Richard Ellis's Homepage

Richard Ellis

Astronomy 249-17, Caltech

Pasadena CA 91125

Position: Steele Professor of Astronomy
Office: (626)-395-2598
Cell: (626)-676-5530
Secretary: (626)-395-4970
Fax: (626)-568-9352
Email: rse@astro.caltech.edu

Overview of Research:

I am working primarily in observational cosmology addressing issues related to the nature of the world model, the origin and evolution of galaxies, the growth of large scale structure and the nature and distribution of dark matter. I am enthusiastic about the use of new instruments and observational opportunities when they further the progress that can be made in these areas. In particular I am involved in promoting and managing the science partnership for the Thirty Meter Telescope.

Recent Outreach Activities:

Read the interview on Searching for the First Stars sponsored by the Kavli Foundation.

Watch the two supernova cosmology teams present reminiscences and anecdotes at Stockholm University as part of the 2011 Nobel Prize in Physics celebrations (WMV format)

Read the Scientific Background on the Accelerating Universe awarded the 2011 Nobel Physics Prize in part to the Supernova Cosmology Project (led by Saul Perlmutter )

Watch the promotional video about the excitement of the Thirty Meter Telescope

Watch an interview about 90 years of gravitational lensing produced for the Royal Society

Listen to an interview on BBC Radio Wales on how I became an astronomer (light entertainment only!)

Scientific Publications:

Check my scientific output on Google Scholar

Past and Present Students:

Check my proud list of successful graduate students!

Research Programs:

My current interests at Caltech fall under 4 main headings:

Gravitational lensing: I have been interested in the role that gravitational lensing can play in cosmology and galaxy formation studies since the late 1980's. I remain hopeful that during my scientific career we can launch an imaging satellite capable of tracing the growth of structure from the time-dependent clustering of dark matter seen from weak lensing signals. On small scales I am using strong lensing to separate dark and baryonic matter distributions in clusters to understand how baryons influence the dark matter profile. Strong lensing also enlarges the apparent sizes of background galaxies and I have used this phenomenon to locate distant galaxies and study their internal properties such as their abundance gradients and velocity fields.

Distant Supernovae: I took part in one of the earliest successful studies to locate and characterize cosmologically-distant Type Ia supernovae and later joined the Supernova Cosmology Project . The resulting "accelerating Universe", recently awarded the 2011 Nobel Prize in Physics, is a bewildering result which has motivated a number of more ambitious ongoing and future supernovae surveys. I am putting most of my effort into examining the validity of using Type Ia SNe for future studies. My research includes examining the environmental dependence of supernova properties as well as the question of possible spectral evolution such as might arise from changes in the progenitor composition. This work is of a long term nature and is being undertaken with spectrographs on Keck and HST.

Large Scale Structure: I have been an enthusiastic promoter of multi-object spectroscopy since the 1980's, working with colleagues to develop early robotic positioners for the former Anglo-Australian Telescope and several multi-slit spectrographs. This work culminated in the 2 degree Field Galaxy Redshift Survey which demonstrated the presence of a baryonic acoustic peak in the large scale distribution of nearby galaxies whose precise measurement at various epochs is a very powerful cosmological probe. I am working with an international team to realize the Prime Focus Spectrograph for the Subaru 8m Telescope as part of the SuMIRe Project . When constructed this instrument will undertake a survey of 4 million faint galaxies to directly map the cosmic expansion history since a redshift 2.

Galaxy Formation and Evolution: I have been interested in studying the properties of distant galaxies since I was a postdoc in the late 1970's. I use the combination of HST images, Spitzer photometry, ground-based K-band imaging and, most of all, Keck spectroscopy to better understand the origin of the wide diversity of galaxy morphologies. Key questions I am working on include the mass-dependent assembly of galaxies over the redshift range 0 to 7, tracing cosmic reionization through statistical measures of Lyman alpha emission in distant galaxies, and the onset of ordered rotation and high velocity dispersions in spiral and elliptical galaxies respectively. I am a recent convert to the phenomenal advances being made in these areas through the use of adaptive optics.