About Me and My Research

Current focus of my research is intensity mapping of multiple emission lines. This technique is able to map out the Universe and its structure from current time up to the early epoch of reionization and beyond. In my studies I combine simulations tailored for intensity mapping, model analysis, forecasting, parameter estimation and machine learning techniques. Until 2019, I worked as a research assistant at the Scuola Superiore Normale in Pisa, Italy, on cross-studies of hydrogen 21cm intensity mapping and galaxies like Lyman-alpha emitters to probe the late stages of reionization. Before, as a research fellow at the University of Heidelberg, I had kicked off my research on intensity mapping in general scenarios of gravity beyond LCDM. During my Ph.D. at Copenhagen University and as a visiting scientist at the University of California, Irvine, I laid the foundation for my multi-line modelling expertise with simulations of 21cm, Lyman-alpha and H-alpha cosmological volumes and the study of their cross-sginals, as well as sensitivity forecasts for missions like SPHEREx and the Cosmic Dawn Intensity Mapper (CDIM).
Besides my work on multi-line intensity mapping, I also worked to design a convolutional neural network that revolutionizes galaxy deblending as part of the COIN collaboration, developed new Bayesian statistical techniques for bias detection, and demonstrated the detectability of dark energy fluctuations with galaxy clusters. As a research employee at the German Aerospace Center (DLR) in Cologne, Germany, working for the program strategy space, I developed mission concepts and strategies for the space research and technology program. Currently I joined the Hamburg Observatory to continue advancing the intensity mapping technique, supplemented by the application of advanced machine learning within the Platform for Challenges in Data Science as part of the Cluster of Excellence Quantum Universe.

Research Projects

  • Line Intensity Mapping
    as a probe of Astrophysics and the Epoch of Reionization

    I work on simulations tailored for multi-line intensity mapping, to then employ them for parameter, calibration and cross-correlation studies, as well as the creation of realistic mock observations.
    [For a first release of simulations see arXiv:1611.09682]

  • Probing Cosmology
    with Line Intensity Mapping

    Besides multi-line simulations for astrophysics, I also simulate intensity mapping, especially the 21cm line during reionization and cosmic dawn, in general gravity scenarios to explore this novel observable and forecast the feasibility to detect deviations from LCDM.
    [See e.g. arXiv:1805.03629, 1910.02763]

  • Future Missions

    With my simulation-derived realistic mock observations for intensity mapping of multiple lines (Lyman-alpha, H-alpha, 21cm, CII, CO, ..), I provide detectabilty studies and forecasting for upcoming probes like SPHEREx and the Cosmic Dawn Intensity Mapper (CDIM).
    [See arXiv:1903.03144, 1903.03629, 1903.11744]

  • Methods and Tools

    I am also interested in advanced statistical and machine learning tools for astronomy and cosmology. I so far worked on machine learning for galaxy deblending, as well as statistical tests of bias with Bayasian methods and genetic algorithms.
    [See arXiv:1310.8435, 1407.2531, 1905.01324]

Codes

  • The RENOIR project
    Reionization in multi-colour

    The RENOIR-code models hydrogen 21cm, Lyman-alpha and H-alpha emission and surface brightness during the epoch of reionization (redshift z>6) for intensity mapping studies. It is calibrated with obervations of high-redshift galaxies, and is based on the semi-numerical 21cmFAST code (Mesinger et al. '10). Updated calibration and additional emission lines (z.B. CO, CII, OIII) are in progress.
    [language: mostly C, python]

  • Intensity mapping in generalized gravity

    This code simulates both the global signal and intensity maps of 21cm hydrogen emission during reionization and cosmic dawn in generalized gravity scenarios (for an effective gravitational constant, general initial conditions, and/or interacting quintessence).
    [language: C, python]

  • Lyman-alpha emitter (LAE) calibration

    Add-on modules that calculate galaxy LAE maps, with their angular correlation and luminosity function calibrated against observations, and derive cross-statistics with 21cm intensity maps like the real-space and fourier-space cross-correlation coefficients.
    [language: mostly C, python]

  • Mission sensitivity predictions

    A fast code in C that enables the prediction of the sensitivity on intensity mapping power spectra, depending on mission design (e.g. mirror size, instrument temperature) and planning (e.g. integration time).
    [language: C]

  • MapMock

    Takes simulated surface brightness fields and together with instrument sensitivity predictions creates realistic mock observational maps.
    [language: C]

  • Blend2Flux CNN

    Convolutional neural network designed to deblend large samples of galaxy-pairs in photometric images, outputting the flux of the individual galaxies. To be made public within the COIN Cosmostatistics network.
    [language: python with Keras library]

  • Bayesian Robustness for bias detection

    Code that calculates the Bayesian robustness (ratio of evidences) of data sub-samples and compares these to unbiased mock data, to detect possibly biased sub-samples.
    [language: Mathematica]

  • Generalized spherical collapse

    Code that follows the spherical collapse of overdensities while including dark energy perturbations, to calculate characteristic quantities like the density threshold of collapse.
    [available in: Mathematica, Fortran95]

For more information and collaboration, feel free to contact me.

Short CV

Research Experience

2020 - Hamburg University, Observatory of Hamburg, Germany.
Senior Post-doctoral Researcher, Excellence Cluster Quantum Universe.
2019 - 2020 German Aerospace Center (DLR), Germany.
Research Employee.
2018 - 2019 Scuola Normale Superiore, Italy.
Research Associate, mentor: Andrei Mesinger
2017 Institute for Theoretical Physics, Heidelberg University.
Transregio TRR33 Post-doctoral Fellow, mentor: Luca Amendola
2015 - 2016 University of California, Irvine, USA.
Visiting scientist, mentor: Asantha Cooray

Degrees and Programmes

2017 Ph.D. in Physics, Copenhagen University, Denmark.
Thesis Advisors: Steen H. Hansen, David A. Rapetti.
2013 Master of Science Physics, Heidelberg University.
Thesis Advisors: Luca Amendola, Valerio Marra.
2011/12 NPAC, Institut d’astrophysique spatiale, Université Paris-Sud, France.
Thesis Advisor: Nicole Nesvadba.
2010 Bachelor of Science Physics, Heidelberg University.
Thesis Advisor: Matthias Bartelmann.

Awards and Memberships

2019 Marie Sklodowska-Curie Actions Seal of Excellence, call H2020-MSCF-IF-2018.
2019 Member International Astrostatistics Association (IAA).
2018 Top three in Ph.D. prize for best Astronomy Ph.D. thesis in Denmark.
2018 Square Kilometre Array (SKA): Science team member, member synergy focus group.
2018 Member of COIN (Cosmostatistics Initiative).
2017 Transregio33 (The Dark Universe) Post-doctoral Fellowship.
2017 Science working group member: CDIM satellite (Cosmic Dawn Intensity Mapper), NASA.
2015 Member American Astronomical Society (AAS).
2011 Erasmus scholarship for Master studies at Université Paris-Sud 11, France.
2007 e-fellows.net price for online-scholarship programme.
2007 Excellence Award of the German Physical Society (DPG).

Publications

You can find my scientific publications on ADS and arXiv.

Contact Me

Address
Caroline Heneka
University of Hamburg
Hamburg Observatory
Gojenbergsweg 112
21029 Hamburg
Germany
Phone
+49 (soon to be updated)
Email
cosmo[at]caroline-heneka.de