Quasars, the luminous beacons of the Universe, are powered by accretion onto supermassive black holes. These enigmatic objects provide critical insights into galaxy evolution, black hole formation, and the early Universe. With advancements in wide-field, highly multiplexed spectroscopic surveys, we now stand at the threshold of a new era in quasar research.
This PhD project will leverage cutting-edge datasets from the 4MOST spectrograph on the ESO VISTA telescope and the MOONS spectrograph on the Very Large Telescope (VLT). These surveys, commencing observations in 2025, significantly extend the reach of traditional optical datasets such as those from the Sloan Digital Sky Survey (SDSS). By probing deeper and extending into the near-infrared spectrum, 4MOST and MOONS are uniquely equipped to uncover more distant and obscured quasars.
As a PhD researcher, you will address key questions:
How abundant are distant and obscured quasars in the Universe?
How do their properties compare to the well-studied optically selected populations from SDSS?
What role do these quasars play in the broader context of galaxy formation and evolution?
The project is observationally driven and will use proprietary data from these surveys to explore the physical characteristics of high-redshift and obscured quasars. You will also contribute to the vibrant research community at Southampton, working alongside leading experts in multi-wavelength galaxy surveys and spectroscopy.
Key Responsibilities
As a PhD candidate, you will:
Analyze spectroscopic data from 4MOST and MOONS to study the properties of high-redshift and obscured quasars.
Compare findings with existing datasets, including SDSS, to identify differences in quasar demographics and physical properties.
Contribute to the scientific output of the 4MOST and MOONS Guaranteed Time Observation (GTO) consortia.
Collaborate with international scientists in the UK, Europe, the USA, and Chile.
Present research findings at national and international conferences.
Publish results in high-impact peer-reviewed journals.
Develop advanced skills in spectroscopy, observational astrophysics, and data analysis.
Entry Requirements
A strong undergraduate degree (equivalent to a UK 2:1 honours degree or higher) in Physics, Astronomy, or a related discipline.
A keen interest in observational astronomy and galaxy formation.
Strong analytical and problem-solving skills.
What We Offer
Funding Opportunities:
Competitive funding packages, including bursaries and scholarships for UK, EU, and international students.
Tuition fees may be covered depending on funding availability and eligibility.
Research Environment:
Access to proprietary data from world-leading spectroscopic surveys, including 4MOST and MOONS.
Opportunities to collaborate with international research teams and institutions.
Training in advanced techniques, including multi-wavelength spectroscopy and data analysis.
A vibrant research community with ongoing projects in galaxy formation and astrophysics.
Professional Development:
Support for attending conferences and workshops to present your findings.
Networking opportunities with global experts in the field.
How to Apply
Applications will be reviewed on a rolling basis, and funding will be allocated to suitable candidates as applications are received. Apply early to maximize your chances of being considered.
Application Process:
Online Application: Submit your application through the University of Southampton’s online portal.
Select "PhD Physics (Full time)" under the program type.
Supervisor Name: Insert “Manda Banerji” in Section 2 of the application form.
Required Documents:
Curriculum Vitae (CV).
Two reference letters.
Degree transcripts and certificates.
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