et al. 2016)? Intruigingly, we showed that the satellites around Cen A move in a coherent fashion, similar to the planes-of-satellites in the Local Group (Müller et al. 2018a), posing a major challenge to our understanding of structure formation.

Dwarf galaxy survey in the Local Universe

The Local Volume – our local galactic neighbourhood – is still mainly uncharted territory if it comes down to the low-surface brightness population, especially the gas-poor dSph which will remain undetected in large-scale radio surveys.

Together with the Master student Roberto Scalera we survey nearby group of galaxies, beginning with the M101 complex, using the public data from the Sloan Digital Sky Survey (SDSS) (Müller et al. 2017b) and whatever data we can exploit (DES, KiDS, ATLAS and more). Of special interest will be the Canes Venatici cloud with its many dwarf members. The Canes Venatici cloud, together with the Local Group, the Sculptor group and the Centaurus group, forms the socalled Local Sheet, the large-scale filament going through the Local Volume. What will we uncover in such a survey? Will we find ultra diffuse galaxies there? Such dwarf galaxy surveys will lay the foundation for future studies.

To support the efforts to detect such low-surface brightness objects we develop an open-source software, embracing both visual inspection of the image and automated pattern recognition algorithms.

An astronomical image with a hidden dwarf galaxy. Click on this image to apply a Gaussian filter to make the dwarf galaxy visible.

Besides science?

Apart from being a scientist, I am an avid e-guitar player and a proud owner of a Gibson Les Paul (unburst). Additionally, I am an enthusiastic table top player and member of the Tabletop Verein Basilisk, a club dedicated to provide a friendly and lively environment for this hobby, which involves model building, painting, and of course playing.

I also like travel and see new places. Being a scientist certainly helps coming around. When I have free time, especially during my travels I photograph, with focus on landscape and street photography.

When at home, I also like to program (i.e. this and the two previous websites), read books, play games, and write on my blog.

At a seminar with the founder of Shinkendo, Kaiso Toshishiro Obata.

A roadtrip through Iceland, with uncommonly good weather.

Three week hike through Sweden's wilds on the so-called Kungsleden.

Photography. True colour, black beach in Iceland.


Selected peer-reviewed articles

My publication record can be viewed in the ADS database.

  • 2021 · Müller O., Schnider E. „Dwarfs from the Dark (Energy Survey): a machine learning approach to classify dwarf galaxies from multi-band images“, accepted
  • 2021 · Müller O., Pawlowski M., Lelli F., et al. „The coherent motion of Cen A dwarf satellite galaxies remains a challenge for CDM cosmology“, A&A Letters, 645, 5
  • 2020 · Müller O., Marleau F., Duc P.-A., et al. „Spectroscopic study of MATLAS-2019 with MUSE: An ultra-diffuse galaxy with an excess of old globular clusters“, A&A, 640, 10
  • 2019 · Müller O., Rejkuba M., Pawlowski M., et al. „The dwarf galaxy satellite system of Centaurus A“, A&A, 629, 18
  • 2019 · Emsellem E. et al., „The ultra-diffuse galaxy NGC 1052-DF2 with MUSE: I. Kinematics of the stellar body“, accepted for publication in A&A, arXiv:1812.07345
  • 2019 · Müller O., Famaey B., Zhao H. „Predicted MOND velocity dispersions for a catalog of ultra-diffuse galaxies in group environments“, A&A 623, 36
  • 2018 · Kroupa P., Banik I., Haghi H., Zonoozi A.H., Dabringhausen J., Javanmardi B., Müller O., Wu X., Zhao H., „A common Milgromian acceleration scale in nature“, Nature Astronomy, 1
  • 2018 · Kroupa P., Haghi H., Javanmardi B., Zonoozi A.H., Müller O., Banik I., Wu X., Zhao H., Dabringhausen J., „Does the galaxy NGC1052–DF2 falsify Milgromian dynamics?“, Nature 561, E4-E5
  • 2018 · Müller O., Pawlowski M., Jerjen H., Lelli, F. „A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology“, Science 359, 534
  • 2017 · Müller O., Jerjen H., Binggeli B., „New low surface brightness dwarf galaxies in the Centaurus group.“, A&A 597, A7
  • 2015 · Müller O., Jerjen H., Binggeli B., „New dwarf galaxy candidates in the Centaurus group.“, A&A 583, A79
Cover of Science magazine

Our work on the Centaurus group was highlighted on the cover of Science.

Popular science

  • 2020 · Müller O. „Kosmisches Planktor", Spektrum der Wisenschaft
  • 2018 · Müller O. „Von astronomischen Höhen und Tiefen – hinter den Kulissen eines Science Artikels", ScienceBlogs, Schreibwettbewerb, 2. Platz
  • 2018 · Müller O. and Kroupa P. „Nicht so schnell mit MOND – Die Zwerggalaxie NGC1052-DF2 als kritischer Test für MOND und das Dunkle Materie Modell", ScienceBlogs
  • 2017 · Müller O. „Ein Universum ohne Dunkle Materie, ScienceBlogs, Schreibwettbewerb

Book contributions

  • 2018 Müller O., „A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology.“ Conference proceeding to IAU Symposium 344
  • 2017 Müller O., „Glauben an das Unbekannte.“ natura obscura

Media appearances

Selected Articles

  • 2021 · Scientists Find More Evidence That Galaxies Are Synced Up In a 'Cosmic Web' · Vice
  • 2019 · Forscher entdecken eine zweite Galaxie ohne dunkle Materie – und befeuern damit eine langjährige Debatte unter Wissenschaftern · NZZ
  • 2019 · NGC 1052-DF2 – von der MUSE geküsst · ScienceBlogs
  • 2018 · Dancing Dwarf Galaxies Deepen Dark Matter Mystery · Scientific American
  • 2018 · Synchronized Galactic Orbit Challenges Our Best Theory of How the Universe Works · Gizmodo
  • 2018 · Galaxy rotations raise doubts on dark matter · Cosmos Magazine
  • 2018 · New observations of galaxies challenge the standard cosmological model · Ars Technica
  • 2018 · Die Ergebnisse sprechen gegen das Standardmodell · Welt der Physik
  • 2018 · Schweizer Forscher stellt Universum auf den Kopf · 20 Minuten
  • 2018 · Ein Doktorand greift nach den Sternen, die Uni Basel löscht das Licht · TagesWoche
  • 2015 · Basler Game-Studio landet mit erstem Spiel ersten Hit · 20 Minuten


  • 2021 · Zwerggalaxien vs. Dunkle Materie · nano
  • 2018 · The Plane of Satellite Galaxies around Centaurus A · Youtube
  • 2018 · These synchronized galaxies are upending what we know about the universe · Science Magazine
  • 2016 · couch developers · Die Macher


If you are interested in inviting me as a speaker, please write me an e-mail about the occasion. I enjoy talking in front of a crowd, be this in a school or to interested people, and of course for academics as well.