Finding the First Supermassive Black Holes with Euclid and WFIRST
Lead Research Organisation:
University of Portsmouth
Department Name: Institute of Cosmology and Gravitation
Abstract
More than 50 quasars have now been discovered at z > 6, or less than a billion
years after the Big Bang. Their existence poses severe challenges to current
theories of cosmological structure formation because it is not known how black
holes above a billion solar masses formed by such early times. We will use state
of the art supercomputer simulations to model the births and evolution of the first
quasars in the universe that include how x-rays from the black holes reionized
the early universe. Our models will produce synthetic observables such as near
infrared (NIR) continuum and Lyman-alpha luminosities for supermassive black
holes down through cosmic time and predict the properties of quasars yet to be
found at z > 6.
years after the Big Bang. Their existence poses severe challenges to current
theories of cosmological structure formation because it is not known how black
holes above a billion solar masses formed by such early times. We will use state
of the art supercomputer simulations to model the births and evolution of the first
quasars in the universe that include how x-rays from the black holes reionized
the early universe. Our models will produce synthetic observables such as near
infrared (NIR) continuum and Lyman-alpha luminosities for supermassive black
holes down through cosmic time and predict the properties of quasars yet to be
found at z > 6.
Planned Impact
Schools: ICG is a member of the South East Physics Network (SEPNet; www.sepnet.ac.uk) which
coordinates a regional outreach programme led by a central outreach director to support the
development and dissemination of good practice and the assessment of impact. Since 2011, SEPnet
outreach has delivered activities to over 100k people. Since 2012, the ICG has employed a SEPnet /
Ogden Outreach Officer (Jennifer Gupta) who has developed our own professionally-run schools
programme. This includes our popular "A Visit from Space" (engaging 609 KS2 children since Oct
2013), our own Astrodome facility (targeted at secondary schools), and our "Cosmology
Masterclass", which supports A-level Physics (e.g. 107 students attended in 2013-14, 60%
commenting that the event changed their view on studying STEM at university). On top of this,
ICG members engaged with 2729 school pupils in 2013-14 through individual talks, workshops and
other events and hosted several work experience students. With all these activities, I am committed
to encouraging wider participation in science and higher education. We work with our University
Education, Liaison and Outreach Team to ensure our activities are advertised to target widening
participation schools, of which there are many in the Portsmouth area.
Public Engagement: All ICG members are encouraged to communicate the results of their science to
help inspire the public. Our main engagement is through talks and presentations e.g. in 2014, ICG
members delivered 37 public activities (e.g. Bestival, Winchester Science Festival). We also host
annual public lectures by prominent external cosmologists (Bernard Shutz in 2014) which always sell
out to capacity. ICG staff and students help deliver major annual "BBC Stargazing Live" local events
with thousands of ticketed visitors. Finally, we engage with the public through traditional and online
media. In the last year, staff have featured in a variety of print articles (Economist, Nature, Astronomy),
appeared on the BBC Horizon (March 2015) and "Sky at Night" (June 2014), and worked to obtain
excellent exposure in the local media (print, radio and TV).
coordinates a regional outreach programme led by a central outreach director to support the
development and dissemination of good practice and the assessment of impact. Since 2011, SEPnet
outreach has delivered activities to over 100k people. Since 2012, the ICG has employed a SEPnet /
Ogden Outreach Officer (Jennifer Gupta) who has developed our own professionally-run schools
programme. This includes our popular "A Visit from Space" (engaging 609 KS2 children since Oct
2013), our own Astrodome facility (targeted at secondary schools), and our "Cosmology
Masterclass", which supports A-level Physics (e.g. 107 students attended in 2013-14, 60%
commenting that the event changed their view on studying STEM at university). On top of this,
ICG members engaged with 2729 school pupils in 2013-14 through individual talks, workshops and
other events and hosted several work experience students. With all these activities, I am committed
to encouraging wider participation in science and higher education. We work with our University
Education, Liaison and Outreach Team to ensure our activities are advertised to target widening
participation schools, of which there are many in the Portsmouth area.
Public Engagement: All ICG members are encouraged to communicate the results of their science to
help inspire the public. Our main engagement is through talks and presentations e.g. in 2014, ICG
members delivered 37 public activities (e.g. Bestival, Winchester Science Festival). We also host
annual public lectures by prominent external cosmologists (Bernard Shutz in 2014) which always sell
out to capacity. ICG staff and students help deliver major annual "BBC Stargazing Live" local events
with thousands of ticketed visitors. Finally, we engage with the public through traditional and online
media. In the last year, staff have featured in a variety of print articles (Economist, Nature, Astronomy),
appeared on the BBC Horizon (March 2015) and "Sky at Night" (June 2014), and worked to obtain
excellent exposure in the local media (print, radio and TV).
Organisations
People |
ORCID iD |
Daniel Whalen (Principal Investigator) |
Publications
Chen K
(2017)
Magnetar-powered Supernovae in Two Dimensions. II. Broad-line Supernovae Ic
in The Astrophysical Journal
Chen K
(2017)
How the First Stars Regulated Star Formation. II. Enrichment by Nearby Supernovae
in The Astrophysical Journal
Chen K
(2017)
Low-energy Population III supernovae and the origin of extremely metal-poor stars
in Monthly Notices of the Royal Astronomical Society
Haemmerlé L
(2018)
The evolution of supermassive Population III stars
in Monthly Notices of the Royal Astronomical Society
Haemmerlé L
(2018)
On the Rotation of Supermassive Stars
in The Astrophysical Journal
Herrington N
(2022)
Modeling Supermassive Primordial Stars with MESA
Herrington N
(2023)
Modelling supermassive primordial stars with mesa
in Monthly Notices of the Royal Astronomical Society
Patrick S
(2023)
The collapse of atomically cooled primordial haloes - I. High Lyman-Werner backgrounds
in Monthly Notices of the Royal Astronomical Society
Rydberg C
(2020)
Detecting strongly lensed supernovae at z ~ 5-7 with LSST
in Monthly Notices of the Royal Astronomical Society
Description | Our research has shown that Euclid will be able to detect the first quasars out to redshifts z ~ 13. Once identified by Euclid, they can then be studied spectroscopically by the James Webb Space Telescope (JWST) or extremely large telescopes (ELTs; 30m - 40m mirrors) on the ground. Consequently, synergies between Euclid and JWST will inaugurate the era of z ~ 5 - 15 quasar astronomy in the coming decade. |
Exploitation Route | We need to study larger samples of primordial quasars with numerical simulations to better predict the properties of early populations of them. This can be straightforwardly done with tools my group has developed with STFC funding. |
Sectors | Other |