Astrophysics at Oxford: 2010-2015
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
Astrophysicists at Oxford are trying to determine six basic things about the Universe. (1) What is it made of? The Universe appears to be at the beginning of a period of accelerated expansion driven by some mysterious stuff known as 'dark energy'. Einstein had a theory for what this stuff is: he called it the Cosmological Constant. We will be testing his theory by measuring the apparent brightnesses of distant exploding stars (supernovae), by measuring the distortions of distant galaxies as light is bent by the gravity of more nearby galaxies, and by measuring the precise positions of about one million galaxies. (2) What is the history of Hydrogen in the Universe? Hydrogen - the most abundant element in the Universe - is the most important building material for making stars. Atoms of Hydrogen combine into molecules within dense clouds, and these clouds provide the nursery for the birth of new stars. We will be using giant new telescopes operating at millimetre and radio wavelengths to observe, and hence understand, this process throughout most of the history of the Universe. (3) What can we learn about how galaxies formed from galaxies observed at current times? We are involved in large observational programmes that can be viewed as 'archaeology' of nearby galaxies looking for clues of important events in their history, for example by finding fast-moving gas orbiting a dormant supermassive black hole. We also study the relation between stellar populations and dark matter by studying the orbits of stars within and beyond the optical light in a galaxy. (4) What can we learn about how galaxies formed from distant galaxies observed at earlier times? Because of the finite speed of light, distant galaxies are seen when the Universe, and the galaxies within it, were young, and often these galaxies are so dusty that they are only effectively studied using infrared and radio observations. We map out the large-scale distribution of galaxies in the distant Universe using a combination of wide-field imaging (taking pictures) and spectroscopy (spreading light out into its constituent colours). We study these systems as they form and evolve, sometimes in dramatic bursts of star formation associated with supermassive black holes. (5) When did the first galaxies form? The Hydrogen in the Universe formed atoms about 300,000 years after the Big Bang, but was largely re-ionized (converted back to protons and electrons) during the so-called Epoch of Reionization. We use giant ground-based telescopes and satellites (e.g. the Hubble Space Telescope) to study these first galaxies and determine whether it was radiation associated with the birth of these galaxies, or stars within them, that was responsible for the re-ionization. (6) How do black holes influence star and galaxy formation? Black holes grow by 'gobbling up' gas and stars in a process called accretion. This process seems commonly to yield outflows in the form of winds and jets, the latter capable of reaching speeds very close to the speed of light. We study these systems in our own galaxy and in distant galaxies to determine the physics of such 'feedback mechanisms' (growth of the black hole is halted, albeit temporarily, by outflows driven by processes associated with the black hole). Our aim is to understand the influence of (compact) black holes on the formation of stars, galaxies and clusters of galaxies on much large physical scales.
Organisations
- University of Oxford (Lead Research Organisation)
- UNIVERSITY OF EDINBURGH (Collaboration)
- Leiden University (Collaboration)
- California Institute of Technology (Collaboration)
- University of California, Los Angeles (UCLA) (Collaboration)
- UNIVERSITY OF BRITISH COLUMBIA (Collaboration)
- Paris Institute of Astrophysics (Collaboration)
Publications
Awad Z
(2014)
Deuterium chemistry of dense gas in the vicinity of low-mass and massive star-forming regions
in Monthly Notices of the Royal Astronomical Society
Podsiadlowski Philipp
(2014)
The evolution of massive binaries
in Binary Systems, their Evolution and Environments
Davis T
(2014)
The ATLAS3D Project - XXVIII. Dynamically driven star formation suppression in early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Favrie N
(2014)
A thermodynamically compatible splitting procedure in hyperelasticity
in Journal of Computational Physics
Serra P
(2014)
The ATLAS3D project - XXVI. H i discs in real and simulated fast and slow rotators
in Monthly Notices of the Royal Astronomical Society
Booth R
(2014)
Simulations of RS Oph and the CSM in Type Ia Supernovae
in Proceedings of the International Astronomical Union
Young Matthew P.
(2014)
The number of solutions to Mordell's equations in constrained ranges
in arXiv e-prints
Cortese L
(2014)
THE SAMI GALAXY SURVEY: TOWARD A UNIFIED DYNAMICAL SCALING RELATION FOR GALAXIES OF ALL TYPES
in The Astrophysical Journal
McDermid R
(2014)
CONNECTION BETWEEN DYNAMICALLY DERIVED INITIAL MASS FUNCTION NORMALIZATION AND STELLAR POPULATION PARAMETERS
in The Astrophysical Journal
Weijmans A
(2014)
The ATLAS 3D project - XXIV. The intrinsic shape distribution of early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Podsiadlowski P
(2014)
Binary Effects on Supernovae
in Proceedings of the International Astronomical Union
Magdis G
(2014)
A FAR-INFRARED SPECTROSCOPIC SURVEY OF INTERMEDIATE REDSHIFT (ULTRA) LUMINOUS INFRARED GALAXIES
in The Astrophysical Journal
Velander M
(2014)
CFHTLenS: the relation between galaxy dark matter haloes and baryons from weak gravitational lensing
in Monthly Notices of the Royal Astronomical Society
Fu L
(2014)
CFHTLenS: cosmological constraints from a combination of cosmic shear two-point and three-point correlations
in Monthly Notices of the Royal Astronomical Society
Driskill J
(2014)
Wetting transparency of graphene in water.
in The Journal of chemical physics
Mohamed S.
(2014)
3D Models of Stellar Interactions
in Asymmetrical Planetary Nebulae VI Conference
Betoule M
(2014)
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
in Astronomy & Astrophysics
Kylasa S
(2014)
PuReMD-GPU: A reactive molecular dynamics simulation package for GPUs
in Journal of Computational Physics
Shrivastava Anshumali
(2014)
Asymmetric LSH (ALSH) for Sublinear Time Maximum Inner Product Search (MIPS)
in arXiv e-prints
Naab T
(2014)
The ATLAS3D project - XXV. Two-dimensional kinematic analysis of simulated galaxies and the cosmological origin of fast and slow rotators
in Monthly Notices of the Royal Astronomical Society
Smirnov D
(2014)
Effect of exchange interaction on the spin fluctuations of localized electrons
in Physics of the Solid State
Dan M
(2014)
The structure and fate of white dwarf merger remnants
in Monthly Notices of the Royal Astronomical Society
Fogarty L
(2014)
The SAMI Pilot Survey: the kinematic morphology-density relation in Abell 85, Abell 168 and Abell 2399
in Monthly Notices of the Royal Astronomical Society
Maguire K
(2014)
Exploring the spectral diversity of low-redshift Type Ia supernovae using the Palomar Transient Factory
in Monthly Notices of the Royal Astronomical Society
Willert J
(2014)
Leveraging Anderson Acceleration for improved convergence of iterative solutions to transport systems
in Journal of Computational Physics
Dumbser M
(2014)
A posteriori subcell limiting of the discontinuous Galerkin finite element method for hyperbolic conservation laws
in Journal of Computational Physics
Gofford J
(2014)
REVEALING THE LOCATION AND STRUCTURE OF THE ACCRETION DISK WIND IN PDS 456
in The Astrophysical Journal
Duc P
(2014)
Identification of old tidal dwarfs near early-type galaxies from deep imaging and H i observations
in Monthly Notices of the Royal Astronomical Society
Wang X
(2014)
microRNAs are biomarkers of oncogenic human papillomavirus infections.
in Proceedings of the National Academy of Sciences of the United States of America
Korobeinikov I
(2014)
Thermoelectric properties of n-Bi2Te3 - x - y Se x S y solid solutions under high pressure
in Physics of the Solid State
Justham S
(2014)
LUMINOUS BLUE VARIABLES AND SUPERLUMINOUS SUPERNOVAE FROM BINARY MERGERS
in The Astrophysical Journal
Pimbblet K
(2014)
How typical is the Coma cluster?
in Monthly Notices of the Royal Astronomical Society
Meng X
(2014)
THE BIRTH RATE OF SNe Ia FROM HYBRID CONe WHITE DWARFS
in The Astrophysical Journal
Wang D
(2014)
Anomalous luminescence from Yb2+-doped Ca2PO4Cl
in Journal of Luminescence
Scott N
(2014)
Distribution of Slow and Fast Rotators in the Fornax Cluster
Roy P. Deb
(2014)
Polarimetric studies of comet C/2012 L2 (LINEAR)
in Asteroids, Comets, Meteors 2014
Shetty S
(2014)
SALPETER NORMALIZATION OF THE STELLAR INITIAL MASS FUNCTION FOR MASSIVE GALAXIES AT z ~ 1
in The Astrophysical Journal
Hudson M
(2015)
CFHTLenS: co-evolution of galaxies and their dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Houghton R
(2015)
Revisiting the original Morphology-Density Relation
Mould J
(2015)
Black holes in 4 nearby radio galaxies
in Astrophysics and Space Science
Cappellari Michele
(2015)
General spherical anisotropic Jeans models of stellar kinematics: including proper motions and radial velocities
in arXiv e-prints
Description | Canada France Hawaii Telescope Lensing Survey (CFHTLenS) |
Organisation | Leiden University |
Department | Leiden Institute of Physics |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | Miller was responsible for the shear measurements for this international collaboration, and took part in the cosmology analysis. |
Collaborator Contribution | Other aspects of the lensing analysis. |
Impact | Research publications |
Start Year | 2008 |
Description | Canada France Hawaii Telescope Lensing Survey (CFHTLenS) |
Organisation | University of British Columbia |
Country | Canada |
Sector | Academic/University |
PI Contribution | Miller was responsible for the shear measurements for this international collaboration, and took part in the cosmology analysis. |
Collaborator Contribution | Other aspects of the lensing analysis. |
Impact | Research publications |
Start Year | 2008 |
Description | Canada France Hawaii Telescope Lensing Survey (CFHTLenS) |
Organisation | University of Edinburgh |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Miller was responsible for the shear measurements for this international collaboration, and took part in the cosmology analysis. |
Collaborator Contribution | Other aspects of the lensing analysis. |
Impact | Research publications |
Start Year | 2008 |
Description | EarLy unIverse Exploration with nIRspec (ELIXIR) |
Organisation | Paris Institute of Astrophysics |
Country | France |
Sector | Academic/University |
PI Contribution | The Oxford network node has been analysing data from Hubble Space Telescope deep imaging fields (including those from the new WFC3 infrared camera) to determine observing strategies for JWST, and also to provide an initial target list for spectroscopy with NIRSpec on JWST. |
Collaborator Contribution | This is an EU FP7 network associated with the NIRSpec instrument on the James Webb Space Telescope. The Instrument Science Team comprises: Stephane Charlot (IAP, Paris - lead network); Andrew Bunker (Oxford); Marijn Franx (Leiden); Santiago Arribas (Madrid); Roberto Maiolino (Rome); Hans-Walter Rix (MPIA Heidelberg) and Peter Jakobsen (ESA), with out industrial partner (Astrium, Germany). We are responsible for the NIRSpec near-infrared spectrograph, which is being built and tested, and we will execute a 900-hour GTO programme to investigate galaxies at high redshift. The EU FP7 ELIXIR Network is intended to plan the science for this large programme. |
Impact | The Network funds several PhD students and Early Stage Researchers at the nodes across Europe, including two graduate students at Oxford (Joseph Caruana and Silvio Lorenzoni). These researchers have participated in many of the papers from our group, and Lorenzoni has a first-author paper accepted. |
Start Year | 2008 |
Description | Galaxies in the Reionization Epoch |
Organisation | California Institute of Technology |
Department | Caltech Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Oxford has been responsible for reducing the Hubble Space Telescope images and identifying potential high-redshift candidates through colour selection. |
Collaborator Contribution | Oxford has lead this project, in collaboration with Prof Richard Ellis at Caltech, using archival Hubble Space Telescope images with WFC3 to identify Lyman-break galaxies at z=7 and beyond. Caltech has mainly been involved in the spectroscopic follow-up. |
Impact | Five refereed accepted papers so far (Bunker et al. 2010; Wilkins et al. 2010; Lorenzoni et al. 2011; Wilkins et al. 2011, Wilkins et al. 2012). A press release in December 2009, resulting in extensive coverage. Several invited talks at conferences. |
Start Year | 2009 |
Description | Kilo Degree Survey weak lensing collaboration |
Organisation | Leiden University |
Department | Leiden Institute of Physics |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | Responsible for the Point Spread Function modelling and weak lensing shear measurement, employed by the survey. Jointly responsible for cosmology analysis and paper writing. |
Collaborator Contribution | All other aspects of data collection, survey analysis and paper writing |
Impact | Research papers |
Start Year | 2011 |
Description | Kilo Degree Survey weak lensing collaboration |
Organisation | University of Edinburgh |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Responsible for the Point Spread Function modelling and weak lensing shear measurement, employed by the survey. Jointly responsible for cosmology analysis and paper writing. |
Collaborator Contribution | All other aspects of data collection, survey analysis and paper writing |
Impact | Research papers |
Start Year | 2011 |
Description | The WFC3 Spectroscopic Parallel (WISP) Survey |
Organisation | University of California, Los Angeles (UCLA) |
Department | Physics and Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Oxford is responsible for studying the star formation rates of these galaxies from their H-alpha line luminosities, and for constructing the line luminosity function at redshifts around one. |
Collaborator Contribution | The WISP collaboration, based at UCLA and also the Spitzer Science Center (in Caltech) and with collaborators elsewhere in the USA and Germany, is responsible for reducing the Hubble Space Telescope slitless grism spectroscopy to search for emission line objects at high redshift. Most of this reduction and cataloging occurs in Los Angeles. |
Impact | One refereed paper on the initial work - Atek et al. (2010) - and several more in preparation. Various presentations by the team at American Astronomical Society meetings. |
Start Year | 2008 |
Description | Press release on the first Hubble WFC3 Deep Infrared Images |
Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Media (as a channel to the public) |
Results and Impact | We issued a press release on our work on 8 December 2009 entitled "Reinvigorated Hubble Space Telescope Reveals Most Distant Galaxies Yet". Our press release results in extensive coverage in the scientific media and the international press including: Nature Blog http://blogs.nature.com/news/thegreatbeyond/2009/12/ hubble_revisits_distant_haunt.html BBC News (online) http://news.bbc.co.uk/1/hi/sci/tech/8401374.stm We also appeared in The Times (print version) |
Year(s) Of Engagement Activity | 2009 |