
Prof. Stephen Serjeant
Professor Of Astronomy
Biography
Professional biography
For more detailed and up-to-date information, please visit my research pages at https://stephenserjeant.github.io/
Publications
All publications to date (more complete than the list below, maintained by the NASA Astrophysics Data System)
Preprints (maintained by arXiv.org)
Books
- An Introduction to Galaxies and Cosmology (2015, CUP). Mark H. Jones, Robert J.A. Lambourne and Stephen Serjeant
- Galaxies, Stars and Planets (2012, Open University Press). Simon Clark, Simon Green and Stephen Serjeant
- Observational Cosmology (2010, CUP). Stephen Serjeant
- Earth and Space (2007, Open University Press). Stephen Blake, Stephen Serjeant, Sandy Smith
Observational Cosmology has been very carefully studied by years of OU undergraduates, during which time several errata have been spotted. The errata found from 2010-13 are included here (PDF), and the errata found from 2013-present are here (PDF).
Research, teaching, collaborations and impact interests
For a list of my research interests, teaching interests, impact and engagement, please visit my personal web pages.
Projects
SA-DISCNet: A collaborative data science training network across southern Africa and southern UK
Data intensive science is a major global growth area, as the volume, complexity and rate of digital data within governments and companies continues to rapidly increase. At the same time, powerful analysis techniques continue to evolve for obtaining radical insights into large datasets, including finding clusters and anomalies, as well as detecting and predicting dominant trends and correlations in such data. This data intensive science comes at a crucial time for global development. Major worldwide challenges, as encapsulated in the United Nations' Sustainable Development Goals (SDGs), require multidisciplinary solutions, many of which include data science. Moreover, the South African National Development Plan (NDP) for 2030 recognises the need to "sharpen its innovative edge and continue contributing to global scientific and technological advancement" and "shift to a more knowledge-intensive economy". We therefore propose to build a training network in data intensive science between universities in southern UK and partners in southern Africa to help address these SDGs and NDP priorities. The cornerstones of this network will be the `Data Intensive Science Centre in SEPnet' (DISCnet) and the African Institute of Mathematical Science (AIMS) South Africa. Together, we will pilot an innovative course of training and internships for the next generation of data analysts, focusing on solving SDG-related questions in South Africa and acting as a driver of the country's economy in the 21st century. Our aim with this pilot training programme is to equip and send students to solve data science problems associated with sustainable development goals (SDGs) in SA and beyond. The specific goals of the pilot programme are to: (i) Deliver an initial cohort of at least 10 highly trained African data scientists; (ii) Provide a world-class data science school to African students, leveraging existing DISCnet training material; (iii) Prime-pump a new 8-week hand-on data science training course at AIMS with contributions from DISCnet; (iv) Contribute to the sustainable development goals via 3 month strategic student internships with South African organisations and companies, focusing on economic development and welfare; (v) Understand the details of managing an extended, sustainable training network across southern Africa. This pilot leverages considerable investment from STFC, our university partners, and the Royal Society (RS). Our long-term ambition is to create a sustainable network of comparable scale to DISCnet, e.g. approximately 25 African STEM students per year receiving our specialist training. These students will become the future data science leaders in Africa.
The Astronomy Dark Matter Test Science Project
The test science projects (TSPs) are essential exemplars of addressing major/global challenges for Europe's societies, demonstrating how research infrastructures can align to support Horizon Europe's missions within the EOSC. The successful EOSC-Future/ESCAPE Dark Matter TSP achieved this by creating common tools and EOSC services for high energy/astroparticle dark matter detection experiments. However, all the experimental evidence for dark matter is currently in the form of inference from observational astronomy, yet there are no shared tools or services for observational astronomers to access or interpret the results of direct detection dark matter experiments, and vice versa. Funding and time limitations in the ESCAPE Dark Matter TSP meant that the only cross-disciplinary synergies that could be achieved were between high energy particle physics and the astroparticle physics communities and facilities. We therefore propose the Astronomy Dark Matter Test Science Project as the natural extension of the ESCAPE Dark Matter TSP.
ELSA: Euclid Legacy Science Advanced Analysis Tools
Euclid is an ESA space telescope launching in July 2023, designed to understand the nature of dark energy and dark matter. To achieve this, Euclid will observe over a third of the sky with high resolution imaging and spectroscopy, which will establish “the” reference map of the extra-galactic celestial sphere for decades to come. The giant archive produced will be a goldmine to study the history of the formation and growth of galaxies over the age of the Universe, driving answers to many fundamental science questions on the co evolution of galaxies and supermassive black holes, the interaction between stars, gas, and galactic nuclei in galaxies at cosmic noon, and excelling in the discovery of rare objects including gravitational lenses. However, the richest gold veins are also the most difficult to exploit: the tools developed for Euclid’s primary science will not be enough to open the rich legacy for the astronomical community. We therefore propose ELSA to explore new methodologies and create cutting-edge pipelines, tools and algorithms. Our ambitious goal is to push the boundaries of spectroscopic analysis to the limits, uncovering hidden details of even the faintest and rarest galaxies measured by Euclid. We will leverage state of the art machine learning to efficiently handle the high-dimensional data and reveal the underlying physical processes they encode. This will need dedicated computing resources and highly motivated researchers versed in the most advanced techniques, that will work with our team of leading experts in the field of galaxy evolution to reveal the treasures preserved in the Euclid vault. Our machine learning will be supplemented by citizen science, enormously extending the reach of ELSA’s impact. ELSA will be a forge of knowledge and advanced tools that will not be confined within the boundaries of our teams, but shared with the whole scientific community and beyond to foster new projects and unforeseen discoveries.
Astrophysics Center for Multimessenger studies in Europe
We will bring together scientists from the adjacent fields of astroparticle physics and astronomy, focusing on the complementarity of their approaches and encompassing methods to study extreme astrophysical objects and transient events, by using the multi-messenger and multi-wavelength techniques. This working method involves a set of research infrastructures working together in a coordinated way to share complementary data, expertise and best practices with their users – both scientists and technical staff – in a novel and innovative collaboration at European level. Training for the young scientist is also a requisite for establishing a sustainable program.
STFC Centre For Doctoral Training In Data Intensive Science
STFC Centre for Doctoral Training in Data Intensive Science
European Science Cluster of Astronomy & Particle physics ESFRI research infrastructures
Response to Horizon 2020 European Open Science Cloud call. The bid is being led by Giovanni Lamanna (CNRS). - The current ESFRIs and pan European International organisations participating in such a cluster are: SKA, CTA, KM3NeT, HL-LHC, FAIR, E-ELT, ESO, CERN, JIVE, EST (tbc); other partners such as data centres, e-infrastructures (IVOA et al.) and national centres would be also involved. The commitment and the participation (as beneficiaries) of those EFSRI projects that are also legal entities are foreseen (e.g. SKA Organisation, CTA Observatory, FAIR). - The work-programme has been decided and the leaderships agreed: WP1) Management, networking and dissemination (CNRS-IN2P3). Coordinator: Giovanni Lamanna (LAPP-CNRS). WP2) “Data lake” infrastructures concept: design and implementation (CERN/HL-LHC, SKA, CTA, et al.) Leader: Ian Bird (CERN) WP3) Open-source scientific software and service repository (-> EOSC catalogue) (KM3NeT/FAU, CTA/LAPP, SKA, et al.) Leader: Kay Graf (FAU) WP4) Data (interoperable archives and preservation) (CDS-CNRS, ESO/E-ELT, et al.). Leader: Mark Allen (CDS-CNRS) WP5) Open-science platform (ASTRON/SKA, CTA, et al.). Leader: Michael Wise (ASTRON) WP6) Engagement and Communication (OU, CNRS- LAPP OU TRUST-IT) leader : Stephen Serjeant
STFC CDT DISCNET 2
The DISCnet vision is to train the Data Science Leaders of the future. DISCnet accelerates the pace of scientific discovery in the understanding of our Universe and its fundamental particles through the application of cutting-edge Data Intensive Science. Our centre attracts top students from the physical sciences, and develops them into innovators adept at working in academic and commercial environments, equipped with enviable technical skills, and armed with the full appreciation of uncertainty in decision-making applications that comes from a rigorous scientific background. This enables them to lead disruptive change, potentially transforming sectors of the economy to position the UK at the forefront of the global data revolution. Their diverse and inclusive career network facilitates a life-long capability to develop themselves and to influence others. We have established DISCnet as a national hub of research excellence across three world-class universities, embedded within a global network of premier scientific facilities, and with an industrial placement programme that will directly connect innovation in computational science and fundamental physics to the UK economy.
Consolidated Grant - Astronomy Observation and Astronomy Theory (AO & AT 2016)
Our research programme, Astronomy at the Open University, covers the breadth of cosmic evolution, from dark energy to the birth of planets. We do this research by observation, laboratory experiments, simulations and modelling. We use purpose-designed laboratories and instruments, and instruments on telescopes and spacecraft to make our observations and measurements. Our group is based in the Department of Physical Sciences at the OU. So what are we trying to find out? We have 8 separate projects, from exoplanets and stars to distant galaxies. We already know a lot about how the Solar System came about. The Sun and planets formed from a cloud of dust and gas about 4570 million years ago. The cloud collapsed to a spinning disk and dust and gas spiralled inwards. The core of the disk became hot, forming the Sun, while the leftover dust and gas formed the planets. Boulders gravitated together to make planets, but no-one knows how the dust grains became boulders. We are experimenting with colliding centimetre-sized particles in zero-gravity conditions to see if they stick together, to find the missing link in how planets form. We also look at processes that cause stars to change as they age. Only recently has it been recognised that so many stars are binary systems, where two or more stars are in close association and affect each others' motion. Such systems affect the way mass and energy is lost from a star, and how they are transferred into the interstellar medium. We will study how 'binarity' affects the behaviour of massive stars (>20 times the mass of the Sun) and low mass stars (< the mass of the Sun), and how star populations change as they age. Studying these effects is vital, because the environment of a star influences any planets that surround it. Many hundreds of planets have been discovered around other stars (exoplanets) and we are working to describe the range of properties of these planets, especially when they are located close to their central star. A star can even completely destroy a close-in exoplanet, which could be an important new source of dust in the nearby universe and even in distant galaxies in the early Universe. Also in the early Universe, we can use the way that galaxies warp space and time to learn about the dark matter that surrounds them, and the dark energy that drives them apart. What else do we do? We build and test instruments for ground-based telescopes and for space missions, striving to make them smaller and lighter, and explore how they can be used on Earth for medical or security purposes. One of the most important benefits of our research is that it helps to train and inspire students: the next generation of scientists and engineers. We also enjoy telling as many people as possible about our work, and what we have learned from it about our origins.
Astronomy ESFRI and Research Infrastructure Clusters
15 million euro response to INFRADEV-4 to support all major European research infrastructures in astronomy, in the ESFRI roadmap. The OU is leading the outreach work package, with a maximum value of approx. 0.5 million euro.
STFC DTG 2015 - 2016 (2015 Intake)
STFC DTG Quota 2015-16 AMS record for students starting on or after 01/10/2015
Visitor funding for disadvantaged Southern African PDRAs to the UK
Visitor funds for NRF PDRAs and Stobie PhD students to the UK SALT Consortium
UK SPICA-SAFARI Team Funding Request for Phase 0
UKSA funding for staff time and travel funds for development of the SPICA project, currently shortlisted for the ESA M5 slot (550 million euros).
SPICA Phase-A proposal to UKSA
The SPICA space mission has been selected by the European Space Agency for detailed study as a candidate for its M5 mission, with launch expected around 2030. SPICA is designed to be a powerful astronomical observatory with potential to contribute to many areas of research, but particularly to the study of planet formation and galaxy evolution. The Phase-A study is currently underway, having started in April 2019, and will finish in mid-2021, at which time ESA will select the mission to be flown as M5. SAFARI is the SPICA observatory's far infrared instrument, and as one of the UK institutes participating in the SPICA-SAFARI team, the OU is involved in a number of activities in this phase.
STFC ODA Institutional Award
STFC ODA Institutional Award
Ogden Science Officer / Citizen Science Research Fellow
The Ogden Trust is providing matched funding to a maximum of £75k for 3 years for an 0.5 FTE outreach post, that we can add to the ASTERICS post and can therefore recruit a full-time postdoctoral research assistant.
Astronomy and Planetary Sciences at the Open University
The aim of our programme in Astronomy & Planetary Science at the Open University (APSOU) is to carryout detailed investigations of the origin and evolution of galaxies, stars and planets with a special emphasis on our own Solar System through a combination of observation, simulation, laboratory analysis and theoretical modelling. Our research is divided into two broad areas, reflecting the historical research strengths. This research programme is well-matched to both nationally- and internationally-agreed research imperatives. In its final report, A Science Vision for European Astronomy2, Astronet’s Science Working Group identified four broad areas of strategic importance; our research covers major topics within each of these areas. APSOU projects also map onto two of the four Science Challenges that form STFC’s Road Map3 for science (‘How did the universe begin and how is it evolving?’ and ‘How do stars and planetary systems develop and is life unique to our planet?’). The present APSOU programme comprises 20 projects (labelled A to T), of which 6 are for consideration by the Astronomy Observation (AO) panel, 1 for Astronomy Theory (AT), and 13 for the Planetary Studies (PL) panel. The AO projects cover the breadth of the 7 themes recognised as UK strengths in the report of STFC’s Astronomy Advisory Panel (AAP), whilst the 13 PL projects are directed towards answering questions raised in two of the three themes identified as UK strengths in the roadmap of STFC’s Solar System Advisory Panel (SSAP)4.
Publications
Book
Book Chapter
First results from the AKARI FU-HYU mission program (2009)
AKARI detections of submm galaxies, and vice versa (2009)
AKARI observation of early-type galaxies in Abell 2218 (2009)
The deepest image of the universe at a wavelength of 15 microns (2009)
The Herschel ATLAS Key Project (2009)
The AKARI deep fields: early results from multi-wavelength follow-up campaigns (2009)
AKARI far-infrared deep galaxy survey (2008)
Deep Optical and Near-IR Observations of the XMM/Chandra Regions in ELAIS (2003)
Dataset
AKARI NEP-Deep field mid-IR source catalogue (2011)
PAH luminous galaxies at z~1 (2011)
20cm survey of the AKARI NEP (2010)
AKARI photometric redshift accuracy (2010)
ULIRGs galaxies in SDSS, 2dF and 6dF (2007)
Final analysis of ELAIS 15-$mu$m (Vaccari+, 2005) (2005)
Chandra/ELAIS mid-infrared sources (Manners+, 2004) (2005)
Hubble Deep Field and Flanking Fields (Serjeant+, 2003) (2005)
ELAIS: final band-merged catalogue (Rowan-Robinson+, 2004) (2004)
Digital Artefact
Journal Article
Strong gravitational lenses from the Vera C. Rubin Observatory (2025)
Euclid : A complete Einstein ring in NGC 6505 (2025)
The detection of strongly-lensed submillimetre galaxies (2025)
A GMRT 610 MHz radio survey of the North Ecliptic Pole (NEP, ADF-N) / Euclid Deep Field North (2024)
A novel high-z submm galaxy efficient line survey in ALMA bands 3 through 8 - an ANGELS pilot (2024)
Euclid preparation : XLIX. Selecting active galactic nuclei using observed colours (2024)
Gas conditions of a star-formation selected sample in the first billion years (2024)
Overcoming Confusion Noise with Hyperspectral Imaging from PRIMAger (2024)
Effects of galaxy environment on merger fraction (2024)
A dusty proto-cluster surrounding the binary galaxy HerBS-70 at z = 2.3 (2024)
Euclid preparation : XXXVIII. Spectroscopy of active galactic nuclei with NISP (2024)
Citizen science in European research infrastructures (2024)
FLASH: Faint lenses from Associated Selection with Herschel (2024)
Using cGANs for Anomaly Detection: Identifying Astronomical Anomalies in JWST Imaging (2023)
z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies : I. Overview (2023)
Citizen Science in the European Open Science Cloud (2023)
Deep ALMA redshift search of a z ∼ 12 GLASS-JWST galaxy candidate (2023)
z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies (2023)
Searching for giant planets in the outer Solar System with far-infrared all-sky surveys (2022)
Massive Molecular Gas Reservoir in a Luminous Submillimeter Galaxy during Cosmic Noon (2022)
Super-resolving Herschel imaging: a proof of concept using Deep Neural Networks (2021)
An Active Galactic Nucleus Recognition Model based on Deep Neural Network (2021)
Close-up view of a luminous star-forming galaxy at z = 2.95* (2021)
A high redshift population of galaxies at the North Ecliptic Pole (2020)
The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description (2020)
Using Convolutional Neural Networks to identify Gravitational Lenses in Astronomical images (2019)
The strong gravitational lens finding challenge (2019)
What do astronomers want from the STFC? (2019)
Probing the high-redshift universe with SPICA: Toward the epoch of reionisation and beyond (2018)
The Herschel-PACS North Ecliptic Pole Survey (2018)
ALMA observations of lensed Herschel sources: testing the dark matter halo paradigm (2018)
A dusty star-forming galaxy at z = 6 revealed by strong gravitational lensing (2018)
Finding bright z ≥ 6.6 Ly α emitters with lensing: prospects for Euclid (2017)
SONS: The JCMT legacy survey of debris discs in the submillimetre (2017)
Hyper Suprime-Camera Survey of the Akari NEP Wide Field (2017)
NEP-AKARI: Evolution with redshift of dust attenuation in 8µm selected galaxies (2017)
The AGN population in the AKARI NEP Deep Field (2017)
Radio identifications in the NEP Deep Field (2017)
AKARI Deep Field South: spectroscopic observations of infrared sources (2017)
Herschel observations in the AKARI NEP field: initial source counts (2017)
Overview of North Ecliptic Pole deep multi-wavelength survey (NEP-DEEP) (2017)
Galaxies on diet: feedback signatures in radio-AGN host galaxies (2017)
The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts (2017)
The Radio-far Infrared Correlation in the NEP Deep Field (2017)
The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES) in the South Ecliptic Pole field (2016)
H-ATLAS: a candidate high redshift cluster/protocluster of star-forming galaxies (2016)
Rest-frame optical spectra and black hole masses of 3 <ɀ<6 quasars (2015)
Extragalactic sources in Cosmic Microwave Background maps (2015)
Dust attenuation up toz≃ 2 in the AKARI North Ecliptic Pole Deep Field (2015)
Lens models of Herschel-selected galaxies from high-resolution near-IR observations (2014)
The first source counts at 18 m from the AKARI NEP Survey (2014)
Constraints on the galaxy 'main sequence' at z > 5: the stellar mass of HDF850.1 (2014)
Up to 100,000 reliable strong gravitational lenses in future dark energy experiments (2014)
Optical – near-infrared catalog for the AKARI north ecliptic pole Deep field (2014)
Herschel-ATLAS: deep HST/WFC3 imaging of strongly lensed submillimetre galaxies (2014)
A tale of two feedbacks: star formation in the host galaxies of radio AGNs (2014)
H2O emission in high-z ultra-luminous infrared galaxies (2013)
The North Ecliptic Pole Wide survey of AKARI: a near- and mid-infrared source catalog (2012)
Herschel-ATLAS/GAMA: spatial clustering of low redshift submm galaxies (2012)
The synergy of large area surveys with AKARI and HERSCHEL (2012)
Detection of Hα emission from z>3.5 galaxies with AKARI-FUHYU NIR spectroscopy (2012)
A multi-wavelength view of galaxy evolution with AKARI (2012)
Overview of the North Ecliptic Pole multi-wavelength survey (NEP-DEEP) (2012)
Strong biases in infrared-selected gravitational lenses (2012)
A comprehensive view of a strongly lensed Planck-associated submillimeter galaxy (2012)
A deep ATCA 20cm radio survey of the AKARI Deep Field South near the South Ecliptic Pole (2012)
Herschel-ATLAS: toward a sample of ~1000 strongly lensed galaxies (2012)
The AKARI NEP-Deep survey: a mid-infrared source catalogue (2012)
Herschel-ATLAS: rapid evolution of dust in galaxies over the last 5 billion years (2011)
Far-infrared luminosity function of local star-forming galaxies in the AKARI Deep Field-South (2011)
Detection of the cosmic far-infrared background in the AKARI Deep Field South (2011)
GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxies (2011)
Herschel-ATLAS: first data release of the Science Demonstration Phase source catalogues (2011)
Infrared luminosity functions of AKARI Sloan Digital Sky galaxies (2011)
Observation of H2O in a strongly lensed Herschel-ATLAS source at z = 2.3 (2011)
The JCMT nearby galaxies legacy survey VI. The distribution of gas and star formation in M81 (2011)
Spitzer imaging of Herschel-ATLAS gravitationally lensed submillimeter sources (2011)
Multi-wavelength probes of distant lensed galaxies (2011)
A pilot study for the SCUBA-2 ‘All-Sky’ Survey (2011)
The detection of a population of submillimeter-bright, strongly lensed galaxies (2010)
A deep survey of the AKARI north ecliptic pole field (2010)
Herschel ATLAS: the cosmic star formation history of quasar host galaxies (2010)
Herschel-ATLAS: extragalactic number counts from 250 to 500 microns (2010)
Herschel-ATLAS: evolution of the 250 µm luminosity function out to z=0.5 (2010)
A search for debris disks in the Herschel-ATLAS (2010)
Polycyclic aromatic hydrocarbon (PAH) luminous galaxies at z ~ 1 (2010)
Source counts at 15 microns from the AKARI NEP survey (2010)
The AKARI FU-HYU galaxy evolution program: first results from the GOODS-N field (2010)
AzTEC half square degree survey of the SHADES fields – I. Maps, catalogues and source counts (2010)
H-ATLAS: PACS imaging for the Science Demonstration Phase (2010)
Herschel-ATLAS: blazars in the science demonstration phase field (2010)
Herschel-ATLAS: the dust energy balance in the edge-on spiral galaxy UGC 4754 (2010)
Mid-infrared spectroscopy of infrared-luminous galaxies at z~0.5-3 (2009)
The mid-infrared view of red sequence galaxies in Abell 2218 with AKARI (2009)
The evolution of star formation in quasar host galaxies (2009)
Far-infrared cosmological survey in AKARI Deep FieldSouth: Galaxy Number Counts (2009)
On the nature of the first galaxies selected at 350 μm (2009)
Photometric redshift accuracy in AKARI deep surveys (2009)
AKARI/IRC deep survey in the North Ecliptic Pole region (2008)
Properties of dusty tori in active galactic nuclei - I. The case of SWIRE/SDSS quasars (2008)
Timeline analysis and wavelet multiscale analysis of the AKARI All-Sky Survey at 90 ?m (2008)
The Infrared Astronomical Mission AKARI (2007)
The Far-Infrared Properties of Spatially Resolved AKARI Observations (2007)
The SCUBA Half Degree Extragalactic Survey - IV. Radio-mm-FIR photometric redshifts (2007)
First Constraints on Source Counts at 350 μm (2007)
The Far-Infrared Surveyor (FIS) for AKARI (2007)
AKARI infrared imaging of reflection nebulae IC4954 and IC4955 (2007)
Deep extragalactic surveys around the Ecliptic Poles with AKARI (ASTRO-F) (2006)
Sub-millimetre properties of massive star-forming galaxies at z ~ 2 in SHADES/SXDF (2006)
The SCUBA Half-Degree Extragalactic Survey - I. Survey motivation, design and data processing (2005)
Properties of FIRBACK-ELAIS 175-mum sources in the ELAIS N2 region (2005)
Final analysis of ELAIS 15-mum observations: method, reduction and catalogue (2005)
The local submillimetre luminosity functions and predictions from Spitzer to Herschel (2005)
The European Large Area ISO Survey - VIII. 90-μm final analysis and source counts (2004)
A study of the 15-μm quasars in the ELAIS N1 and N2 fields (2004)
Mid-infrared sources in the ELAIS Deep X-ray Survey (2004)
Sub-millimeter detections of Spitzer Space Telescope galaxy populations (2004)
Dust and Gas Obscuration in ELAIS Deep X-Ray Survey Reddened Quasars (2004)
The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue (2004)
Large-scale structure in the ELAIS S1 Survey (2004)
The nature of the mid-infrared population from optical identifications of the ELAIS-S1 sample (2004)
The environments of hyperluminous infrared galaxies at 0.44 < z < 1.55 (2004)
The K-band Hubble diagram of submillimetre galaxies and hyperluminous galaxies (2003)
Submillimetre observations of the Hubble Deep Field and Flanking Fields (2003)
SWIRE: The SIRTF Wide-Area Infrared Extragalactic Survey (2003)
The ELAIS deep X-ray survey - I. Chandra source catalogue and first results (2003)
Obscured active galactic nuclei from the ELAIS Deep X-ray Survey (2003)
The coincidence and angular clustering of Chandra and SCUBA sources (2003)
Submillimetre observations of hyperluminous infrared galaxies (2002)
The SCUBA 8-mJy survey - I. Submillimetre maps, sources and number counts (2002)
The SCUBA 8-mJy survey - II. Multiwavelength analysis of bright submillimetre sources (2002)
The local star formation rate and radio luminosity density (2002)
The European Large Area ISO Survey - VII. ROSAT observations of ELAIS sources (2002)
The European Large Area ISO Survey - VI. Discovery of a new hyperluminous infrared galaxy (2001)
The extended counterpart of submm source Lockman 850.1 (2001)
HST/WFPC2 imaging of the QDOT ultraluminous infrared galaxy sample (2001)
Deep Optical and Near Infrared Observations in ELAIS Areas (2001)
Starburst activity in a ROSAT narrow emission-line galaxy (2001)
Radio-quiet quasar environments at 0.5 (2001)
The European Large Area ISO Survey — IV. The preliminary 90-μm luminosity function (2001)
The European Large Area ISO Survey — III. 90-μm extragalactic source counts (2000)
The European Large Area ISO Survey — I. Goals, definition and observations (2000)
The European Large Area ISO Survey — II. Mid-infrared extragalactic source counts (2000)
Clustering of galaxies around radio quasars at 0.5≤z≤0.8 (2000)
IRAS F10214+4724: the inner 100 pc (1998)
A spectroscopic study of IRAS F10214 + 4724 (1998)
The radio—optical correlation in steep-spectrum quasars (1998)
Presentation / Conference
Strong gravitational lensing with the SKA (2015)
A multi-wavelength view of galaxy evolution with AKARI (2012)
Far infrared luminosity function of local galaxies in the AKARI Deep Field South (2012)
The AKARI extragalactic Large Area Survey towards the North Ecliptic Pole (2010)
AKARI infrared bright source catalogues (2010)
The dark and dusty side of galaxy evolution (2010)
The first release of the AKARI-FIS bright source catalogue (2009)
A milestone to SPICA extragalactic surveys: The AKARI NEP survey (2009)
SPICA deep cosmological survey: from AKARI to SPICA (2009)
Coming in from the cold: the galactic plane source populations revealed by AKARI (2009)
Release of the AKARI-FIS Bright Source Catalogue β–1 (2009)
AKARI deep extragalactic survey towards the north ecliptic pole: the NEP-deep survey (2009)
The AKARI north ecliptic pole surveys (2008)
The AKARI cosmological surveys: initial results and new capabilities (2008)
A 15 µm selected sample of hHigh-z starbursts and AGNs (2008)
The Local Sub-mm Luminosity Functions (2004)
Genie observations of small scale astrophysical processes in star forming regions and quasars (2003)
First Results from the ELAIS Deep X-ray Survey (2002)