Studying at MPA

The Max Planck Institute for Astrophysics (MPA) in Garching invites students to carry out their research at MPA. We welcome applicants from Germany and abroad. In principle there are two options for doing research at MPA:

  • Bachelor/Master Thesis
  • PhD Thesis


Bachelor's or Master's thesis

If you are interested in writing your bachelor- or master-thesis in cooperation with LMU/TUM and the MPA, please contact directly the researcher/s offering the project/s you are interested in. Please note that (co-)supervision from a faculty member at LMU or TUM is required, and that if your potential MPA supervisor is not a faculty at the University, he/she will discuss such arrangements with you. Also note that no financial support can be offered by MPA.
Here is a list of projects you can work on at MPA:

MODELING LARGE LYMAN-ALPHA NEBULAE. Advisors: Fabrizio Arrigoni Battaia, Seok-Jun Chang, Max Gronke

Methods:observational / computational

Description: Quasars at high redshifts are usually surrounded by large amounts of gas glowing through the Lyman-alpha line of neutral hydrogen. While the detection of these enormous (often ~100kpc across) nebulae is now — thanks to modern instruments and telescopes sucht as VLT/MUSE — common, it is yet unclear why they exist in the first place and where the energy to power them is coming from. A major hurdle to overcome is to connect theory and observations through the efficient use of radiative transfer models. In this project, you fill deal with data of z~3-4 Lyman-alpha nebulae and try to reproduce them in theoretical models. The (mis)match of these models will provide valuable insights into the gas and photon flows within the nebulae and ultimately what they can tell us about the evolution of galaxies as well as the feeding of their central supermassive black holes.

THE INFORMATION CONTENT OF STACKED SPECTRA Advisors: Seok-Jun Chang, Max Gronke

Research fields: extragalactic astronomy / circumgalactic medium

Methods: theoretical / computational

Description: Electromagnetic radiation is our primary window to observe galaxies and to constrain our theoretical models. In particular, resonant lines such as Lyman-alpha or MgII play a pivotal role in astrophysics as a tool to study low surface brightness region such as the circumgalactic medium. As the detection of a single object is so challenging, it is common practice to perform "stacking" of individual object, thus beating down the noise and enhancing the signal. However, from a theoretical perspective it is unclear what the stacking analysis does to the spectral shape or the information contained in the data. In this project, we will systematically explore the information content of individual spectra versus stacks. To do so, you will run radiative transfer simulations and assemble individual synthetic spectra, perform a stacking analysis, and build a fitting pipeline to obtain the information contained in the stacks.

DOUBLE TROUBLE - MOLECULAR TURBULENT RADIATIVE MIXING LAYERS. Advisors: Max Gronke & Ryan Farber.

Background:

  • Galaxies are in some ways similar to car engines. While a car engine combusts oxygen with hydrocarbon fuel to generate energy and exhaust, galaxies "combust" cold gas with hot gas to generate...more hot or cold gas.
  • Stars can only form from extremely cold, dense gas containing molecular coolants. Thus, whether galactic combustion ultimately generates hot gas or cold gas (and under what conditions) is crucial to understanding how galaxies form and fade.

    • Example Project:

  • Recent work by our group finds the combustion of cold molecular gas is catalyzed by the formation of a cocoon of cool neutral gas which combusts with both ambient hot gas and the molecular gas it appears to protect. However, the precise physics governing such a "double" mixing layer remains to be determined!
  • In this project, you will perform your own cutting-edge MHD simulations of turbulent radiative mixing layers.
    • DERIVATION OF PHYSICAL PARAMETERS FROM GALAXY SPECTRA. Advisor: Guinevere Kauffmann.

    Fitting template spectra from stellar population synthesis models to galaxy spectra to derive physical parameters such as stellar age, metallicity, dust extinction and recent star formation history, has become standard practice in the field. This project will introduce the student to the techniques used for his purpose and provide hands-on experience in coding up simple algorithms described in the literature. We will then move on to exploring some of the unsolved problems in this field, with particular emphasis on probing the stellar content in galactic environments that differ strongly from the disk of our own Milky Way.
    CONSTRAINING DUST LIFECYCLES USING GALAXY SIMULATIONS AND RESOLVED OBSERVATIONS. Advisors: Qi Li & Guinevere Kauffmann.

    Dust reshapes the observed spectral energy distribution. Understanding cosmic dust is therefore essential for our understanding of physical properties of galaxies. Models of dust processes have been recently incorporated in numerical simulations to study the dust lifecycle. These models typically implement dust formation in evolved stars, grain growth by accreting gas-phase metals, destruction via sputtering, and grain-grain collisional processes include shattering and coagulation. However, they suffer great uncertainties. Grain growth, shattering and coagulation in particular have significant impact on the predicted dust mass and grain size distributions, limiting their predicting power for galaxies with a wide range of properties. Resolved observations on dust emission and extinction in galaxies have provided an ideal proving ground for models under various physical conditions. In this project, we aim to combine these observational results with hydrodynamic simulations of galaxies to put a constraint on dust processes. We expect this project to guide the development of state-of-the-art modeling of dust for multiphase environment in the future.


    PhD thesis

    A dissertation in cooperation with MPA can be done as an individually supervised project or through participation in our PhD-programme IMPRS.

    International Max-Planck Research School (IMPRS) on Astrophysics

    In collaboration with the Max Planck Institute for Extraterrestrial Physics (MPE), the Observatory of the Ludwig Maximilians University (USM), and the European Southern Observatory (ESO), MPA offers excellent research opportunities in theoretical and observational astrophysics for IMPRS students, covering all wavelengths from radio waves to gamma rays. Students conduct their graduate studies in a very stimulating environment and have the opportunity to develop a broad background in astrophysics beyond their own dedicated research project. The MPA is one of the most renowned institutions for theoretical and computational astrophysics. Graduate students will receive comprehensive training in theoretical and observational astronomy covering the whole spectrum of research activities present in the participating institutes.

    Link to the IMPRS web pages

    You can find more information about the scientific work at MPA on the webpages of the various research areas:

        Computational Structure Formation
        Galaxy Formation and Evolution
        High Energy Astrophysics
        Physical Cosmology
        Subgalactic Astrophysics
        Information Field Theory

    Programs for PhD students:

    Max Planck PhDnet. It’s a network of Max Planck PhD students! This portal serves as a platform for exchange among doctoral researchers at Max Planck Institutes.
    Christiane Nüsslein-Volhard-Foundation. The foundation supports young female scientists with children and aims to enable them to create the freedom required to further their scientific careers.

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