Stimulating public interest in the dark side of the universe
Submitting Institution
University College LondonUnit of Assessment
PhysicsSummary Impact Type
SocietalResearch Subject Area(s)
Physical Sciences: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Summary of the impact
Cosmologists at UCL — based in the Department of Physics and Astronomy
and the Mullard Space
Science Laboratory (MSSL) — conduct research into dark matter and dark
energy through their
involvement in a number of space missions and ground-based projects. This
research has been
shared with the public through a large number of talks, blogs, articles in
the media, and television
and radio programmes, stimulating significant public interest and
discussion. Increased public
understanding and interaction with the work was further achieved through a
competition to improve
mapping of dark matter. The research also influenced the creative practice
of two artists, inspiring
artworks that have been exhibited internationally and viewed by over 1
million people in total.
Underpinning research
Whilst we know the universe is accelerating, the cause of its
acceleration is still unknown - is it
dark energy, or could it be explained by modifying Einstein's theory of
gravity? Another mystery is
the nature of cold dark matter, a type of matter that is thought to
account for a large part of the total
mass of the universe, and the existence of which is inferred from the
gravitational attraction of
galaxies and stars. Cosmologists at UCL have been investigating these and
other problems since
2004, when cosmology was established as a research area within the
university. These
researchers have played leadership roles in the following cutting-edge
cosmology projects:
(i) The Dark Energy Survey (DES) has been UCL cosmology's
`flagship project'. The $40 million
international DES is using a new wide-field camera, constructed in part at
UCL, on the 4-metre
Blanco telescope in Chile. The survey started in September 2013 and will
map 300 million galaxies
over five years. Its aim is to determine the nature of dark energy and
what is causing the universe's
acceleration. Contributions to the research by the UCL team since 2005
included building the
optical corrector for the DES camera [1] and developing novel methods to
derive galaxy distances
from their colours by utilising artificial neural networks. UCL
researchers also conducted studies of
the feasibility of DES to characterise dark energy and dark matter — for
example, that DES
(combined with Planck) might measure neutrino mass for the first time [2].
(ii) Euclid is a European Space Agency (ESA) mission that is
expected to launch in 2020. It will
carry out spectroscopic measurements of tens of millions of galaxies with
the aim of understanding
the nature of dark matter and dark energy. Since 2006, UCL has been
involved in the inception
and creation of all aspects of the weak lensing science for Euclid. UCL
has contributed and led
scientifically on the development of weak lensing and photometric redshift
methodology, on the
creation of novel approaches for the mitigation and assessment of
systematic effects [3], and in the
survey design.
(iii) Planck - ESA's first mission to study the origins of the
universe — surveyed the sky from 2009
to 2013. Contributions to Planck by UCL researchers [4, 5] included (a)
the selection, calibration
and testing of all the cold optical components of the High Frequency
Instrument on board the
Planck satellite; (b) development of innovative algorithms to constrain
fundamental theories for the
origin of structure in the universe; (c) methods to measure the global
geometry and isotropy of the
universe; and (d) methodology for the reconstruction of the mass
distribution of the universe as
traced by lensing of the cosmic microwave background (CMB). Cosmological
research findings
that are related to these UCL contributions include (a) the first
detection by a single experiment of
the deviation from scale-invariance of the primordial power spectrum, as
predicted by the
fundamental theory of the origin of cosmic structure called "inflation";
and (b) the first full sky map
of where all the mass is in our universe.
(iv) The LOFAR array is the most sensitive radio telescope
ever built in the low frequencies. A
major goal of this telescope is to detect directly the Epoch of
Reionisation, which is the time in the
history of our universe when the first objects were born. The signal that
arrives at the telescope
from the Epoch of Reionisation is 10,000 times smaller than the
contamination from our galaxy.
UCL researchers have played a major role [6] since 2010 in building the
techniques that separate
these signals from each other and from the signal from extragalactic
objects; they implemented an
algorithm that performs foreground subtraction and introduced it in
pipeline form so that other
members of the collaboration could use it.
Key UCL researchers: Ofer Lahav (Perren Chair of Astronomy
2004-present), Sarah Bridle
(Reader in Astronomy 2004-2012), Jochen Weller (Lecturer 2005-2009),
Filipe Abdalla (Lecturer in
Astronomy 2005-present), Hiranya Peiris (Reader in Astronomy
2009-present), Tom Kitching
(Lecturer 2012-present), Mark Cropper (Professor of Astrophysics
1988-present), Peter Doel
(Reader in Astronomy 1998-present) and Giorgio Savini (Lecturer
2009-present).
While aspects of the impact clearly focus on UCL contributions, all four
projects are international
projects. They also involve other UK institutions, which share in the
credit for the impact generated.
References to the research
[1] The impact of camera optical alignments on weak lensing measures for
the Dark Energy
Survey, M. Antonic et al. (incl. Bridle, Doel and Lahav), MNRAS,
431, 3291-3300 (2013)
doi:10.1093/mnras/stt408
[2] Forecasting neutrino masses from galaxy clustering in the Dark Energy
Survey combined with
the Planck measurements, O. Lahav, A. Kiakotou, F.B. Abdalla and
C. Blake, MNRAS, 405, 168-
176 (2010) doi:10.1111/j.1365-2966.2010.16472.x
[3] Defining a weak lensing experiment in space, M. Cropper, H. Hoekstra,
T. Kitching, R. Massey,
J. Amiaux, L. Miller, Y. Mellier, J. Rhodes, B. Rowe, S. Pires, C. Saxton
and R. Scaramella,
MNRAS, 431, 3103-3126 (2013) doi:10.1093/mnras/stt384
[6] Foreground removal using FASTICA: a showcase of LOFAR-EoR, E.
Chapman, F.B. Abdalla,
G. Harker, V. Jelić, P. Labropoulos, S. Zaroubi, M.A. Brentjens, A.G. de
Bruyn and L.V.E.
Koopmans, MNRAS, 423, 2518-2532 (2012) doi:10.1111/j.1365-2966.2012.21065.x
References [2], [3] and [4] best indicate the quality of the
underpinning research.
Details of the impact
UCL research into dark matter and dark energy has led to significant
stimulation of public interest
in these topics, achieved through a large number of public talks, online
blogs, articles in the media,
a BBC television programme and a public competition. It has also impacted
upon two artists,
influencing their creative practice and inspiring a number of their
publicly exhibited artworks.
Public events: UCL cosmologists regularly deliver public talks
based on their research. For
example, dark energy work at UCL was the subject of talks by Ofer Lahav at
the Royal Institution in
June 2013 (attended by 300 people) and at Tate Britain (in March 2009),
and a talk by Sarah Bridle
at the British Astronomical Association (in 2008). Lahav also delivered a
public UCL Lunch Hour
Lecture (in November 2010), "Light and Darkness in the Accelerating
Universe", which was
subsequently uploaded to YouTube and had received almost 2,000 views as of
31 July 2013 [A].
Hiranya Peiris delivered a Space talk at Royal Greenwich Observatory in
March 2013 and a talk at
the British Interplanetary Society in July 2012, both of which were on her
Planck research; a UCL
Science Centre lecture to several hundred sixth formers and teachers in
March 2012; and a talk to
MPs and policymakers at the RCUK event "Impacts: people and skills" in
2010.
Peiris was also invited to present results from the Planck mission on the
origin of the universe at
CERN's first TEDx event, TEDxCERN, in May 2013. The event had a live
audience of 600, as well
as viewing parties at 27 international participating institutions that
were attended by a total of 1,000
people, and 10,870 unique viewers who tuned into the webcast. Peiris's
talk was subsequently
posted on YouTube and had been viewed over 2,000 times as of 31 July 2013
[B].
Blogs: UCL cosmology research is regularly discussed in two blogs
set up by members of staff:
MSSL ASTRO, which was initiated by Tom Kitching in March 2013 on behalf of
MSSL's
Astrophysics Group; and Early Universe @UCL, which was set up by Peiris in
May 2013 to
highlight the Planck research. As of 31 July 2013, these blogs had
received respectively around
2,000 views from 21 countries, and over 3,000 unique viewers with over
10,000 page hits.
Media coverage: Cosmology discoveries at UCL are regularly
reported in press releases that
attract a significant amount of attention from the media. For example, to
accompany the first
release of data from Planck, ESA published two press releases in March
2013 that featured work
contributed by UCL researchers on the physics of the early universe,
large-scale anomalies, and
the weak gravitational lensing of the CMB. This work then received
international press coverage in
March 2013, with articles in the New York Times (NYT), the Financial
Times, The Guardian, The
Economist, and on the BBC's website. These articles stimulated much public
interest and
discussion about Planck and the CMB, as evidenced by the many comments
posted online; for
example, 451 and 345 comments followed the BBC [C] and NYT [D] articles
respectively.
In February 2012, The Economist included both a feature article about
UCL's DES work and an
online video interview with Lahav about the research, which proved to be
one of the most popular
articles published that year. The interview sparked considerable in-depth
discussion about dark
energy by viewers, as evidenced by the detailed online comments [E]. The
article also stimulated a
significant amount of public interest in the topic, as described by the
newspaper's Online Science
Editor, who commented in August 2013: "The nature of dark energy remains
one of the most
perplexing mysteries in all of physics. Despite being abstruse and
baffling, however, the topic
sparks great public interest. Our three-page article about dark energy
(which appeared both in our
print edition and online [...]), focusing on the ambitious Dark Energy
Survey and its quest to
understand the phenomenon, has been read a whopping 115,000 times since it
first appeared in
February 2012. That places it among the most popular pieces The Economist
published in the
whole of 2012, not just in its science section. It also secured 1,200
Facebook "likes" and was
tweeted more than 400 times. An accompanying video interview with
Professor Ofer Lahav has so
far been viewed nearly 12,000 times. Astronomy, it seems, has not lost its
ability to amaze and
inspire." [F]
Television and radio: An episode of Dara Ó Briain's Science Club
featured UCL researcher Filipe
Abdalla talking about the LOFAR array and the challenges of pulling
hard-to-detect cosmological
information out of the data. The episode aired on BBC Two on 1 August
2013, with an audience of
1.22 million [G]. DES research at UCL was discussed on the BBC Radio 4
Today programme by
Bridle, Lahav and Peter Doel in October 2011.
Public competition: In October 2012, UCL's Tom Kitching launched a
public online competition
through the company Kaggle, with the brief to develop algorithms to
improve the mapping of dark
matter using gravitational lensing. The competition was underpinned by
UCL's research on weak
lensing for the Euclid space mission. It ran for two months and attracted
the attention of London-
based Winton Capital Management, which contributed $20,000 of prize funds.
The interesting
problem posed by the challenge attracted 3,553 online entries from 353
teams of participants, and
stimulated much discussion among entrants on the competition's forum about
their solutions and
dark matter [H]. The competition also received significant press
attention, including articles in Time
and Wired magazines, and was discussed in many blogs, including those
written by the
competition's winner and runner-up [I, J]. These participants' detailed
posts about the competition
and their solutions show that taking part increased their interest in and
understanding of the topic.
Winton benefited from its involvement in the competition, using it to
advertise its brand to the exact
demographic in which it was interested in finding future employees; for
example, it led to the
company recruiting a new Senior Data Scientist in 2013. Winton's
Recruitment Manager said:
"Kaggle was a hugely successful venture for Winton. We expend huge amounts
of money and time
on identifying and trying to hire exceptional research scientists for our
business. We only manage
to hire 10-15 per year, though we interview several a week, and through
the Kaggle competition we
sourced two outstanding researchers, one a professor of statistics from
Portugal, the other a
postdoc physicist from California with a PhD from Harvard. The competition
was great branding
and even better it allowed us to help generate new physics research!" [K]
The collaboration
between UCL, Kaggle and Winton is continuing, with a new competition using
Sloan Digital Sky
Survey imaged galaxies soon to be launched.
Creative practice of artists: UCL research has influenced the
creative practice of two artists, both
of whom spent time in the Department of Physics and Astronomy as
Artists-in-Residence and have
created new art inspired by cosmology research carried out at UCL.
The first Artist-in-Residence worked within the department from 2010 to
2011. UCL research on
dark matter, dark energy and DES inspired her to create a new body of
artworks: 100 Billion Suns,
As the World Turns, and History of Darkness. These works have been
exhibited all over the world,
in seven solo exhibitions and 21 group shows, including at Selfridges in
London, the Museum of
Contemporary Art in Sydney, Kettle's Yard in Cambridge, the Modern Art
Museum of Fort Worth,
The Art Institute of Chicago, Kunsthalle Wien, and Ingleby Gallery in
Edinburgh. In total, the
artworks have been viewed by over 1 million people. They also generated
significant press
coverage for the artist, including articles in Wired magazine, The Sunday
Times Culture, Art
Monthly, Observer New Review, AnOther Magazine, The Guardian and The
Independent. She
commented of her experience: "My time spent as Artist-in-Residence in the
Department of Physics
and Astronomy has been invaluable to my research and artistic output.
[...] The ideas I
experienced in the department have inspired several more new works and
will continue to do so for
years to come." [L]
This artist has appeared in two films talking to Lahav about cosmology
research at UCL. "All the
Dead Stars" was made by Tate Britain in 2009 and "When Art Meets
Astronomy" was made by
UCL in 2011; as of 31 July 2013, these films had been viewed on YouTube by
around 8,000
people [M] and around 6,000 people [N] respectively. Lahav also delivered
talks at Tate Britain (in
2009) and the Whitstable Biennale (in 2010) on the connection between the
department's research
and the artist's work; these two talks were attended by a total of around
100 members of the
public.
The second artist began her residency in 2011 and completed an artwork in
February 2013 called
"untitled — the dark energy survey". This artwork was directly inspired by
the DES optical corrector
constructed at UCL and took almost two years to produce. It is now on
display at the University of
London Observatory at Mill Hill, where it will be viewed by hundreds of
visitors every year.
Sources to corroborate the impact
[A] UCL Lunch Hour Lecture on YouTube: http://bit.ly/1g5IDs3
- corroborates the number of views.
[B] TEDxCERN talk on YouTube: http://bit.ly/1foWOHv
- corroborates the number of views.
[C] BBC online article about Planck: http://www.bbc.co.uk/news/science-environment-21866464
-
the comments corroborate that public interest and discussion were
stimulated.
[D] New York Times online article about Planck: http://nyti.ms/1gw7Sl3
- the comments
corroborate that public interest and discussion were stimulated.
[E] The Economist video interview with Lahav: http://econ.st/19EoMqu
- the comments following
the video corroborate the stimulation of public discussion about dark
energy.
[F] Supporting statement from Online Science Editor at The Economist —
corroborates that the
DES article and interview stimulated public interest in dark energy.
Available on request.
[G] Supporting statement from a Series Producer at the BBC — corroborates
the number of viewers
in the audience for the episode of Dara Ó Briain's Science Club. Available
on request.
[H] Public competition website: http://www.kaggle.com/c/DarkWorlds
- corroborates the number of
entries, and that significant discussion amongst participants was
stimulated (on the forum page).
[I] Blog post by public competition winner: http://timsalimans.com/observing-dark-worlds/
-
corroborates that understanding of, and interest in, science were
increased.
[J] Blog post by public competition runner-up:
http://homepages.inf.ed.ac.uk/imurray2/pub/12kaggle_dark/
- corroborates that understanding of,
and interest in, science were increased.
[K] Supporting statement from Recruitment Manager at Winton Capital —
corroborates the benefit
of the public competition to Winton Capital, especially on their
recruitment. Available on request.
[L] Supporting statement from Artist-in-Residence - corroborates the
details of the exhibitions and
that the UCL research had an impact on her work. Available on request.
[M] Tate Britain video on YouTube: http://bit.ly/1c8vZUf
- corroborates the number of views.
[N] UCL "When Art Meets Astronomy" video on YouTube: http://bit.ly/1edv0Th
- corroborates the
number of views.