- Position: Plumian Professor
- Telephone: +44-1223-330879
- Fax: +44-1223-335723
- Email: rse@ast.cam.ac.uk
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.
Research Programmes
I am currently involved in several long-term programmes which
are listed below:
- 2dF galaxy redshift
survey:
this is an approved survey of
over 250,000 galaxies using the wide field multi-fibre system
now in operation at the AAT. Primary aims are to measure the
distribution of galaxies on very large scales, to constrain the
growth in clustering with redshift, to measure redshift space
distortions and to investigate the connection between bias, mean
mass density and luminosity. A team of 20 astronomers in UK and
Australia have joined forces to conduct this survey which is now
the largest systematic redshift survey (see latest
map of the galaxy distribution )
In March 1998 I organised a meeting on Large Scale Structure which was
held in the Royal Society,
London . It provided an opportunity to
discuss
results from 2dF and other projects. The proceedings have appeared in
Phil. Trans. (see Cambridge on-line
version )
- Berkeley-Cambridge
distant
supernovae project:
this is an
ongoing project to find and monitor distant supernovae (SNe) of
Type Ia and, assuming their peak luminosities can be determined
in a consistent manner, estimate the cosmological deceleration
and the rate of supernovae as a function of type and redshift.
A particularly important goal is to eliminate or otherwise models
with a non-zero cosmological constant. HST is being used to track
the most distant SNe (so far up to z=1.2) and provide morphological
types for the host galaxies. The
most recent article on this project discusses
constraints from 42 distant supernovae and provides tantalising
evidence for a non-zero cosmological constant.
-
Resolved studies of distant galaxies:
This is a large HST-based programme to understand the origin of
the faint blue galaxy problem and to place new constraints on
the luminosity and structural evolution of regular massive spirals
and field ellipticals. The datasets being analysed comprise (i)
multicolour HST images of over 300 galaxies with redshifts and
infrared photometry drawn from the CFRS/LDSS surveys and other
archival fields, and (ii) deeper data of the Hubble deep fields
North and South. Plans are underway to conduct integral field
spectroscopy of selected sources from these catalogues.
Recent results on the
declining number of galaxies with irregular morphology
and the
slow growth of disk galaxies have appeared in Ap.J. Further work on
the assembly
history of field ellipticals and origin of bulges and
bars is appearing shortly.
- Gravitational lensing: I coordinate a European collaboration
under the auspices of
European Union TMR network which aims to exploit HST optical and
infrared images and ground-based spectroscopy for addressing the
nature of faint galaxies and the distribution of dark matter on
various scales from precise mass modelling.
- The above programmes are being augmented by new instrument developments
recently completed at Cambridge. These include a panoramic near-IR
4 x 1024 x 1024 HgCdTe camera successfully commissioned at
La Palma and now executing
a major survey at Las Campanas in association
with Carnegie Observatories , and
a near-IR OH suppressed spectrograph
which offers both multi-object and integral field capabilities which
is being developed as a fast-track instrument for Gemini
. These instruments are aimed at
exploring the clustering, star formation characteristics and
evolutionary behaviour of galaxies within the important era
1 < z < 2.5 where relatively little data is currently
available.
Current Committees
Latest Papers (1999 submissions)
Hubble Space
Telescope Imaging of the CFRS and LDSS Redshift Surveys - IV:
Influence of mergers in the evolution of faint field galaxies from
z~1
Lensed Galaxies in Abell
370 II. The ultraviolet properties of arcles and the star formation rate
at high redshift
CIRPASS - a Near-Infrared Integral Field Spectrograph
Hubble Space
Telescope Imaging of the CFRS and LDSS Redshift Surveys - III: Field
Ellipticals at z=0.2-1
Hubble Space
Telescope Near-Infrared and Optical Imaging of Faint Radio Sources
in the Distant Cluster Cl0939+4713
The 2dF Galaxy
Redshift Survey: Spectral Type and Luminosity Functions
A Spectroscopic
Redshift for the Cl0024+16 Multiple Arc System: Implicatios for the
Central Mass Distribution
The Star Formation
Histories of Galaxies in Distant Clusters
A Spectroscopic
Catalog of 10 Distant Rich Clusters of Galaxies
Recent Review Articles
The Formation and Evolution of Galaxies
Nature 395, A3-8 1998
Faint
Blue Galaxies Annual Reviews Astronomy and Astrophysics 35 (389) 1997
Curriculum
Vitae (MS Word)
Publication List
(250kb postscript)
Links:
Institute of Astronomy
Richard's Bookmarks
Not-the-RSE Web page
Donations welcome!
Page maintained by Richard Ellis rse@ast.cam.ac.uk
Last modified : 1st July 1999