UCL Astrophysics Consolidated Grant 2015-2018
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
We now know that not only is our Universe expanding, but that it is expanding at an ever-increasing rate. Fuelled by a mysterious driver
called Dark Energy, galaxies, such as our Milky Way, are rushing away from each other at such enormous acceleration that not even the powerful
force of gravity can hold the universe together.
Researchers in UCL's Astrophysics Group are putting to the test these discoveries with an ambitious programme of research for the coming years.
A map of 300 million galaxies that astronomers will put together using the Dark Energy Survey over the next decade will be combined with a new chart of the Cosmic Microwave Background from the Planck satellite to understand the conditions in the early universe, to detect the tiny mass of the Neutrino particle and to test Einstein's theory of general Relativity on the largest scales. Our astronomers will use the LOFAR radio telescope to study the era long ago when the first stars and galaxies formed and sculpted ionized bubbles within the gas that permeated the Universe.
We will probe how stars form from vast gas and dust clouds and how the chemistry that goes on between the stars affects and controls these
crucial processes, by studying molecules and dust in our own Galaxy, in nearby galaxies, and in distant, very young, galaxies located at the edge
of the Universe.
We will study the lives of massive stars and their deaths in giant explosions called supernovae and how these massive stars enrich the Galaxy
with the gas and dust required to make new stars, new planets and even life itself.
None of this can be done unless astronomers continually improve the instruments with which they carry out their studies of the heavens. UCL's
instrument makers are aiming to create lower cost optics for future infrared telescopes in space and to develop sophisticated new techniques
that can be used to deliver incredibly high angular resolutions on space telescopes observing at infrared wavelengths.
Astronomers need to model the universe that they study with ever more complex mathematical techniques. So UCL's computer experts will generate the sophisticated models, running on supercomputers, that are needed to understand the wealth of observations that are pouring in. They will also generate the basic atomic and molecular data with which to simulate the conditions in the early Universe, in evolving galaxies and in the stars and planetary systems that inhabit the galaxies. These new data will be used in particular to interpret and understand observations of the atmospheres of exoplanets as they pass in front of, and behind, the stars that they orbit.
But all of this will be wasted unless our fellow citizens get to share in the wonder and excitement of our group's work. So we will ensure that our
team members continue to explain their work through talks and lectures, through public events, and through the media, inspiring the next
generation of scientists, helping and challenging industry to develop new technologies, and ensuring that our understanding of the Universe becomes ever deeper and wider.
called Dark Energy, galaxies, such as our Milky Way, are rushing away from each other at such enormous acceleration that not even the powerful
force of gravity can hold the universe together.
Researchers in UCL's Astrophysics Group are putting to the test these discoveries with an ambitious programme of research for the coming years.
A map of 300 million galaxies that astronomers will put together using the Dark Energy Survey over the next decade will be combined with a new chart of the Cosmic Microwave Background from the Planck satellite to understand the conditions in the early universe, to detect the tiny mass of the Neutrino particle and to test Einstein's theory of general Relativity on the largest scales. Our astronomers will use the LOFAR radio telescope to study the era long ago when the first stars and galaxies formed and sculpted ionized bubbles within the gas that permeated the Universe.
We will probe how stars form from vast gas and dust clouds and how the chemistry that goes on between the stars affects and controls these
crucial processes, by studying molecules and dust in our own Galaxy, in nearby galaxies, and in distant, very young, galaxies located at the edge
of the Universe.
We will study the lives of massive stars and their deaths in giant explosions called supernovae and how these massive stars enrich the Galaxy
with the gas and dust required to make new stars, new planets and even life itself.
None of this can be done unless astronomers continually improve the instruments with which they carry out their studies of the heavens. UCL's
instrument makers are aiming to create lower cost optics for future infrared telescopes in space and to develop sophisticated new techniques
that can be used to deliver incredibly high angular resolutions on space telescopes observing at infrared wavelengths.
Astronomers need to model the universe that they study with ever more complex mathematical techniques. So UCL's computer experts will generate the sophisticated models, running on supercomputers, that are needed to understand the wealth of observations that are pouring in. They will also generate the basic atomic and molecular data with which to simulate the conditions in the early Universe, in evolving galaxies and in the stars and planetary systems that inhabit the galaxies. These new data will be used in particular to interpret and understand observations of the atmospheres of exoplanets as they pass in front of, and behind, the stars that they orbit.
But all of this will be wasted unless our fellow citizens get to share in the wonder and excitement of our group's work. So we will ensure that our
team members continue to explain their work through talks and lectures, through public events, and through the media, inspiring the next
generation of scientists, helping and challenging industry to develop new technologies, and ensuring that our understanding of the Universe becomes ever deeper and wider.
Planned Impact
Our Group will continue and develop its current Knowledge Exchange and Outreach programmes, which are described in detail in our 2-page Pathways to Impact document.
For Knowledge Exchange, we will have the professional support of UCL Business (for IP support) and UCL Enterprise (for entrepreneurship training, mentorship and access to venture capital). The transfer of the results of our innovation is being achieved as follows:
(i) By providing accurate and complete molecular data to Industry and to researchers in other fields - this has proved particularly successful with our water and methane line lists, which are extensively used by industry and by modellers of Earth's atmosphere and climate. Current and future applications include the design of high temperature gas sensors; modelling non-thermal rotational distributions of H3+ in storage rings; measuring the refractive index of humid air in the IR; high speed thermometry and tomographic imaging in gas engines; and of course atmospheric models.
(ii) By working through OSL's three main technology transfer firms, Zeeko, OPTICS Glyndyr, through which research level optical design and manufacturing processes are transferred to Industry. They work closely with Industry to establish the link between detailed surface topography and functional performance in order to improve performance or reduce cost, or both. Examples include the semiconductor sector (polishing of large-area display components; the transition to photolithography in the EUV), the defence sector (advanced weapons and surveillance sites; imaging systems for UAVs, head-up displays),
light-weight optics for remote sensing, the high-power laser community (including laser-fusion) and the automobile sector (use of head-up displays in cars).
(iii) By working with commerce, research design labs and other academic areas to produce new technologies, e.g. by enagaging with the new Satellite Applications Catapult on the compact LOw Cost Upper atmosphere Sounder
(LOCUS), which promises to transform the economics of Earth observation missions and provide a cost effective method of monitoring long term trends in the climate.
(iv) By continuing to work with leading IT vendors to test and design new hardware and software solutions which will eventually end up in the marketplace. We are playing a leading role in setting up an Industrial Engagement Database that will connect DiRAC researchers with STFC Innovation and TSB funding calls, TSB Catapult Centre facilitated industrial projects,
and Industry-HEI/RC projects.
Our Outreach Programme will continue to build on its current strong foundations. These include www.ucl.ac.uk/youruniverse/ and www.ucl.ac.uk/star/outreach/themindofuniverse. We have a Work Experience Programme for 16-18-yr-olds and a programme of school visits that provides popular talks on a wide range of topics. Our ULO teaching observatory at Mill
Hill has a regular programme of public open evenings, as well as daytime schools visits, bringing several thousand visitors annually, with a tie-in with the BBC's Stargazing Live. We will continue to draw upon the professional support of the UCL Public Engagement Unit, www.ucl.ac.uk/public-engagement, both in terms of training and access to award-winning events such as 'Science Show-Off' and 'Bright Club'.
We have attracted extensive international media coverage for the discovery at our ULO Observatory of a bright supernova in the nearby M82 galaxy, the closest Type Ia supernova in over 40 years, and for press releases linked to Science and Nature papers on supernova dust and molecules, and on young galaxies at the edge of the Universe, as well as for ESA press releases on Planck results featuring UCL researchers. We will continue our prominent programme of media appearances, talks and podcasts. In engaging with the press, we will continue to have strong support from the MAPS and UCL Communications and Media Relations units.
For Knowledge Exchange, we will have the professional support of UCL Business (for IP support) and UCL Enterprise (for entrepreneurship training, mentorship and access to venture capital). The transfer of the results of our innovation is being achieved as follows:
(i) By providing accurate and complete molecular data to Industry and to researchers in other fields - this has proved particularly successful with our water and methane line lists, which are extensively used by industry and by modellers of Earth's atmosphere and climate. Current and future applications include the design of high temperature gas sensors; modelling non-thermal rotational distributions of H3+ in storage rings; measuring the refractive index of humid air in the IR; high speed thermometry and tomographic imaging in gas engines; and of course atmospheric models.
(ii) By working through OSL's three main technology transfer firms, Zeeko, OPTICS Glyndyr, through which research level optical design and manufacturing processes are transferred to Industry. They work closely with Industry to establish the link between detailed surface topography and functional performance in order to improve performance or reduce cost, or both. Examples include the semiconductor sector (polishing of large-area display components; the transition to photolithography in the EUV), the defence sector (advanced weapons and surveillance sites; imaging systems for UAVs, head-up displays),
light-weight optics for remote sensing, the high-power laser community (including laser-fusion) and the automobile sector (use of head-up displays in cars).
(iii) By working with commerce, research design labs and other academic areas to produce new technologies, e.g. by enagaging with the new Satellite Applications Catapult on the compact LOw Cost Upper atmosphere Sounder
(LOCUS), which promises to transform the economics of Earth observation missions and provide a cost effective method of monitoring long term trends in the climate.
(iv) By continuing to work with leading IT vendors to test and design new hardware and software solutions which will eventually end up in the marketplace. We are playing a leading role in setting up an Industrial Engagement Database that will connect DiRAC researchers with STFC Innovation and TSB funding calls, TSB Catapult Centre facilitated industrial projects,
and Industry-HEI/RC projects.
Our Outreach Programme will continue to build on its current strong foundations. These include www.ucl.ac.uk/youruniverse/ and www.ucl.ac.uk/star/outreach/themindofuniverse. We have a Work Experience Programme for 16-18-yr-olds and a programme of school visits that provides popular talks on a wide range of topics. Our ULO teaching observatory at Mill
Hill has a regular programme of public open evenings, as well as daytime schools visits, bringing several thousand visitors annually, with a tie-in with the BBC's Stargazing Live. We will continue to draw upon the professional support of the UCL Public Engagement Unit, www.ucl.ac.uk/public-engagement, both in terms of training and access to award-winning events such as 'Science Show-Off' and 'Bright Club'.
We have attracted extensive international media coverage for the discovery at our ULO Observatory of a bright supernova in the nearby M82 galaxy, the closest Type Ia supernova in over 40 years, and for press releases linked to Science and Nature papers on supernova dust and molecules, and on young galaxies at the edge of the Universe, as well as for ESA press releases on Planck results featuring UCL researchers. We will continue our prominent programme of media appearances, talks and podcasts. In engaging with the press, we will continue to have strong support from the MAPS and UCL Communications and Media Relations units.
Organisations
Publications
Crocce M
(2015)
Galaxy clustering, photometric redshifts and diagnosis of systematics in the DES Science Verification data
in Monthly Notices of the Royal Astronomical Society
Yachmenev A
(2015)
Automatic differentiation method for numerical construction of the rotational-vibrational Hamiltonian as a power series in the curvilinear internal coordinates using the Eckart frame.
in The Journal of chemical physics
Aalto S
(2015)
Probing highly obscured, self-absorbed galaxy nuclei with vibrationally excited HCN
in Astronomy & Astrophysics
Vedantham H
(2015)
Lunar occultation of the diffuse radio sky: LOFAR measurements between 35 and 80 MHz
in Monthly Notices of the Royal Astronomical Society
Bisbas T
(2015)
EFFECTIVE DESTRUCTION OF CO BY COSMIC RAYS: IMPLICATIONS FOR TRACING H 2 GAS IN THE UNIVERSE
in The Astrophysical Journal
Fenech Danielle Marie
(2015)
Peering into the heart of the M82 starburst: Type II supernova remnants and a possible relic GRB?
in IAU General Assembly
Codella C
(2015)
Astrochemistry at work in the L1157-B1 shock: acetaldehyde formation
in Monthly Notices of the Royal Astronomical Society: Letters
Wade G
(2015)
The MiMeS survey of magnetism in massive stars: introduction and overview
in Monthly Notices of the Royal Astronomical Society
Saro A
(2015)
Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters
in Monthly Notices of the Royal Astronomical Society
Morford Jack
(2015)
e-MERLIN Radio Continuum Measurements of OB Star Winds in Cyg OB2
in IAU General Assembly
Matsuura M
(2015)
A STUBBORNLY LARGE MASS OF COLD DUST IN THE EJECTA OF SUPERNOVA 1987A
in The Astrophysical Journal
Evans M
(2015)
Gravitational instabilities in a protosolar-like disc - I. Dynamics and chemistry
in Monthly Notices of the Royal Astronomical Society
M Tessenyi
(2015)
Twinkle -A British space mission to explore faraway worlds
in Proceedings of the International Astronautical Congress, IAC
Clark S.
(2015)
An Astrophysical Laboratory: Understanding and Exploiting the Young Massive Cluster Westerlund 1
in The Messenger
Goldstein D
(2015)
ERRATUM: "AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY" (2015, AJ, 150, 82)
in The Astronomical Journal
Dunstall P
(2015)
The VLT-FLAMES Tarantula Survey XXII. Multiplicity properties of the B-type stars???
in Astronomy & Astrophysics
Ciesla L
(2015)
The imprint of rapid star formation quenching on the spectral energy distributions of galaxies
in Astronomy & Astrophysics
Pattle K
(2015)
The JCMT Gould Belt Survey: first results from the SCUBA-2 observations of the Ophiuchus molecular cloud and a virial analysis of its prestellar core population
in Monthly Notices of the Royal Astronomical Society
Sandqvist A
(2015)
Herschel HIFI observations of the Sgr A +50 km s -1 Cloud Deep searches for O 2 in emission and foreground absorption
in Astronomy & Astrophysics
Morello G
(2015)
REVISITING SPITZER TRANSIT OBSERVATIONS WITH INDEPENDENT COMPONENT ANALYSIS: NEW RESULTS FOR THE GJ 436 SYSTEM
in The Astrophysical Journal
Matsuura M.
(2015)
ALMA Observations of Supernova 1987A
in Revolution in Astronomy with ALMA: The Third Year
Bevan A
(2015)
Modelling supernova line profile asymmetries to determine ejecta dust masses: SN 1987A from days 714 to 3604
in Monthly Notices of the Royal Astronomical Society
Martins F.
(2015)
VizieR Online Data Catalog: Spectra of 12 ON stars (Martins+, 2015)
in VizieR Online Data Catalog
Sousa-Silva C
(2015)
ExoMol line lists - VII. The rotation-vibration spectrum of phosphine up to 1500 K
in Monthly Notices of the Royal Astronomical Society
Walborn N
(2015)
SPECTRAL VARIATIONS OF Of?p OBLIQUE MAGNETIC ROTATOR CANDIDATES IN THE MAGELLANIC CLOUDS
in The Astronomical Journal
Owens A
(2015)
A global potential energy surface and dipole moment surface for silane.
in The Journal of chemical physics
Soumagnac M
(2015)
Star/galaxy separation at faint magnitudes: application to a simulated Dark Energy Survey
in Monthly Notices of the Royal Astronomical Society
Gruen D
(2015)
Weak lensing by galaxy troughs in DES Science Verification data
in Monthly Notices of the Royal Astronomical Society
Morello Giuseppe
(2015)
A new data analysis technique for Spitzer transit observations
in IAU General Assembly
Chang C
(2015)
Wide-Field Lensing Mass Maps from Dark Energy Survey Science Verification Data.
in Physical review letters
Kirk D
(2015)
Optimizing spectroscopic and photometric galaxy surveys: same-sky benefits for dark energy and modified gravity
in Monthly Notices of the Royal Astronomical Society
Al-Refaie A
(2015)
ExoMol line lists - VIII. A variationally computed line list for hot formaldehyde
in Monthly Notices of the Royal Astronomical Society
Evans C. J.
(2015)
VizieR Online Data Catalog: VFTS. B-type stars classification and RV (Evans+, 2015)
in VizieR Online Data Catalog
Fenech Danielle Marie
(2015)
Non-Thermal Emission from the massive stellar association Cygnus OB2
in IAU General Assembly
Wright G
(2015)
The Mid-Infrared Instrument for the James Webb Space Telescope , II: Design and Build
in Publications of the Astronomical Society of the Pacific
Canty J
(2015)
Methane and ammonia in the near-infrared spectra of late-T dwarfs
in Monthly Notices of the Royal Astronomical Society
Martins F
(2015)
Surface abundances of ON stars
in Astronomy & Astrophysics
Reeve D. C.
(2015)
VizieR Online Data Catalog: Limb-darkening coefficients (Reeve+, 2016)
in VizieR Online Data Catalog
Owens A
(2015)
Accurate prediction of H 3 O + and D 3 O + sensitivity coefficients to probe a variable proton-to-electron mass ratio
in Monthly Notices of the Royal Astronomical Society
Salji C
(2015)
The JCMT Gould Belt Survey: constraints on prestellar core properties in Orion A North
in Monthly Notices of the Royal Astronomical Society
Majumdar S
(2015)
Effects of the sources of reionization on 21-cm redshift-space distortions
in Monthly Notices of the Royal Astronomical Society
Azzam A
(2015)
The dipole moment surface for hydrogen sulfide H2S
in Journal of Quantitative Spectroscopy and Radiative Transfer
Flaugher B
(2015)
THE DARK ENERGY CAMERA
in The Astronomical Journal
Burke DJ
(2015)
Trapping and desorption of complex organic molecules in water at 20 K.
in The Journal of chemical physics
Kessler R
(2015)
THE DIFFERENCE IMAGING PIPELINE FOR THE TRANSIENT SEARCH IN THE DARK ENERGY SURVEY
in The Astronomical Journal
Rauw G
(2015)
X-RAY EMISSION FROM MASSIVE STARS IN CYG OB2
in The Astrophysical Journal Supplement Series
Chang C
(2015)
MODELING THE TRANSFER FUNCTION FOR THE DARK ENERGY SURVEY
in The Astrophysical Journal
Justtanont K.
(2015)
H
2O Isotopologues in Extreme OH/IR Stars
in Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time
Owens A
(2015)
Accurate prediction of the ammonia probes of a variable proton-to-electron mass ratio
in Monthly Notices of the Royal Astronomical Society
Oikonomou F
(2015)
Simulations for a next-generation UHECR observatory
in Journal of Cosmology and Astroparticle Physics
Description | Since its inception in April 2015, this grant had produced 850 publications as of March 3rd 2020. The papers cover a large range of science, given that this is a Consolidated Grant having seven different funded projects. The Dark Energy Survey has completed a significant fraction of its survey and has produced a large number of papers which are reflected in the total output of papers for this grant. Large numbers of papers on Herschel and Planck results continue to be published by us, as well as papers on stellar, circumstellar and supernova physics, on astrochemistry and star formation, on molecular data for exoplanet studies, and on astronomical instrumentation studies. |
Exploitation Route | The results will and have been used to influence the future research carried out by ourselves and other astrophysicists. |
Sectors | Aerospace, Defence and Marine,Digital/Communication/Information Technologies (including Software),Education,Culture, Heritage, Museums and Collections |
URL | https://www.darkenergysurvey.org/news-and-results/press-releases/ |
Description | The Group conducts activities intending to reach out to the public and private sectors and we have collaborations that are leading to technological, scientific or commercial developments, e.g. Tennyson's Exomol programme has established links with Technical University of Denmark and Servomex plc, who use linelist data to model spectra of gas emissions at the top of smokestacks for environmental monitoring. Exomol data also contributes to atmospheric and climate models; Viti has a collaboration with academic chemists to produce experimental and theoretical surface chemistry reaction rates; DES, Planck and Euclid projects are linked to multiple industrial contracts, some of which have UK industrial firms developing processes to meet instrument specifications. We have developed a very active Artists in Residence Programme: http://www.judygoldhill.com/ http://www.janegrisewood.com/ http://andycharalambous.com/ |
First Year Of Impact | 2015 |
Sector | Education,Culture, Heritage, Museums and Collections |
Impact Types | Cultural,Societal |
Description | UCL Centre for Doctoral Training in Data Intensive Science and Technologies |
Amount | £2,645,591 (GBP) |
Funding ID | ST/P006736/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 09/2017 |
End | 09/2024 |
Title | Jovian and Kronian Magnetodisc Field and Guiding Centre Dynamics of Trapped Particles Data |
Description | Data files and basic Matlab visualisation functionality of Jovian and Kronian UCL magnetodisc model output and guiding centre dynamics of trapped particles data described in the JGR Space Physics paper 2020JA027827 Trapped Particle Motion In Magnetodisk Fields by Guio, P. and Staniland, N. and Achilleos, N. A. and Arridge, C. S.(https://doi.org/10.1029/2020JA027827) |
Type Of Material | Database/Collection of data |
Year Produced | 2020 |
Provided To Others? | Yes |
URL | https://zenodo.org/record/3749390 |
Title | Jovian and Kronian Magnetodisc Field and Guiding Centre Dynamics of Trapped Particles Data |
Description | Data files and basic Matlab visualisation functionality of Jovian and Kronian UCL magnetodisc model output and guiding centre dynamics of trapped particles data described in the JGR Space Physics paper 2020JA027827 Trapped Particle Motion In Magnetodisk Fields by Guio, P. and Staniland, N. and Achilleos, N. A. and Arridge, C. S.(https://doi.org/10.1029/2020JA027827) |
Type Of Material | Database/Collection of data |
Year Produced | 2020 |
Provided To Others? | Yes |
URL | https://zenodo.org/record/3749389 |
Title | Duo update |
Description | Duo is a general variational diiatomic molecule nuclear motion program. It has been updated to provide the inner region of an R-matrix treatment of ultra-low energy collisions. |
Type Of Technology | Software |
Year Produced | 2018 |
Open Source License? | Yes |
Impact | Calculations of ultra-low energy collisions: original test on Ar -- Ar |
URL | https://github.com/Trovemaster/Duo |
Title | ExoCross |
Description | A post processor for ExoMol (and HITRAN) data |
Type Of Technology | Software |
Year Produced | 2018 |
Open Source License? | Yes |
Impact | This program is being widely used to post process ExoMol data |
URL | https://github.com/Trovemaster/exocross |
Title | TROVE |
Description | A new version of the code TROVE was developed which explicitly included the symmetry of methane. |
Type Of Technology | Software |
Year Produced | 2013 |
Impact | The production of linelists for methane and silane |
URL | https://github.com/Trovemaster/TROVE |
Description | The DESI First light was reported in October 2019 on BBC TV News at 10, BBC World Service and other media |
Form Of Engagement Activity | A broadcast e.g. TV/radio/film/podcast (other than news/press) |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | The DES First light was reported in October 2019 on BBC TV News at 10, BBC World Service and other media |
Year(s) Of Engagement Activity | 2019 |