Research Fellow in Neutron Stars Astrophysics

TN United Kingdom; Dorking; On-site; GBP 40,000 - 80,000; Full time

Job summary

An established industry player is seeking a Research Fellow in Neutron Stars Astrophysics. This exciting role involves advancing theoretical research in compact object astrophysics, focusing on neutron stars atmospheric modeling and X-ray spectro-polarimetry. The successful candidate will lead the development of advanced radiative transfer codes and contribute to significant research projects. With excellent benefits, including generous holiday allowances and a defined benefit pension scheme, this position offers a unique opportunity to make impactful contributions in a collaborative and innovative environment.

Benefits

41 days holiday

Defined benefit pension scheme

Cycle to work scheme

Season ticket loan

Enhanced maternity pay

Enhanced paternity pay

Enhanced adoption pay

Employee assistance program

Discounted medical insurance

Qualifications

• Strong programming skills in high-level languages for astrophysics research.
• Solid background in numerical analysis and algorithm development.

Responsibilities

• Lead the development of radiative transfer codes for neutron star modeling.
• Conduct research on atmospheric emission from magnetized neutron stars.

Skills

Fortran F90-95

C

C++

Python

JAX

Numerical Analysis

Astrophysical Radiative Transfer

Education

PhD in Astronomy

PhD in Physics

PhD in Astrophysics

Tools

Linux

Unix

Job description

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Research Fellow in Neutron Stars Astrophysics, Dorking

Client:

Location:

Dorking, United Kingdom

Job Category:

Other

EU work permit required:

Yes

Job Reference:

63aaab84d385

Job Views:

3

Posted:

08.05.2025

Expiry Date:

22.06.2025

Job Description:

About the role

The Department of Space and Climate Physics at University College London (UCL) seeks to appoint a motivated Research Fellow within the Astrophysics Group. This position is part of our plan to expand MSSL-UCL’s theoretical research in compact object astrophysics, focusing on neutron stars atmospheric modelling and X-ray spectro-polarimetry. The successful applicant will pursue a vigorous research programme and lead the development of advanced radiative transfer codes to model the spectral, timing, and polarimetric properties of atmospheric emission from strongly magnetized neutron stars.

About you

The successful candidate must possess:

• Excellent knowledge of a high-level programming language (e.g., Fortran F90-95, C, C++, Python, JAX) in a Linux/Unix environment
• A solid background in numerical analysis with the ability to translate physical concepts into efficient numerical algorithms
• Expertise in neutron star X-ray emission and astrophysical radiative transfer

Applicants should have (or be close to completing) a PhD in astronomy, physics, or astrophysics.

Candidates are required to submit: 1) an application form, 2) a research statement (max. 3 pages), 3) a CV with three references (max. 2 pages), and 4) a list of publications. The research statement should summarize your main expertise and achievements, and explain how you meet the project criteria.

For informal inquiries, contact Prof. Silvia Zane.

Additional information can be found in the attached job description.

What we offer

We provide an exciting role with excellent benefits, including:

• 41 days holiday (27 days annual leave, 8 bank holidays, 6 closure days)
• Defined benefit pension scheme (CARE)
• Cycle to work scheme and season ticket loan
• Enhanced maternity, paternity, and adoption pay
• Employee assistance program: Staff Support Service
• Discounted medical insurance