Dr. Martin Dominik

Research Theme:
St. Andrews
Email address:
Telephone number:
+44 (0)1334 463068
School of Physics & Astronomy, Physical Science Building, North Haugh, St Andrews, KY16 9SS, United Kingdom

Research interests

Martin Dominik is a Royal Society University Research Fellow at the School of Physics & Astronomy at the University of St Andrews. His research focuses on applications of the gravitational microlensing effect, and in particular on its potential for studying planets orbiting stars other than the Sun.

Gravitational microlensing events arise from the bending of light of observed stars caused by the gravity of an intervening stellar or sub-stellar mass object, resulting in a characteristic transient brightening (photometric signature) and a shift of the centroid of light (astrometric signature). Observing these signatures can provide us with population statistics of faint or unseen objects over a mass range spanning more than 9 decades, from black holes over neutron stars, white dwarfs, brown dwarfs, gas- and ice-giant planets, super-Earths and rocky planets, down to satellites of Lunar mass.

While more than 1000 extra-solar planets have been reported, revealing an amazing diversity, there is still uncharted territory remaining to be explored, namely towards lower planet masses and temperatures. Gravitational microlensing is uniquely suited to fill this gap of knowledge with its detection sensitivity peaking beyond the snow line.

Dominik is the co-PI and Science Coordinator of the MiNDSTEp campaign, which monitors ongoing gravitational microlensing events with high-quality photometry at high cadence, after previously having been co-PI of the PLANET collaboration, which in 1995 established the first round-the-clock microlensing follow-up network, and led the detection of 5-Earth mass planet OGLE-2005-BLG-390Lb, which provided the first observational hint for Earth-like planets being common in the Universe. Dominik is also a co-I of the RoboNet campaign, using a network of 1m and 2m robotic telescopes, including the three SUPAscopes, which form part of the LCOGT network. He is PI of the ARTEMiS project, providing a software system for real-time data modelling, visualisation, and implementation of an efficient strategy, which steers the automated target selection of both the MiNDSTEp and RoboNet campaigns.

While upcoming high-cadence wide-field microlensing surveys are now set to probe the mass function of cold planets down to Earth mass, Dominik is currently developing lucky imaging photometry for the MiNDSTEp and RoboNet campaigns in order to extend the sensitivity by a further two decades in mass, reaching even beyond the Moon.

On the other end of the mass spectrum, Dominik is co-I of a project to identify isolated stellar-mass black holes by means of astrometric microlensing.


Martin Dominik has been teaching General Relativity, as well as selected lectures of the SUPA Astrobiology course.

Research outputs

  1. High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016 DOI
    D. F. Evans, J. Southworth, B. Smalley, U. G. Jørgensen, M. Dominik, M. I. Andersen, V. Bozza, D. M. Bramich, M. J. Burgdorf, S. Ciceri et al., Astronomy & Astrophysics, 610 (2018)
  2. OGLE-2014-BLG-0289 DOI
    A. Udalski, C. Han, V. Bozza, A. Gould, I. A. Bond, P. Mróz, J. Skowron, Ł. Wyrzykowski, M. K. Szymański, I. Soszyński et al., Astrophysical Journal, 853, 1 (2018)
  3. RoboTAP DOI
    M. Hundertmark, R. A. Street, Y. Tsapras, E. Bachelet, M. Dominik, K. Horne, V. Bozza, D. M. Bramich, A. Cassan, G. D'Ago et al., Astronomy & Astrophysics, 609 (2018)
  4. OGLE-2016-BLG-1190Lb DOI
    Y. H. Ryu, J. C. Yee, A. Udalski, I. A. Bond, Y. Shvartzvald, W. Zang, R. Figuera Jaimes, U. G. Jorgensen, W. Zhu, C. X. Huang et al., Astronomical Journal, 155, 1 (2017)
  5. Ground-based parallax confirmed by Spitzer. Binary microlensing event MOA-2015-BLG-020 DOI
    Tianshu Wang, Wei Zhu, Shude Mao, I. A. Bond, A. Gould, A. Udalski, T. Sumi, V. Bozza, C. Ranc, A. Cassan et al., Astrophysical Journal, 845, 2 (2017)
  6. Microlensing constraints on the mass of single stars from HST astrometric measurements DOI
    Noé Kains, A. Calamida, K. C. Sahu, S. Casertano, J. Anderson, A. Udalski, M. Zoccali, H. Bond, M. Albrow, I. Bond et al., Astrophysical Journal, 843, 2 (2017)
  7. OGLE-2014-BLG-1112LB DOI
    C. Han, A. Udalski, V. Bozza, M. K. Szymański, I. Soszyński, J. Skowron, P. Mróz, R. Poleski, P. Pietrukowicz, S. Kozłowski et al., Astrophysical Journal, 843, 2 (2017)
  8. MOA-2016-BLG-227Lb: a massive planet characterized by combining light-curve analysis and Keck AO imaging DOI
    N. Koshimoto, Y. Shvartzvald, D. P. Bennett, M. T. Penny, M. Hundertmark, I. A. Bond, W. C. Zang, C. B. Henderson, D. Suzuki, N. J. Rattenbury et al., Astronomical Journal, 154, 1 (2017)
  9. Relativistic deflection of background starlight measures the mass of a nearby white dwarf star DOI
    Kailash C. Sahu, Jay Anderson, Stefano Casertano, Howard E. Bond, Pierre Bergeron, Edmund P. Nelan, Laurent Pueyo, Thomas M. Brown, Andrea Bellini, Zoltan G. Levay et al., Science, 356, 6342 , p. 1046-1050 (2017)
  10. Faint source star planetary microlensing DOI
    N. J. Rattenbury, D. P. Bennett, T. Sumi, N. Koshimoto, I. A. Bond, A. Udalski, Y. Shvartzvald, D. Maoz, U. G. Jørgensen, M. Dominik et al., Monthly Notices of the Royal Astronomical Society, 466, 3 , p. 2710-2717 (2017)
Last updated: 17 Apr 2018 at 21:13