Welcome to my webpage! My name is Edmond Cheung and I'm a postdoctoral fellow at the Kavli IPMU.

My research focuses on galaxy evolution. Specifically, I am interested in the connection between galaxy structure and galaxy evolution. I've studied the dependence of galaxy quenching on inner galactic structure of z~1 AEGIS galaxies, and now I am investigating the role of galaxy bars on galaxy evolution.

When I start my fellowship at IPMU, I'll be working on the MaNGA survey, an SDSS IV project that will provide resolved spectroscopy for 10,000 nearby galaxies.


Figure 3 of Cheung et al. 2013

Bars are thought to be the major drivers of secular evolution. They are also present in up to two thirds of the local disk population, suggesting that they significantly affect galaxy evolution, at least at z~0.

Using Galaxy Zoo 2, I've lead a project in which we searched for evidence of bar-driven secular evolution. Specifically, we explored the behavior of bars as a function of several parameters that are predicted to significantly affect bar-driven secular evolution. The above plot is Figure 3 from Cheung et al. 2013. It shows that the bar likelihood, i.e., the likelihood a bar exists, is related to the properties of a galaxy, indicating that the existence of bars are connected to galaxy properties.

Moreover, these trends match the predictions of bar-driven secular evolution, strongly supporting the theory of secular evolution. This implies that bars are important drivers of galaxy evolution. See Cheung et al. 2013. for more details.


Figure 7 of Cheung et al. 2012

The number of red sequence galaxies has doubled since z~1 while the number of blue cloud galaxies has remained relatively constant. A natural interpretation is that galaxies evolve from blue to red with time, i.e., from star forming to 'quenched.'

In Cheung et al. 2012, I led a project to discover what the underlying physical processes are behind quenching. While we were unable to identify the quenching mechanism, we were able to place strong constraints on the quenching process. We found that red and blue galaxies were best separated by the central stellar surface mass density (see above figure, which is Figure 7 from Cheung et al. 2012), suggesting that whatever quenches galaxies must also significantly increase the central stellar mass of galaxies.


Here is the list of my first author publications:

  • Galaxy Zoo: Are Bars Responsible for the Feeding of Active Galactic Nuclei at 0.2<z<1.0?
  • Galaxy Zoo: Observing Secular Evolution Through Bars
  • The Dependence of Quenching upon Inner Structure of Galaxies
        (Data: Single Sersic Catalog   Bulge Sersic = 4 Catalog   Bulge Sersic = 2 Catalog   README file )

    And co-author publications:

  • Galaxy Zoo: CANDELS barred discs and bar fractions
  • Galaxy Zoo: an independent look at the evolution of the bar fraction over the last eight billion years from HST-COSMOS
  • Serendipitous Discovery of a Massive cD Galaxy at z = 1.096
  • CANDELS: The Progenitors of Compact Quiescent Galaxies at z ~ 2
  • Structural Parameters of Galaxies in CANDELS
  • What Turns Galaxies Off? The Different Morphologies of Star-forming and Quiescent Galaxies since z ~ 2 from CANDELS
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Proucts, and Mosaics
  • CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
  • Teams

    I am a member of the following teams:


    ec2250 at gmail dot com