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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)

ORCID 0000-0002-0517-7943

Books

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

An Introduction to Galaxies and Cosmology (2nd ed) (2015)

Observational Cosmology (2010)

Book Chapter

Testing the efficiency of infrared spectral features as redshift indicators in AKARI deep surveys (2009)

Tuning in the radio: deep radio surveys supporting the AKARI North and South Ecliptic Pole Ultra Deep Fields (2009)

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)

ELAIS deep X-ray survey. I. (Manners+, 2003) (2004)

ISO ELAIS 15{mu}m survey (Lari+, 2001) (2002)

Digital Artefact

The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE (2010)

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)

ALMA Detection of [O ɪɪɪ] 88 μm at z = 12.33: Exploring the Nature and Evolution of GHZ2 as a Massive Compact Stellar System (2024)

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)

The Radio Galaxy Environment Reference Survey (RAGERS): a submillimetre study of the environments of massive radio-quiet galaxies at z = 1–3 (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 : Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees (2024)

Euclid preparation : XXXVIII. Spectroscopy of active galactic nuclei with NISP (2024)

An Upper Limit to Differential Magnification Effects in Strongly Gravitationally Lensed Galaxies (2024)

Citizen science in European research infrastructures (2024)

An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies (2024)

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 μ m and Data Release for the COSMOS Field (2024)

Citizen science, accessibility, art & science, critical thinking, policy and engagement: thoughts and lessons learned from the REINFORCE experience (2024)

The RAdio Galaxy Environment Reference Survey (RAGERS): Evidence of an anisotropic distribution of submillimeter galaxies in the 4C 23.56 protocluster at z = 2.48 (2024)

A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging (2024)

FLASH: Faint lenses from Associated Selection with Herschel (2024)

Transfer learning for galaxy feature detection: Finding giant star-forming clumps in low-redshift galaxies using Faster Region-based Convolutional Neural Network (2024)

Characterisation of Herschel-selected strong lens candidates through HST and sub-mm/mm observations (2023)

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)

z-GAL: A NOEMA spectroscopic redshift survey of bright Herschel galaxies : II. Dust properties (2023)

Bright extragalactic ALMA redshift survey (BEARS) III: Detailed study of emission lines from 71 Herschel targets (2023)

The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates (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)

Galaxy Zoo: Clump Scout - Design and first application of a two-dimensional aggregation tool for citizen science (2022)

Searching for giant planets in the outer Solar System with far-infrared all-sky surveys (2022)

Multiwavelength properties of 850-μm selected sources from the North Ecliptic Pole SCUBA-2 survey (2022)

The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope (2022)

Massive Molecular Gas Reservoir in a Luminous Submillimeter Galaxy during Cosmic Noon (2022)

A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years (2022)

Modelling high-resolution ALMA observations of strongly lensed dusty star forming galaxies detected by Herschel (2022)

An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Survey Description and First Results (2022)

Detecting gravitational lenses using machine learning: exploring interpretability and sensitivity to rare lensing configurations (2022)

Optically detected galaxy cluster candidates in the AKARI North Ecliptic Pole field based on photometric redshift from the Subaru Hyper Suprime-Cam (2021)

Super-resolving Herschel imaging: a proof of concept using Deep Neural Networks (2021)

The Importance of Citizen Scientists in the Move Towards Sustainable Diets and a Sustainable Food System (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)

How Does Citizen Science Compare to Online Survey Panels? A Comparison of Food Knowledge and Perceptions Between the Zooniverse, Prolific and Qualtrics UK Panels (2021)

Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission (2021)

Engaging citizens in sustainability research: comparing survey recruitment and responses between Facebook, Twitter and qualtrics (2021)

Early science with the Large Millimeter Telescope: a 1.1 mm AzTEC survey of red-Herschel dusty star-forming galaxies (2021)

Chronos: A NIR spectroscopic galaxy survey to probe the most fundamental stages of galaxy evolution (2021)

Identification of AKARI infrared sources by the Deep HSC Optical Survey: construction of a new band-merged catalogue in the North Ecliptic Pole Wide field (2021)

NEPSC2, the North Ecliptic Pole SCUBA-2 survey: 850-μm map and catalogue of 850-μm selected sources over 2 deg2 (2020)

A high redshift population of galaxies at the North Ecliptic Pole (2020)

Piloting Citizen Science Methods to Measure Perceptions of Carbon Footprint and Energy Content of Food (2020)

IRAM 30m-EMIR Redshift Search of z = 3 − 4 Lensed Dusty Starbursts selected from the HerBS sample (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)

Spectroscopic confirmation and modelling of two lensed quadruple quasars in the Dark Energy Survey public footprint (2019)

The strong gravitational lens finding challenge (2019)

What do astronomers want from the STFC? (2019)

AKARI NEP field: Point source catalogs from GALEX and Herschel observations and selection of candidate lensed sub-millimeter galaxies (2019)

Probing the high-redshift universe with SPICA: Toward the epoch of reionisation and beyond (2018)

JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results (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)

Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel (2018)

GravityCam: Wide-field high-resolution high-cadence imaging surveys in the visible from the ground (2018)

AKARI/IRC source catalogues and source counts for the IRAC Dark Field, ELAIS North and the AKARI Deep Field South (2017)

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)

The SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120° to 140° (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)

AKARI all-sky bright source catalogue: far-infrared luminous quasars and the optical far-infrared correlation (2017)

Witnessing the birth of the red sequence: ALMA high-resolution imaging of [CII] and dust in two interacting ultra-red starbursts at z = 4.425 (2016)

The JCMT nearby galaxies legacy survey – X. Environmental effects on the molecular gas and star formation properties of spiral galaxies (2016)

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)

H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry (2015)

Evolution of mid-infrared galaxy luminosity functions from the entire AKARI NEP deep field with new CFHT photometry (2015)

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)

Polycyclic aromatic hydrocarbon feature deficit of starburst galaxies in the AKARI North Ecliptic Pole Deep field (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)

Detection of Hα emission from z > 3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy (2013)

The preferentially magnified active nucleus in IRAS F10214+4724 - I. Lens model and spatially resolved radio emission (2013)

H2O emission in high-z ultra-luminous infrared galaxies (2013)

The local luminosity function of star-forming galaxies derived from the Planck Early Release Compact Source Catalogue (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)

Star formation and AGN activity in galaxies classified using the 1.6μm Bump and PAH features at z = 0.4-2 (2012)

The JCMT Nearby Galaxies Legacy Survey - VIII. CO data and the LCO(3-2)-LFIR correlation in the SINGS sample (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)

Measurements of CO redshifts with Z-Spec for lensed submillimeter galaxies discovered in the H-ATLAS survey (2012)

The AKARI NEP-Deep survey: a mid-infrared source catalogue (2012)

Planck early results. XIII. Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue (2011)

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)

Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters (2011)

Herschel-ATLAS: The link between accretion luminosity and star formation in quasar host galaxies (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)

Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS (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)

Herschel-ATLAS galaxy counts and high-redshift luminosity functions: the formation of massive early-type galaxies (2011)

The JCMT Nearby Galaxies Legacy Survey – V. The CO(J= 3–2) distribution and molecular outflow in NGC 4631 (2011)

The JCMT Nearby Galaxies Legacy Survey - IV. Velocity dispersions in the molecular interstellar medium in spiral galaxies (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: dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours (2010)

Herschel-ATLAS: evolution of the 250 µm luminosity function out to z=0.5 (2010)

Herschel-ATLAS: the angular correlation function of submillimetre galaxies at high and low redshift (2010)

A search for debris disks in the Herschel-ATLAS (2010)

Ultra deep AKARI observations of Abell 2218: resolving the 15 μm extragalactic background light (2010)

Polycyclic aromatic hydrocarbon (PAH) luminous galaxies at z ~ 1 (2010)

Evolution of infrared luminosity functions of galaxies in the AKARI NEP-deep field: revealing the cosmic star formation history hidden by dust (2010)

Environmental dependence of 8 μm luminosity functions of galaxies atz~ 0.8: comparison between RXJ1716.4+6708 and the AKARI NEP-deep field (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)

The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light (2010)

Luminosity functions of local infrared galaxies with AKARI: implications for the cosmic star formation history and AGN evolution (2010)

Green Bank Telescope Zpectrometer CO(1-0) observations of the strongly lensed submillimeter galaxies from the Herschel ATLAS (2010)

AzTEC half square degree survey of the SHADES fields – I. Maps, catalogues and source counts (2010)

The JCMT Nearby Galaxies Legacy Survey - III. Comparisons of cold dust, polycyclic aromatic hydrocarbons, molecular gas and atomic gas in NGC 2403 (2010)

H-ATLAS: PACS imaging for the Science Demonstration Phase (2010)

The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey. II. Warm molecular gas and star formation in three field spiral galaxies (2010)

The Herschel ATLAS (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 space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA (2009)

The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey. I. Star-forming molecular gas in Virgo Cluster spiral galaxies (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)

The SCUBA Half-Degree Extragalactic Survey (SHADES) - VII. Optical/IR photometry and stellar masses of submillimetre galaxies (2008)

The SCUBA Half Degree Extragalactic Survey (SHADES) – IX. The environment, mass and redshift dependence of star formation (2008)

The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveys (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 SCUBA HAlf Degree Extragalactic Survey (SHADES) - V Submillimetre properties of near-infrared-selected galaxies in the Subaru/XMM -Newton deep field (2007)

The Infrared Astronomical Mission AKARI (2007)

The Far-Infrared Properties of Spatially Resolved AKARI Observations (2007)

Far-Infrared Distributions in Nearby Spiral Galaxies NGC 2841 and NGC 2976 Observed with AKARI/Far-Infrared Surveyor (FIS) (2007)

Properties of UIR Bands in NGC6946 Based on Mid-Infrared Imaging and Spectroscopy with Infrared Camera on Board AKARI (2007)

Optical Identification of 15 micron Sources in the AKARI Performance Verification Field toward the North Ecliptic Pole (2007)

Multi-Wavelength Analysis of 18 micron -Selected Galaxies in the AKARI/Infrared-Camera monitor field towards the North Ecliptic Pole (2007)

The SCUBA HAlf Degree Extragalactic Survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies (2007)

The SCUBA Half Degree Extragalactic Survey - IV. Radio-mm-FIR photometric redshifts (2007)

First Constraints on Source Counts at 350 μm (2007)

The ultraluminous and hyperluminous infrared galaxies in the Sloan Digital Sky Survey, 2dF Galaxy Redshift Survey and 6dF Galaxy Survey (2007)

The Far-Infrared Surveyor (FIS) for AKARI (2007)

Optical identification of 15 μm sources in the AKARI performance verification field toward the north ecliptic pole (2007)

AKARI infrared imaging of reflection nebulae IC4954 and IC4955 (2007)

The SCUBA Half-Degree Extragalactic Survey - II. Submillimetre maps, catalogue and number counts (2006)

Deep extragalactic surveys around the Ecliptic Poles with AKARI (ASTRO-F) (2006)

A combined re-analysis of existing blank-field SCUBA surveys: comparative 850-mum source lists, combined number counts, and evidence for strong clustering of the bright submillimetre galaxy population on arcminute scales (2006)

Sub-millimetre properties of massive star-forming galaxies at z ~ 2 in SHADES/SXDF (2006)

A robust sample of submillimetre galaxies: constraints on the prevalence of dusty, high-redshift starbursts (2005)

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)

The European Large Area ISO Survey: optical identifications of 15-mum and 1.4-GHz sources in N1 and N2 (2005)

Final analysis of ELAIS 15-mum observations: method, reduction and catalogue (2005)

Spectral energy distributions and luminosities of galaxies and active galactic nuclei in the Spitzer Wide-Area Infrared Extragalactic (SWIRE) legacy survey (2005)

Sloan digital sky survey quasars in the Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) ELAIS N1 Field: properties and spectral energy distributions (2005)

The local submillimetre luminosity functions and predictions from Spitzer to Herschel (2005)

The European Large Area ISO Survey - IX. The 90-mum luminosity function from the Final Analysis sample (2004)

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)

First isights into the Spitzer Wide-area Infrared Extragalactic Legacy Survey (SWIRE) galaxy populations (2004)

Sub-millimeter detections of Spitzer Space Telescope galaxy populations (2004)

Spitzer Observations of the SCUBA/VLA Sources in the Lockman Hole: Star Formation History of Infrared-Luminous Galaxies (2004)

Spitzer observations of MAMBO Galaxies: weeding out active nuclei in starbursting protoellipticals (2004)

The Mid-Infrared Luminosity Function of Galaxies in the European Large Area Infrared Space Observatory Survey Southern Fields (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)

Discovery of the galaxy counterpart of HDF 850.1, the brightest submillimetre source in the Hubble Deep Field (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)

Near- and mid-infrared colours of star-forming galaxies in European Large Area ISO Survey fields (2002)

Deep radio imaging of the SCUBA 8-mJy survey fields: submillimetre source identifications and redshift distribution (2002)

Submillimetre observations of hyperluminous infrared galaxies (2002)

A new method for ISOCAM data reduction - II. Mid-infrared extragalactic source counts in the ELAIS Southern field (2002)

Observations of the Hubble Deep Field South with the Infrared Space Observatory - I. Observations, data reduction and mid-infrared source counts (2002)

Observations of the Hubble Deep Field South with the Infrared Space Observatory - II. Associations and star formation rates (2002)

The evolution of type 1 active galactic nuclei in the infrared (15mum): the view from ELAIS-S1 (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)

A new method for ISOCAM data reduction - I. Application to the European Large Area ISO Survey Southern Field: method and results (2001)

Deep Optical and Near Infrared Observations in ELAIS Areas (2001)

Starburst activity in a ROSAT narrow emission-line galaxy (2001)

The European Large-Area Infrared Space Observatory Survey V: A BeppoSAX Hard X-Ray Survey of the S1 Region (2001)

Radio-quiet quasar environments at 0.5 (2001)

The European Large Area ISO Survey — IV. The preliminary 90-μm luminosity function (2001)

The Nature of the Faint Radio Source Population and Star Formation History derived from Sub-MJY Surveys (2001)

The European Large Area ISO Survey — III. 90-μm extragalactic source counts (2000)

Starburst galaxies and structure in the submillimetre background towards the Hubble Deep Field (2000)

Hubble Space Telescope imaging survey of sub-mJy star-forming galaxies — I. Morphologies at z ∼ 0.2 (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)

High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey (1998)

The radio—optical correlation in steep-spectrum quasars (1998)

Observations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometry (1997)

Observations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysis (1997)

Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies (1997)

Observations of the Hubble Deep Field with the Infrared Space Observatory - V. Spectral energy distributions, starburst models and star formation history (1997)

Observations of the Hubble Deep Field with the Infrared Space Observatory - I. Data reduction, maps and sky coverage (1997)

Hidden quasars reddened by dust? (1996)

The redshift cutoff in steep spectrum radioquasars (1996)

Presentation / Conference

Identifying muon rings in VERITAS data using convolutional neural networks trained on images classified with Muon Hunters 2 (2021)

Synergies between SALT and Herschel, Euclid & the SKA: strong gravitational lensing & galaxy evolution (2015)

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)

Extremely Red mid-infrared selected objects in the AKARI NEP deep field: dust obscured type-1 AGN? (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)

The ELAIS deep X-ray survey (2001)

QSO environments at intermediate redshifts (2001)

Report

A new HST/Herschel deep field at the North Ecliptic Pole: preparing the way for JWST, SPICA and Euclid (2012)