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| Postdoctoral Position at the Astronomical Institute of the Czech Academy of Sciences | Closing date: 2020-02-24
Contact: Vladimir Karas |
| We are Public Research Institution and the largest professional astronomical organization in the Czech Republic, located at Ondrejov observatory and in Prague. Successful applicants will collaborate with researchers in our scientific departments (theory, observation, and data analysis are all welcome). Recently the Institute has been involved in space programs of ESA and ground-based projects within ESO, including the European ALMA. Experience in one of the subjects studied at the Institute is valued but independent new projects will be also considered. | | ▸ more | The appointment is initially for one year; an extension for another year is expected upon satisfactory scientific performance. A necessary condition is to satisfy legal requirements for the employment in Czech Republic (EU member state). Salary will be based on the domestic level and it includes health insurance. There is a possibility of institute accommodation in Ondrejov; in Prague private accommodation has to be arranged.
In a cover letter please indicate the working group that you intend to join. Applicants should contact a faculty member with whom they wish to work for further information, to define a joint research programme, and to discuss the starting date. This is considered to be an important part of the proposal.
Applications (containing Curriculum Vitae, List of Publications, and Summary of Research Plans) can be submitted by email to:
sekretariat @ asu.cas.cz (subject: "postdoc 2020", pdf file please).
Please provide the exact date of PhD defense. Applications can be submitted before finishing PhD, in which case a statement from the supervisor stating the planned date of the defense should be included. Successful candidates must hold PhD degree in the field and present a certificate of that by 29th April. Preferences will be given to early-stage researchers.
Please arrange for two recommendation letters to be sent directly (the same electronic address as above).
To receive full consideration, this year application deadline is: 24th February 2020 (the anticipated starting date is in July). Applications will be acknowledged by email and a confirmation will be requested from eligible applicants. Once the selection process is completed, successful applicants will be notified.
Further information:
o See http://www.asu.cas.cz for the list of working groups at the Institute.
o See http://www.euraxess.cz for details about the research employment and work conditions in Czech Republic.
o See http://www.numbeo.com/cost-of-living/comparison.jsp to compare cost of living.
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| Chief Finance Officer | Closing date: 2020-01-26
Contact: Human Resources |
This is an ideal role for a talented and influential finance leader who can work at operational and strategic level to deliver excellence and change in a complex international environment.
To apply online for this role, please visit our recruitment portal: https://recruitment.skatelescope.org/vacancy/chief-finance-officer-406818.html | | ▸ more | The Square Kilometre Array (SKA) is a global project to build a multi-purpose radio telescope that will play a major role in answering key questions in modern astrophysics and cosmology. Thirteen countries are now participating in the project, with others engaged in discussions regarding possible membership. Facilities for the new telescope will be located in South Africa and Australia, with our headquarters in a purpose-built building at Jodrell Bank, Cheshire, UK. SKA HQ currently houses around 90 staff but has just undergone a major expansion to accommodate up to 150 staff as the project moves towards construction and operation of the SKA telescopes.
Negotiations between the governments of SKA member countries to establish the SKA Observatory as an Inter-Governmental Organisation (IGO) have recently concluded; the IGO is expected to be established in late 2020.
The Role
This is a new high-profile leadership position in what will grow to be one of the world?s largest research infrastructure projects; the successful candidate will lead the Finance department at a strategic level, as well as overseeing the application of the company?s Finance Policies and Procedures. The post holder will report to the Director-General and be supported initially by a small team of 3 staff at SKA Headquarters.
The establishment of this role presents a unique opportunity to be involved at a critical time, as the company transitions to an IGO, and the global project moves from the conclusion of its design activities to construction. The postholder will require the vision and drive to plan and then establish the necessary future financial and commercial requirements of the SKA Observatory as it enters operation, while acting as the financial leader for the delivery of a multi-million Euro cutting-edge research infrastructure.
In line with the evolution of organisation, the successful candidate should be a high-potential individual with the capability in the future to take on a broader commercial leadership role as required.
Key Responsibilities, Accountabilities and Duties
- Work closely with key stakeholder groups to develop a finance operating model and new financial procedures and processes for the future IGO;
- Provide high-level financial advice and guidance to the Director General, senior managers, the Board and its relevant sub-committees;
- Develop and maintain strong working relationships with external parties including project partners, Intergovernmental Organisations, advisors, contractors and suppliers;
- Ensure effective cross-functional working by the Finance team, and in particular with HR and Procurement, to contribute to the development of financial planning across the company;
- Lead and manage budget management and business continuity planning for finance, including risk analysis, mitigation and recovery;
- Ensure that company financial systems are robust, compliant with best practice, and support current activities and future growth;
- Ensure that relevant regulatory requirements are met;
- Manage and develop the Finance Department and its functions, including financial accounting, management accounting, cash flow and treasury management, compliance and control, audit, payroll and pensions;
- Oversee the the implementation and on-going development of the new ERP system;
- Provide visible leadership to staff, setting clear direction, developing and motivating staff through change;
- Travel both inside and outside of the UK as necessarily required by the position. It is anticipated that the need for travel will be infrequent; and
- Undertake any other reasonable duties as directed by the Director-General.
Mandatory Knowledge, Skills and Experience
- University degree or equivalent in finance, accounting, business administration or a related area;
- Qualified member of an internationally recognised professional finance-related body or equivalent;
- Proven track record of working in an international context with internal and external stakeholders, building effective working relationships at all levels with people from a broad range of national and cultural backgrounds;
- An influential communicator with commercial acumen and a track record of operating effectively at a strategic board level or equivalent;
- A highly motivated strategic leader with an analytical and enquiring mind, able to identify and deliver effective changes to meet organisational needs now and in the future;
- A technical expert with an in-depth knowledge of financial management and accounting principles, laws, strong 'hands on' financial analysis, budgeting, forecasting and reporting skills and working knowledge of financial controls and risk management;
- Knowledge of foreign currency transactions and associated risks;
- Strong IT skills and open to new technologies;
- Able to work effectively at operational level to develop a small team to deliver excellent operational services, whilst also operating effectively at strategic level;
- A leader with high integrity and openness combined with commitment to good governance, equality and diversity and sustainability; and
- A flexible team player who collaborates effectively with other functions and is adaptable to change.
Desirable Knowledge, Skills and Experience
- Experience of interacting with public bodies such as universities, research organisations, local and national government departments, etc;
- Experience of research grant funding;
- Experience of managing, and accounting for, in-kind contributions;
- Experience with procurement in an international setting;
- Experience of managing subsidiaries from a finance perspective;
- Experience of facilities contract management;
- Proficient in the use or development of ERP systems, ideally Unit4 Business World
- Experience working with distributed staff located in remote location
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| IT Operations Specialist (Linux) | Closing date: 2020-01-19
Contact: Human Resources |
An ideal role for a Linux and Cloud specialist who is keen to support a ground-breaking international project.
Click here to apply online via our recruitment portal: https://recruitment.skatelescope.org/vacancy/it-operations-specialist-linux-406864.html | | ▸ more | The Square Kilometre Array (SKA) is a global project to build a multi-purpose radio telescope that will play a major role in answering key questions in modern astrophysics and cosmology. Thirteen countries are now participating in the project, with others engaged in discussions regarding possible membership. Facilities for the new telescope will be located in South Africa and Australia, with our headquarters in a purpose-built building at Jodrell Bank, Cheshire, UK. SKA HQ currently houses around 90 staff but has just undergone a major expansion to accommodate up to 150 staff as the project moves towards construction and operation of the SKA telescopes.
Negotiations between the governments of SKA member countries to establish the SKA Observatory as an Inter-Governmental Organisation (IGO) have recently concluded; the IGO is expected to be established in late 2020.
An ideal role for a Linux and Cloud specialist who is keen to support a ground-breaking international project.
The Role
The purpose of this role is to implement, maintain and improve server and service operations within SKAO Site(s) and in Cloud platforms. The role holder will Interface with all staff and provide expertise to stakeholders as required, supporting the development of services from the programme, especially in the realms of Linux-based systems and native cloud developments.
The role reports to the Head of Information Technology and is part of a small multi-disciplinary team of technical specialists based at the Head Office. The team ensure that an international team including Astronomers, Project Managers, Engineers and Software Developers who are building the largest radio telescope in the world have the technological tools and services they need to ensure effective communication and collaboration.
Key Responsibilities, Accountabilities and Duties
- Operation of Linux-based physical and virtual servers including their implementation/installation, maintenance and optimisation
- Operation and management of server-based and serverless services in Public Cloud infrastructure such as but not exclusively Amazon Web Services and Google Cloud
- Securing and patching Linux-based and related technologies to appropriate levels
- Operating, implementing and maintaining web-hosting services based on Linux technologies
- Operating, implementing and maintaining Cloud and local database services
- Achieving high availability (and continuity) of services through appropriate use of duplication, replication, disaster recovery and backup and restore technology and services
- Provision and securing of remote access to systems and applications
- Supporting the installation, maintenance and optimisation of, often open source, applications on servers and Cloud platforms and as Software as a Service
- Continual development of event management/monitoring and automation to improve service and reduce manual overheads
- Perform installation and upgrading of scientific software packages including astronomical data reduction tools
- Work as part of the team to support of the wider Information & Communications Technology (ICT) services including incident, request & problem ticket management, device builds and support of the communications and presentation technologies in the HQ
- Would also be required to undertake any other duties within the individual's capabilities as may be reasonably required.
Key Outcomes
- Robust and reliable services running optimally with minimal downtime
- Excellent ICT service with positive reviews from internal and external service users
- Continual Service Improvement (CSI) of services
- Value for money in procurement, automation, on-time project delivery and identified savings
- Effective and proven business continuity and disaster recovery capabilities
Mandatory Knowledge, Skills and Experience
- Relevant university degree-level education or equivalent experience
- Considerable experience (typically at least 4-5 years) with Linux-based systems and software including:
1) compilation and installation of software, especially open source
2) backup and restore, securing and patch management
- Experience of maintaining Private and Public Cloud services
- Knowledge and experience with ?as a Service? technologies including Platform, Database, Software and serverless/container Cloud offerings
- Programming/scripting experience and capability across multiple platforms
- Knowledge of configuration management methods and tools
- Able to plan work and problem solve, individually and as part of a team, to optimise service and meet deadlines in a dynamic and collaborative environment
- Able to communicate effectively both orally and in writing with an international team that spans a wide range of sectors (commercial and academic), cultures and backgrounds.
- Flexible team player who is adaptable to change and demonstrates a commitment to high-quality service provision
- Willing and able to work, on occasion outside of normal business hours, including evenings and weekends to meet the needs of an international organisation.
Desirable Knowledge, Skills and Experience
- Knowledge and background with IT Service Management disciplines and Frameworks such as ITIL and Change Management
- Experience of specific software provisioning, configuration management, and application-deployment tools.
- Experience of scientific computing
- Knowledge and experience in Microsoft-based technologies supplementing the team capability
- Knowledge of enterprise networks (local area, wireless, wide area)
- Experience with Apple and Google device and mobile device technologies and device management systems
- General interest in Astronomy and related sciences and technologies
- Certification held in industry/community - recognised disciplines/technologies pertinent to the role
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| Software Quality Engineer (UK based role) | Closing date: 2020-01-19
Contact: Human Resources |
An ideal role for a talented software quality team leader who is interested in working on a ground breaking international project.
Click here to apply online via our recruitment portal: https://recruitment.skatelescope.org/vacancy/software-quality-engineer-405613.html | | ▸ more | The Square Kilometre Array (SKA) is a global project to build a multi-purpose radio telescope that will play a major role in answering key questions in modern astrophysics and cosmology. Thirteen countries are now participating in the project, with others engaged in discussions regarding possible membership. Facilities for the new telescope will be located in South Africa and Australia, with our headquarters in a purpose-built building at Jodrell Bank, Cheshire, UK. SKA HQ currently houses around 90 staff but has just undergone a major expansion to accommodate up to 150 staff as the project moves towards construction and operation of the SKA telescopes.
Negotiations between the governments of SKA member countries to establish the SKA Observatory as an Inter-Governmental Organisation (IGO) have recently concluded; the IGO is expected to be established in late 2020.
An ideal role for a talented software quality team leader who is interested in working on a ground breaking international project.
The Role
The SKA software is being designed and developed by a number of teams that are located world-wide. In order to ensure software is developed, tested, and integrated coherently and smoothly, the SKA Organisation must clearly define our expectations with a well-defined set of processes and tools.. This activity will be supported by a small team at the SKA Organisation, acting as part of the SAFe System Team, developing and maintaining the Continuous Integration and Delivery platform used by agile development teams.
Key Responsibilities, Accountabilities and Duties
The main functions of this role will be to:
- Lead the SKA SAFe® System Team in the implementation and maintenance of the Continuous Delivery pipeline infrastructure. (Source code repository, workflow manager, issue tracker, CI system, documentation system, automated testing infrastructure etc.)
- Work with the SKA Software teams to define and implement the Continuous Delivery pipeline for the SKA software system.
- Work with the SKA SAFe® System Team to support agile development teams in adopting DevOps practices.
- Maintain and update the SKA Software Engineering Process documentation.
- Work with other staff in the SKA Office to develop processes to support software quality during procurement and construction, in accordance with DevOps practices.
- Support system-wide integration and verification.
Mandatory Knowledge, Skills and Experience
The successful applicant for this role will bring:
- Experience in the development and support of large software systems.
- Experience in leading a technical team providing vision and technical leadership.
- Experience in modern processes for efficiently developing high quality software ? for example DevOps, continuous integration, agile processes, test driven development etc.
- Demonstrated understanding and enthusiasm for working based on lean/agile principles.
- Ability to communicate effectively, both orally and in writing, to an audience that spans a wide range of cultures and backgrounds.
- A flexible team player who is adaptable to change.
- Able & willing to travel overseas occasionally.
Desirable Knowledge, Skills and Experience
The ideal candidate would also be:
- Experience in developing Python and C/C++ software in a GNU/Linux environment.
- Familiar with methods and algorithms used in Radio Astronomy Interferometry.
- Familiar with the formalism for, and requirements of, quality control environments such as ISO9000.
Equal Opportunities Statement
Equality, Diversity and Inclusion are at the core the SKA's agenda and we are committed to being an equal opportunities employer. Our aim to is recruit and retain the most talented individuals, regardless of gender, race, disability, age, sexual orientation, marital status, religion or nationality.
Women have traditionally been under-represented in the fields of science and engineering; SKA Organisation welcomes and encourages female applicants.
Where applicants with a disability need facilities or adjustments to enable them to participate in the recruitment process, these will be provided.
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| Postdoctoral Fellowship in Gravitational Astrophysics | Closing date: 2020-01-31
Contact: Martin Pessah |
| The Niels Bohr International Academy at The Niels Bohr Institute invites applications for 3-year Postdoctoral positions in the area of transient electro-magnetic and gravitational wave astrophysics. Exceptional and highly motivated candidates will also be considered for 5-year positions at the Assistant Professor level. Applicants are requested to submit their applications via the via the online application system before January 15, 2020 for full consideration. | | ▸ more | The Niels Bohr International Academy at The Niels Bohr Institute invites applications for 3-year Postdoctoral positions in the area of transient electro-magnetic (EM) and gravitational wave (GW) astrophysics. Exceptional and highly motivated candidates will also be considered for 5-year positions at the Assistant Professor level. The preferred starting date is Fall 2020. Applicants are requested to submit their applications via the online application system (including a cover letter, CV, publication list, a research statement, and three letters of recommendation). For full consideration, applications should be received by January 15, 2020. Applications will be reviewed continually up until January 31, 2020.
The successful candidate will have a unique opportunity to conduct research in collaboration with a vibrant group of scientists covering a broad range of topics relevant for EM+GW astrophysics, including newly appointed Assistant Prof. Johan Samsing (GW astrophysics, N-body dynamics, black hole merger synthesis modeling); Associate Prof. Irene Tamborra (particle astrophysics, multi-messenger astrophysics, neutrinos in and from neutron star mergers, supernovae, etc.); and Prof. Martin Pessah (astrophysical fluid dynamics, magnetohydrodynamics, black hole accretion discs).
We are especially looking for candidates interested in the modeling of gravitational wave sources, their expected EM and GW signals, and how current and future observatories (LIGO/Virgo, LISA, DECIGO, CE/ET) can be used to probe their astrophysical origin. Topics of particular interest include:
- (1) Relativistic N-body/hydro simulations of stellar systems hosting black holes.
- (2) Interaction of black holes near intermediate mass- and super-massive black holes.
- (3) Dynamics and merger of compact objects in active galactic nuclei discs.
- (4) Modeling of Milky Way GW sources and how they relate to LIGO/Virgo observations.
Applications from outstanding candidates with relevant expertise in complementary aspects of transient EM+GW astrophysics are warmly welcome.
The successful candidate will also have exclusive access to some of the largest dedicated astrophysics computer resources in Scandinavia, including a general-purpose cluster with more than 3000 cores, a GPU cluster, a petabyte of storage, and dedicated data analysis servers. The successful candidate will also have the opportunity to guide more junior fellows, teach courses at various levels, participate in outreach activities, and organize international meetings. The position also includes a generous research and travel budget.
For further information, questions and informal inquiries please email Asst. Prof. Johan Samsing (jsamsing @ gmail.com) or Prof. Martin Pessah (mpessah @ nbi.dk). Note that interested candidates who have already submitted applications in response to the add: https://jobregister.aas.org/ad/4c33fc64 are already under consideration and should therefore not re-submit their applications.
The Niels Bohr International Academy strives to attract the best and the brightest by providing the environment to enable curiosity-driven breakthrough research in the physical sciences and mathematics. The Academy hosts numerous workshops, symposia and PhD-schools every year, as well as a number of outreach activities, including an annual series of public lectures. The University of Copenhagen wishes to reflect the diversity of society and welcomes applications from all qualified candidates regardless of personal background.
Postdoctoral Fellows at the University of Copenhagen receive a competitive salary (including pension) and funds for travel and computing. Generous parental leave, state-subsidized childcare, vacation, and full medical care are provided to employees in Denmark. A favorable tax scheme is generally granted to international researchers.
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| 6-year Research Position in Dynamics of Planetary Systems | Closing date: 2020-02-10
Contact: Alexandre Correia |
| The Physics Department of the University of Coimbra, Portugal, invites applications for a research position in Dynamics of Planetary Systems under the CEEC FCT program. Applicants can be researchers of all nationalities, who have the potential to develop innovative research and have a relevant scientific CV in Astrophysics. | | ▸ more | Description:
The successful applicant is expected to do research in one of the following topics: solar system dynamics, TNOs, planet formation and evolution, dynamics of multi-planetary systems. Computational experience is required and a background in celestial mechanics is a plus. Applications by researchers working on other research topics related to the field of solar system or exoplanets will also be evaluated.
Qualifications: PhD in Astrophysics or similar already concluded.
Application deadline: 10th February 2020
Host institution: CFisUC, Department of Physics, University of Coimbra, PORTUGAL (EU).
Type of contract: 6 year Contract:
Salary: from 30.000 to 60.000 EUR / year (depending on experience).
Benefits include social security and 25 vacation days.
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APPLICATION PROCEDURE:
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Job Reference: CEEC-FCT-Planets
Language: English
Candidates should contact Prof. Alexandre Correia (acor @ uc.pt) before February 10th 2020, with the following documents:
1. CV (including publication list)
2. A brief research plan (maximum 3 pages)
3. Name and contact of 2 scientists who can provide a letter of recommendation.
4. The application should include a motivation letter mentioning: expectations of applicant, short summary of current research interests, and relevance of research profile of candidate for the hosting institution.
The pre-selected candidate will get the support from the University of Coimbra to apply to the CEEC program.
Contacts and further information:
Alexandre Correia:
http://sweet.ua.pt/correia
University of Coimbra:
http://www.fis.uc.pt/bx/
FCT Program:
https://www.fct.pt/apoios/contratacaodoutorados/empregocientifico/ceec_ind_3.phtml.en
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| Three double-degree PhD fellowships in exoplanet research at the Niels Bohr Institute, University of Copenhagen, Denmark | Closing date: 2020-02-03
Contact: Uffe Gråe Jørgensen, Niels Bohr Institute |
The Niels Bohr Institute is offering three PhD scholarships in the field of exoplanets. The fellowships are part of the EU funded Network CHAMELEON -- virtual laboratories for exoplanets and planet forming disks (http://chameleon.wp.st-andrews.ac.uk/recruitment/), which combines the expertise of eight European research institutes to cover relevant aspects of exoplanetary atmospheres and protoplanetary disk modelling, observation and interpretation.
Starting date: 1st of September 2020 or as soon as possible thereafter. | | ▸ more | Fellowship 1: Irradiation and impact of stellar variability on exoplanet atmospheres
Aim: Development of self-consist models for stellar and irradiated exoplanet atmospheric systems and synthetic spectra. Using these models for studying the effect of stellar variability and activity on the exoplanet?s atmosphere and its potential habitability.
Double degree with University of Leuven, Belgium.
Fellowship 2: Low-temperature chemistry for DRIFT-MARCS.
Aim: Combining the experience from cool star modelling by the MARCS code with surface interaction and low-temperature gas- and cloud chemistry from the DRIFT code. Comparing model computations with existing and coming observations of a wide range of exoplanets.
Double degree with University of St Andrews, Scotland.
Fellowship 3: Connecting the atmosphere and the interior in extrasolar gas planets.
Aim: Connecting the interior of exoplanets with observations of the atmosphere (i.e. spectra, colours etc), and compare results from 1D and 3D computations. Using these models to study inflated close-in planets (i.e. solving the hot jupiter radius anomaly).
Double degree with University of Leuven, Belgium.
Principal supervisor: Professor Uffe Gråe Jørgensen, Niels Bohr Institute, uffegj @ nbi.dk, direct phone: (+45) 61 30 66 40. Secondment supervisors: In St Andrews Dr Christiane Helling, and in Leuven Dr Ludmila Carone and Professor Leen Decin.
The fellowships are part of the EU funded Network CHAMELEON -- virtual laboratories for exoplanets and planet forming disks, which combines the expertise of eight European research institutes (Universities of St Andrews, Groningen, Copenhagen, Edinburgh, Leuven and Antwerp, the Max-Planck Institute in Heidelberg and the Netherlands Institute for Space Research) to cover relevant aspects of exoplanetary atmospheres and protoplanetary disk modelling, observation and interpretation. The network will consist of the 15 PhD students and the respective supervisors and local research groups. Students of all nationalities are welcomed. A detailed description of all the 15 announced PhD fellowships of the network and how to apply is listed at (http://chameleon.wp.st-andrews.ac.uk/recruitment/).
Starting date: 1st of September 2020 or as soon as possible thereafter.
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| 2 PhD positions in the field of evolved stars and ALMA | Closing date: 2020-02-20
Contact: Clio Gielen |
The Institute of Astronomy, KU Leuven, Belgium has 2 open PhD positions in the field of evolved stars, entitled ?ATOMIUM: ALMA Tracing the Origins of Molecules formIng dUst in oxygen-rich M-type stars?.
The aim of the PhD positions is to establish the dominant physical and chemical processes in the winds of oxygen-rich evolved stars over a range of stellar masses, pulsation behaviours, mass-loss rates, and evolutionary phases. One student will focus on the analysis of the lower-mass asymptotic giant branch (AGB) stars, the other one on the more massive red supergiant (RSG) stars. | | ▸ more | The context
Over 200 molecules and 15 dust species have been detected in the interstellar medium, stellar winds, exoplanets, supernovae, active galactic nuclei etc. One of the most fundamental questions in astrophysics deals with the phase transition from simple molecules to larger gas-phase clusters and eventually dust grains. The outflows of evolved stars are the best laboratories to answer this pivotal question due to their rich chemistry and relatively simple dynamical structure. Aiming to establish the dominant physical and chemical processes in the winds of evolved stars, we have requested and were granted an ESO ALMA Large Program, called ATOMIUM ?ALMA Tracing the Origins of Molecules In dUst-forming oxygen-rich M-type stars?. The ATOMIUM project is the first ALMA Large Program which is granted in the field of stellar evolution.
The projects
The aim of the 2 open PhD positions is to establish the dominant physical and chemical processes in the winds of oxygen-rich evolved stars over a range of stellar masses, pulsation behaviours, mass-loss rates, and evolutionary phases. One student will focus on the analysis of the lower-mass asymptotic giant branch (AGB) stars, the other one on the more massive red supergiant (RSG) stars. The students will work in parallel to unravel the phase transition from gas-phase to dust species, pinpoint the chemical pathways, map the morphological structure, and study the interplay between dynamical and chemical phenomena for both types of stars.
The host institute
The Institute of Astronomy of KU Leuven in Belgium is a vibrant research group of some 70 scientists, engineers, and administrative staff (fys.kuleuven.be/ster), including 6 full-time and 3 part-time professors. The institute is an expertise centre in stellar physics and active in several international consortia and collaborations, involving telescopes at observatories worldwide and in space. The IoA is responsible for the organisation of the 2-year Master in Astronomy & Astrophysics at the Faculty of Science and operates the 1.2m Mercator telescope at La Palma Observatory, Canary Islands.
The positions
The selected PhD students will be offered a 2-year contract, once renewable with 2 more years after positive evaluation. The salary will be commensurate to the standard scale for PhD students in Belgium; it includes social and medical insurance as well as pension rights. The foreseen starting date is September-October 2020. The successful PhD applicants will have to register at, and comply with, the regulations of the Arenberg Doctoral School of the KU Leuven. Good command of the English language is a requirement to be approved by the doctoral school. The successful PhD applicants will follow a doctoral programme including personal training in management, science communication, and teaching. As part of the doctoral requirements, the students will have to take up a teaching task of at maximum 4 hours per week in one of the Bachelor (in Dutch) or Master (in English) programmes. PhD students at IoA are also required to perform at least one Mercator observing run of 10 nights per year for the pooled IoA long-term monitoring programmes.
Requirements and Instructions to Apply
PhD applicants must hold a M.Sc. degree in physics/astrophysics/mathematics or equivalent, at the latest one month before the position can be taken up. Proficiency in English is required.
The application package should be sent as one single PDF containing
(i) a curriculum vitae, with a publication list if relevant;
(ii) a statement of interest (max. one page, including a brief description of research interests and relevant experience);
(iii) copies of university grades, certificates and/or diplomas;
(iv) names and contact details of 2 experts who are prepared to send confidential recommendation letters should they be requested to do so.
The application material should be sent by e-mail to Clio.Gielen @ kuleuven.be with subject ?PhD-ATOMIUM-applicantname? latest by February 20th 2020.
Applications that do not strictly follow these guidelines will not be considered.
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| PhD positions at The Australian National University, Canberra, Australia | Closing date: 2020-12-25
Contact: David McClelland |
| PhD position at the ANU Centre for Gravitational Physics in the filed of optics, electro-optics, electronics, control systems, isolation systems and modelling. | | ▸ more | Projects with the Centre for Gravitational Astrophysics will develop skills in a number of highly employable areas such as: optics, electro-optics, electronics, control systems, isolation systems and modelling. We also have research projects which aim to develop spin-off technology into commercial products, for example high sensitivity trace gas analysis, laser intensity and frequency stabilization techniques and more.
More details about some of the available projects can be found at : https://physics.anu.edu.au/quantum/people/profile.php?ID=288&tab=available_projects
For more information
Contact:
Prof. McClelland, David
(02) 612 59888
David.McClelland @ anu.edu.au
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| Senior Lecturer in Astrophysics, Botswana International University of Science and Technology (BIUST) | Closing date: 2020-02-14
Contact: Professor Greg Hillhouse |
| The University wishes to appoint a suitably qualified individual to undertake teaching and research in Astrophysics. BIUST has been designated as the national Host Institution for Botswana?s involvement in the African VLBI Network and ultimately SKA Phase 2 and this post is part of an ambitious expansion of Astrophysics capability at the institution. | | ▸ more | SENIOR LECTURER IN ASTROPHYSICS
Botswana International University of Science and Technology (BIUST)
Faculty of Sciences
Department of Physics and Astronomy
The position will be based at BIUST Campus, Palapye, Botswana
Please note: Processing of received applications will commence from 14th February 2020. *The position will remain vacant until filled*.
MAIN PURPOSE OF THE JOB:
To teach and educate undergraduate and graduate students in Physics and Astronomy and to build the knowledge base in Astrophysics through research and publications. To administer teaching activities within the discipline of Physics and Astrophysics and provide leadership at the module or course level. To establish a national and international research reputation in the field of Astrophysics. To be active in professional service related to Astrophysics.
BIUST has been designated as the national Host Institution for Botswana?s involvement in the African VLBI Network and ultimately SKA Phase 2 and this post is part of an ambitious expansion of Astrophysics capability at the institution.
QUALIFICATIONS AND EXPERIENCE:
A PhD in Physics with a focus on Astrophysics
A minimum of two (2) years? experience (after obtaining PhD degree) in teaching and research at university level. However two years of relevant industrial/professional experience shall be equivalent to one year of teaching experience.
At least 8 publications in reputable refereed journals
Research or technology development related to Radio Astronomy will be considered an added advantage
REMUNERATION:
The University offers an attractive package commensurate with qualifications and experience.
The position is offered on a fixed-term contract of five (5) years/ pensionable terms
If you meet the requirements of the above stated position please send your application letter and detailed Curriculum Vitae including at least three (3) recent professional references to:
Director, Human Resources at recruitment.phyastronomy @ biust.ac.bw
Note that only shortlisted candidates will be responded to.
For an informal discussion, please contact Professor Greg Hillhouse, Head of Physics and Astronomy, by emailing hillhouseg @ biust.ac.bw
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| Postdoctoral positions in Astrophysics and Cosmology | Closing date: 2020-02-01
Contact: Uri Keshet and Yuri Lyubarski |
| The Astrophysics and Cosmology team in Ben-Gurion University (BGU) invites applications for two postdoctoral fellowships. | | ▸ more | Research fields include high-energy astrophysics, plasma astrophysics, and cosmology. The work, with Professors Yuri Lyubarski and Uri Keshet, will include analytic, computational, or phenomenological aspects, depending on the applicant: relevant experience is necessary.
Each fellowship is for a period of 2+1 years, to begin in 2020. Applicants should send their CV, list of publications, and description of previous research (up to 3 pages), and arrange for at least two letters of reference to be sent directly, to astro @ bgu.ac.il.
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| Post Doctoral Positions in Quantum optics and precision sensing at ANU in Canberra, Australia | Closing date: 2020-01-05
Contact: Sareh Rajabi |
| Applications open for Post Doctoral Positions in Quantum optics and precision sensing at The Australian National University in Canberra, Australia | | ▸ more | Classification: Academic Level A /B
Salary package: $80,439 - $113,165 per annum plus 17% superannuation
Term: Full time, Fixed term (2 years) with a possibility of extension
* Flexible and family friendly role
* On campus childcare facilities
* Support network and mentoring program for early career academics
The Research School of Physics represents Australia's largest university based research and teaching activity in the physics discipline. The School is home to a number of major national facilities such as Australia's largest accelerator and the H1-NF National Stellarator Facility. Hundreds of academics, technical staff and students form the School's greatest asset, its people. This critical mass of researchers is of fundamental importance in fostering the kind of interdisciplinary interactions that create modern research excellence.
The ANU Node of the ARC Centre of Excellence for Gravitational-wave Discovery (OzGrav) conducts research on high precision laser interferometry for gravitational wave detection and other applications. The ARC Centre of Excellence for Engineered Quantum Systems (EQUS) aims to build sophisticated quantum machines to harness the quantum world for practical applications. OzGrav -ANU and EQUS-ANU reside within the Department of Quantum Science at the Research School of Physics, a dynamic group researching applications of quantum and optical technologies in a range of different areas. It co-hosts three ARC Centres of Excellence, an innovations hub that supports start-up companies, and several other major projects.
The Position
We are seeking to appoint up to three experimental physicists to work on optical instrumentation.
The successful candidates should have a PhD or equivalent in physics or a related discipline and a background in optical physics, electro-optics, quantum optics, control systems and low noise electronics.
The Australian National University is a world-leading institution and provides a range of lifestyle, financial and non-financial rewards and programs to support staff in maintaining a healthy work/life balance whilst encouraging success in reaching their full career potential. For more information, please visit https://internaljobs.anu.edu.au/ci/en/listing/
CLOSING DATE: JANUARY 5th, 2020.
To see what the Science at ANU community is like, we invite you to follow us on social media at http://www.instagram.com/anu_science/ and https://www.facebook.com/ScienceANU/.
If you wish to discuss the position after obtaining the selection documentation, please contact: Professor David McClelland, phone (02) 6125 9888, e-mail david.mcclelland @ anu.edu.au.
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| The Australian National University new Centre for Gravitational Astrophysics: Full Professor | Closing date: 2020-01-12
Contact: Sareh Rajabi |
| Call for expression of interest for a Full Professor position at Centre for Gravitational Astrophysics, The Australian National University | | ▸ more | The Australian National University in Canberra, Australia, has recently established a new Centre for Gravitational Astrophysics (CGA), jointly supported by the Research School of Astronomy and Astrophysics and the Research School of Physics.
The Centre encompasses all aspects of gravitational wave physics and astrophysics, including instrumentation, theory and data analysis, source follow-up and multi-messenger astronomy. It will bring together existing ANU researchers in these areas under one umbrella and expand the capability by making up to seven new tenure-track academic appointments across these research programs over the next year. The inaugural CGA Director is Professor David McClelland.
We are now seeking Expressions of Interest for the key appointment of a Full Professor (Level E). It is the intention that the appointee will initially take on the role of Deputy Director, in the anticipation that they will take over as Director within the next five years. We are seeking an inspirational scientific leader with an equity agenda from any area of research covered by the Centre, who can grow ANU?s leadership across all areas of gravitational wave astronomy. If you think you have the skills, vision and drive required to fill this role, please consider applying, regardless of your current level of appointment.
The appointment comes with an attractive start-up package and the ability to help shape the future of the CGA through subsequent faculty hires. This is a tenure-track position with a negotiable probation period.
We are now seeking a 2-page Expression of Interest (EoI), along with a complete CV. EoIs will be accepted any time up to 12 January 2020. We anticipate advertising the position in mid-December with a closing date for applications in late January 2020. You are encouraged to contact Professor David McClelland (david.mcclelland @ anu.edu.au) for further information. Please email your expression of interest and CV to the CGA Administrator, Dr Sareh Rajabi (sareh.rajabi @ anu.edu.au), before the closing date.
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| Tenure-Track Position in Gravitational Astrophysics, The Australian National University | Closing date: 2020-01-15
Contact: Sareh Rajabi |
| Call for expression of interest for a female-only tenure-track position in Gravitational Astrophysics, at the Centre for Gravitational Astrophysics, The Australian National University | | ▸ more | (open to female identifying candidates only)
The Australian National University in Canberra, Australia, has recently established a new Centre for Gravitational Astrophysics (CGA), jointly supported by the Research School of Astronomy and Astrophysics and the Research School of Physics.
The Centre encompasses all aspects of gravitational wave physics and astrophysics, including instrumentation, theory and data analysis, source follow-up and multi-messenger astronomy. It will bring together existing ANU researchers in these areas under one umbrella and expand the capability by making up to seven new tenure-track academic appointments across these research programs over the next year. The inaugural CGA Director is Professor David McClelland.
We are seeking to appoint an outstanding early or mid-career academic with a strong research record in gravitational wave astrophysics (theory and data analysis, source follow-up, multi-messenger astronomy). This will be a tenure-track position attracting a significant start-up package. It will be a key foundation position in the CGA. The appointee will assist with recruiting additional appointments into the CGA, helping to shape its future.
We are now seeking Expressions of Interest (EoI) in this position. An EoI will comprise a 1-page statement of achievement and proposed program of research at ANU, along with a 2-page CV. EoIs will be accepted any time up until January 12, 2020. Please email your EOI to the CGA administrator, Dr Sareh Rajabi, sareh.rajabi @ anu.edu.au, and expect confirmation of receipt.
For further information, please contact Professor Susan Scott (susan.scott @ anu.edu.au) or Professor David McClelland (david.mcclelland @ anu.edu.au) at RSPhys and/or Associate Professor Christian Wolf (christian.wolf @ anu.edu.au) at RSAA.
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| Postdoctoral researcher in exoplanet observations (SAINT-EX) | Closing date: 2020-01-10
Contact: Brice-Olivier Demory |
| Applications are invited for a Postdoctoral position at the Centre for Space and Habitability (CSH, http://csh.unibe.ch) of the University of Bern. The successful applicant will work as a member of the SAINT-EX research team led by Prof. Brice-Olivier Demory (http://www.saintex.unibe.ch). The Postdoctoral researcher will be expected to conduct a competitive research programme in exoplanets and will be coordinating the science operations of the SAINT-EX ground-based observatory. | | ▸ more | SAINT-EX is a 1-m, fully robotic telescope located in San Pedro Martir (Mexico) that focuses 1) on the search for transiting exoplanets orbiting ultra-cool dwarfs (similar to TRAPPIST-1) and 2) in providing ground-based support to the ESA CHEOPS mission (launch Dec 2019). The successful Postdoctoral researcher will also have the opportunity to be involved in the SPECULOOS collaboration. A high-degree of interaction with the CSH members is also expected.
Candidates with previous expertise in exoplanet observations and/or ground-based telescope operations are strongly encouraged to apply.
As per the University of Bern?s rules, candidates to this position should have been awarded their PhD after 1 August 2017.
Starting salary is 87?750 CHF, with an initial appointment of 2 years. Child allowance and maternity/paternity leave are offered. The earliest starting date is 1 August 2020. The position comes with a research budget for travel, publication costs and computing resources.
Applications are invited from all nationalities and should consist of 1) a cover letter, 2) a CV, 3) a research proposal (3 pages), 4) a summary of past achievements (1 page), 5) a list of publications and 6) the names of 3 references. Materials should be submitted through the web interface at:
https://ohws.prospective.ch/public/v1/jobs/3f797e2c-bc5a-4a5e-b80b-276db2397724
Applications received by 10 January 2020 will receive full consideration.
Inquiries to: Prof. Brice-Olivier Demory
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| PhD position in radio/X-ray extragalactic astronomy | Closing date: 2020-02-01
Contact: Francesco De Gasperin |
| We are offering a 3-year PhD position at the University of Hamburg in observational extra-galactic astronomy. The student research will focus on active galactic nuclei, galaxy evolution and/or galaxy cluster science. Specifically, the student will work on low-frequency radio data from LOFAR combined with eRosita X-ray observations of the Virgo cluster. | | ▸ more |
The Observatory offers a diverse and rich research environment. Our teams have strong expertise in radio, X-ray and numerical modeling. The candidate will have privileged use of our own LOFAR station, state-of-the-art computing facilities and early access to large survey data from LOFAR, eRosita, 4MOST. The student will be part of the LOFAR collaboration, which includes hundreds of scientists across the European continent. The Hamburg Observatory is part of the Quantum Universe cluster of excellence, which will link the candidate with a large community of scientists. Funding for computing facility and travels to attend and present at domestic and international meetings will be available. The position comes with no teaching duties, but there is the possibility of gaining teaching experience upon request. A master in astronomy, physics or equivalent is a requirement; good programming skills and knowledge of radio interferometry are important assets.
The application must include:
- a motivational letter (max 1 page)
- transcripts
- CV
- 2 letters of recommendation
Please send all documents via email to Prof. de Gasperin (fdg @ hs.uni-hamburg.de) by February 1st, 2020. Please note that incomplete applications cannot be considered.
The position is expected to begin as early as possible after March 1st, 2020.
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| Postdoctoral Research Position(s) in Observational Extragalactic Astronomy at the University of Geneva | Closing date: 2020-01-10
Contact: Prof. Pascal Oesch |
| Applications are invited for up to two postdoctoral research positions in observational extragalactic astronomy at the University of Geneva, Switzerland. The successful candidates will work in the group "Galaxy Build-up at Cosmic Dawn" with Prof. Pascal Oesch on research projects focused on the first generations of galaxies involving deep multi-wavelength observations from HST, Spitzer, ALMA, VLT+Keck, and soon from JWST. | | ▸ more | Interested candidates will have the opportunity to get involved in several international collaborations, including the ALMA Large Program REBELS, and teams preparing for upcoming facilities such as the multi-object spectrograph VLT/MOONS as well as ESA's Euclid Space Telescope. Candidates with prior experience in photometric redshift measurements or Lyman Break selections are especially encouraged to apply, to prepare for the exploitation of the Euclid Deep Fields for z>6 research.
At the Geneva Observatory and the associated Laboratory of Astrophysics of the Swiss Federal Institute of Technology in Lausanne (EPFL), the successful candidates will find a rich and vibrant research environment in the fields of extra-solar planets, stellar physics, high energy astrophysics, galaxy evolution, and observational cosmology.
The initial appointment will be for one year, renewable annually, contingent upon satisfactory performance, mutual agreement, and availability of funds. The appointments are expected to start mid 2020, and require the completion of a PhD in Astronomy, or related field.
To apply, qualified candidates are encouraged to send an email with a single PDF file to pascal.oesch @ unige.ch containing a cover letter, a CV with publication list, and a brief research statement. Candidates should also arrange for three letters of reference to be e-mailed to the same address.
Applications received by January 10, 2020, will receive full consideration.
Preliminary inquiries may be addressed via e-mail to pascal.oesch @ unige.ch.
For more information on our group, please visit: https://www.unige.ch/sciences/astro/cosmicdawn/en/
Included Benefits:
Standard Swiss Social Security, Accident Insurance and Pension contributions.
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| PhD position in exoplanet observations | Closing date: 2020-01-15
Contact: Francois Bouchy |
| Applications are invited for a PhD position within the exoplanet team at the University of Geneva to work on photometric observations of transiting exoplanets. The main focus of the PhD thesis will be to study the density of exoplanets by deriving their precise radii from light curve analysis of NGTS, K2 and TESS surveys and complementary follow-up observations. | | ▸ more | The successful candidate is expected to contribute to the follow-up activities, and focus on retrieving the signatures of Super-Earth and Neptune-like planets with high-precision photometry. While the PhD project will be based on photometric observations, he/she will also participate in ongoing high-precision RV follow-up using CORALIE, HARPS and NIRPS. The successful candidate will be in charge to the transit modelling, identification of false positives, ranking and vetting of transiting candidates, coordination, execution and analysis of photometric observations carried out with EulerCam at the 1.2 m Euler telescope at La Silla observatory. He/She will also contribute to the activities of the NGTS transit survey and to DACE platform tools related to light curve analysis.
The Department of Astronomy of the University of Geneva offers a modern and vibrant work environment, with a wide range of activities including theory, numerical simulations, observations and instrumental developments in the domains of exoplanets, stellar physics, galactic dynamics, observational cosmology and high-energy astrophysics. The exoplanet team is especially well renown, with strong involvement in planet detection, the determination of the planet physical properties, the characterisation of planet atmospheres, and the development of an associated world-class instrumentation. We are also co-leading the Swiss-wide National Centre of Competence in Research (NCCR) PlanetS (http://nccr-planets.ch/), dedicated to the study of the origin, evolution, and characterisation of planets inside and outside our Solar System. The applicant will also have the opportunity to develop collaborations with members of PlanetS.
The applicant is required to have a Master in Astrophysics. Proficiency in Python programming is considered as a plus. This four-year PhD position is founded by Swiss National Science Foundation with a gross salary around 50,000 CHF a year. The position is available immediately and a rapid start by the student would be appreciated. The University is actively seeking to increase the numbers of women in physics and hence women are strongly encouraged to apply. Interested applicants should send (in a single pdf file) a curriculum vitae, academic transcripts, a motivation letter including information on skills and previous experience, names of people who can be contacted for a letter of recommendation, and the contact details to Prof. François Bouchy, University of Geneva, francois.bouchy @ unige.ch, before 15th January 2020.
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| Post-doctoral position in exoplanet observations | Closing date: 2020-01-15
Contact: Monika Lendl |
| Applications are invited for a postdoctoral position within the Swiss research platform PlanetS to work on photometric observations of transiting exoplanets. PlanetS (http://nccr-planets.ch/) is a Switzerland-wide research network for planetary sciences with a large focus on exoplanets. The available position is co-offered by the University of Geneva and the University of Bern. It will be located primarily within the exoplanet team at the University of Geneva, with a 6-month stay foreseen at the University of Bern. | | ▸ more | The successful candidate is expected to contribute to the follow-up of long-period transiting planets detected by space-based surveys (TESS, K2) and contribute to their interior modelling. He/She will participate in ongoing observing programs of the Geneva exoplanet team, consisting of radial-velocity (CORALIE, HARPS, NIRPS) and photometric (EulerCam, NGTS) observations. He/she will be charged mainly with the analysis of photometry, with a particular focus on the confirmation of long-period giant planets, most importantly single-transit candidates. He/she is expected to complete tasks including light curve modeling, target selection, prioritisation and the joint analysis of photometric and RV data. He/she will spend six months at the University of Bern to conduct the interior modelling of long-period planets using the Bern planetary evolution and structure models.
PlanetS presents a vibrant research environment with a wide range of activities including theory, numerical simulations, observations and instrumental developments related to exoplanets. The successful candidate will have ample opportunity to collaborate within PlanetS, in particular with regard to the CHEOPS space mission and projects related to the characterisation of planetary atmospheres. The exoplanet team at the University of Geneva is renown for its strong involvement in planet detection, the determination of the planet physical properties, the characterisation of planetary atmospheres, and the development of an associated world-class instrumentation.
Applicants are expected to have completed a PhD in Astronomy or Astrophysics or expect to complete it by the start of the position. Applicants are also expected to have experience in observation, data reduction and analysis, especially related to high-precision photometry. Additional experience with either theoretical modelling of planetary interiors or high-precision radial-velocities would be advantageous.
The duration of the appointment is initially for two years, with a possible prolongation for a third year depending on performance and available funding. This position is funded by the Swiss National Science Foundation with a gross salary around 80,000 CHF a year. The position is available immediately and to be started at latest on 1 May 2020. Interested candidates should contact Dr. Monika Lendl at the University of Geneva. Applications should be sent via email to monika.lendl @ unige.ch and contain (in a singe pdf file) 1) curriculum vitae, 2) list of publications, 3) a short research statement describing past achievements and future projects (max. 2 pages) and arrange for two letters of recommendation to be sent before 15 January 2020.
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| PhD positions in Prague: theory, instrumentation, observations | Closing date: 2020-01-15
Contact: PhD program committee |
| We are inviting applications for multiple 4-year PhD positions in Prague, Czech Republic, in the fields of Astronomy & Astrophysics, Astroparticle Physics, Cosmology, Gravitational Physics, Mathematical Physics, and String Theory. The areas of research include theory, observation, and instrumentation. Some of the projects are part of large international collaborations (LSST, Pierre Auger, CTA, ASAS-SN). The list of available projects is at http://physicsphd.cz/. We will continue to update the website and add more projects until early December. | | ▸ more | PhD thesis research will be conducted at one of the participating institutions in Prague: Charles University (Institute of Theoretical Physics and Astronomical Institute), Institute of Physics of the Czech Academy of Sciences, Astronomical Institute of the Czech Academy of Sciences, and Institute of Mathematics of the Czech Academy of Sciences. The PhD degrees are awarded by Charles University. The positions are funded by individual grants (both national and EU, including ERC grants or equivalents) and institutional fellowships. The positions are open to candidates of any nationality.
PhD students receive medical insurance with no or small co-pays, subsidized meals, possibility of staying in student dormitories, and free "Czech as foreign language" classes. There are no fees or tuition for PhD students. Prague remains cheaper than other comparable European cities while offering similar level of comforts and entertainments.
For more information and application procedure, please see http://physicsphd.cz. The application deadline is January 15 2020 for positions beginning in the Fall semester of 2020.
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| User Support Astronomer | Closing date: 2020-01-20
Contact: Pauline Conlon |
| The European Organisation for Astronomical Research in the Southern Hemisphere (ESO) is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. | | ▸ more | The User Support Department is the main interface between the La Silla Paranal Observatory and the Service Mode users of its facilities. The department is part of the Data Management and Operations Division which provides high-reliability support to the operation of the ESO facilities and to their community of users in the framework of an integrated end-to-end system and maintains the archive facility and its data holdings as a powerful resource for both scientific and operational use.
The User Support Department is looking for an astronomer with a strong and active research profile. The post holder should have a strong interest in maximizing ESO's science output through conducting expert user support and contributing to the development of efficient processes, tools and high-quality documentation for the user community.
Main Duties and Responsibilities
The successful candidate will be responsible for the support of Service Mode users of the La Silla Paranal Observatory facilities and of VLT and/or VLTI operations.
The main tasks include:
- Support the users of the Very Large Telescope (VLT) and/or the Very Large Telescope Interferometer (VLTI) in the areas of Phase 1 (observing proposal preparation) and Phase 2 (review of observation blocks and observing strategy) as well as providing helpdesk support including post-observation support for data reduction;
- Support the Paranal Observatory during programme execution and follow-up;
- Have an active role in the operation teams of the instruments to be supported; and
- in the medium term, become involved in preparations for ELT operations and support of its users.
As an astronomer and member of the ESO Science Faculty, you will be expected and encouraged to conduct astronomical research and participate actively in the scientific life of ESO. Research in areas directed towards using the capacities of the VLT/VLTI and ALMA and future capabilities of the ELT will be strongly encouraged.
Reports to:
Head of the User Support Department.
Key Competences and Experience
Essential Competences and Experience:
- Several years of active astronomical research at least at postdoctoral level with a solid publication record;
- Familiarity with a broad range of instrumental, data analysis, and observational techniques;
- Experience in the use of current large observing facilities, either ground- or space-based;
- Solid knowledge of at least one of the major data reduction packages;
- Excellent cross-disciplinary communication skills both oral and written;
- Pro-active approach to contribute ideas for improvement and future developments;
- Effective and committed team member able to build effective links across different teams;
- Excellent organisational and time-management skills;
- Open and friendly attitude to interact with a variety of users.
Desirable Competences and Experience:
- Experience in optical and near-IR spectroscopy and/or with Adaptive Optics assisted observations;
- Familiarity with Python and SQL;
- Ability to work efficiently in a multi-cultural environment both independently and within a team.
Qualifications:
Essential educational level: Ph.D. in Astronomy, Physics or equivalent.
Language skills:
The position requires an excellent working knowledge of English.
Remuneration and Contract:
We offer an attractive remuneration package including a competitive salary (tax free), comprehensive pension scheme and medical, educational and other social benefits, as well as financial help in relocating your family and the possibility to place your child/children in daycare.
The contract is for a fixed term duration of three years, and is subject to successful completion of the probation period. There may be a possibility of extension(s) subject to individual performance and organisational requirements as defined in the applicable policies and staff rules and regulations. For any further information, please visit ESO's conditions of employment.
Duty Station:
Garching near Munich, Germany. The post holder will be requested to make occasional duty trips to the La Silla Paranal Observatory in northern Chile.
Career Path: V
Application:
If you are interested in working in areas of front-line science and technology and in a stimulating international environment, please visit http://www.eso.org for further details.
Applicants are invited to apply online at http://recruitment.eso.org/. Applications must be completed in English and should include a motivation letter, a CV containing a publication list and a research statement. Also required are the names and contact details of three persons familiar with your work and willing to provide a reference letter. Referees will be automatically invited to submit their letter, however, applicants are strongly advised to trigger these invitations (using the web application form) well in advance of the application deadline.
Deadline for applications is 9 January 2020.
Interviews are expected to start soon after this date.
No nationality is in principle excluded, however, recruitment preference will be given to nationals of Australia, Austria, Belgium, the Czech Republic, Denmark, Finland, France, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland, the United Kingdom and Chile irrespective of gender, age, disability, sexual orientation, race or religion.
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| PhD positions in Astrophysics at the University of Hertfordshire | Closing date: 2020-02-01
Contact: Sugata Kaviraj |
The Centre for Astrophysics Research (CAR) at the University of
Hertfordshire is offering several PhD positions to commence in Oct
2020 | | ▸ more | Several STFC scholarships are available for UK students.
University-funded scholarships (which provide full funding) are
available for EU and international students. In addition, the
Bell-Burnell fund, administered by the IoP, aims to support full or
part-time graduates who wish to study towards a doctorate in physics
and are from groups that are currently under-represented in physics.
For the purpose of this fund the definition of under-represented
groups refers to: women, students of Black-Caribbean, Black-African
and other minority ethnic (BAME) heritage, students with disabilities,
or who require additional funding to support inclusive learning, LGBT+
students and students from disadvantaged backgrounds who may struggle
to find the levels of funding needed to complete their studies.
https://www.herts.ac.uk/research/centres/car/research-degrees-and-studentships
Priority will be given to applications received by 1 Feb 2020. Those
wishing to apply to study at Hertfordshire through the Bell-Burnell
fund should contact the Postgraduate Tutor (s.kaviraj @ herts.ac.uk) as
soon as possible (and no later than 15 Dec 2015, see webpage above for
more details).
The Centre has a strong research programme, across a broad spectrum of
theoretical and observational topics and is offering projects in the
following areas:
Galaxies, Active Galactic Nuclei and Cosmology
https://www.herts.ac.uk/research/centres/car/research-degrees-and-studentships/phd-projects/galaxies-active-galactic-nuclei-and-cosmology
Star formation and Stellar Evolution
https://www.herts.ac.uk/research/centres/car/research-degrees-and-studentships/phd-projects/star-formation-and-stellar-evolution
Extra-solar planets and brown dwarfs
https://www.herts.ac.uk/research/centres/car/research-degrees-and-studentships/phd-projects/extrasolar-planets-and-brown-dwarfs
Prospective applicants who wish to find out more about the department
or the projects on offer are encouraged to contact their prospective
supervisors (who are listed at the top of each project description).
General enquiries about the process may be addressed to Dr Sugata
Kaviraj, the Postgraduate Tutor (s.kaviraj @ herts.ac.uk)
|
| Postdoctoral Position in Fast Radio Burst Science | Closing date: 2020-01-05
Contact: Human Resources |
This post is a Postdoctoral research position in precision cosmology using fast radio bursts.
This position will be a 3-year full-time 100-percent research role within the SKA Science Team, working with Dr. Evan Keane. The role involves research in the field of Fast Radio Burst (FRB) science as part of the SUPERHeRO project; this is funded by a grant from Fondation MERAC.
Application Deadline: January 5th 2020
Application method: Online at this URL: https://recruitment.skatelescope.org/vacancy/postdoctoral-position-in-fast-radio-burst-science-402213.html | | ▸ more | The Role
This position will be a 3-year full-time 100-percent research role within the SKA Science Team, working with Dr. Evan Keane. The role involves research in the field of Fast Radio Burst (FRB) science as part of the SUPERHeRO project; this is funded by a grant from Fondation MERAC. The goals of this project are to increase the precision with which one can use FRBs as cosmological probes, with an emphasis on the Helium Epoch of Reionization. In particular three main lines of investigation will be pursued: 1. improving models of the Milky Way's electron density distribution; 2. understanding artefacts and biases in the observed FRB population as a result of the systems used to find them; 3. "FRB Origins" - understanding the progenitors of FRBs, e.g. through studies of their environments. Additionally, time will be available for the pursuit of other related research pursuits.
Key Responsibilities, Accountabilities and Duties
The main responsibility of the role is to perform research so as to progress the field of FRB cosmology towards being a precision science in pursuit of the goals of the SUPERHeRO project. It is expected that knowledge from traditional observational cosmology will be integrated with knowledge from traditional radio astronomy to improve the potential for performing FRB cosmology. The results obtained from this work will be published in the scientific literature. The role is based at SKA Headquarters at Jodrell Bank Observatory in Cheshire, UK. No travel is required as part of this role. Support for Carbon-offset travel is available for attendance at conferences, workshops, meetings and for collaborative visits, if desired.
Mandatory Knowledge, Skills and Experience
* PhD in radio astronomy, astrophysics or a closely related discipline
* A track record of publication in one or more of the following areas: fast radio bursts, interstellar medium, cosmology.
* Expertise in software programming, analytical and numerical modelling
* Familiarity with Milky Way electron density models
* Familiarity with time-domain radio astronomy observing systems
* Excellent communication and inter-personal skills
* Flexible team player who is adaptable to change, able to work independently and as part of a team.
Desirable Knowledge, Skills and Experience
* Experience in the quantification of cosmology foregrounds
* Experience in algorithms used to detect fast radio bursts
* Experience in radio frequency interference mitigation
* A track record of observations of fast radio burst sites
Equal Opportunities Statement
Equality, Diversity and Inclusion are at the core the SKA's agenda and we are committed to being an equal opportunities employer. Our aim to is recruit and retain the most talented individuals, regardless of gender, race, disability, age, sexual orientation, marital status, religion or nationality.
Women have traditionally been under-represented in the fields of science and engineering; SKA Organisation welcomes and encourages female applicants.
Where applicants with a disability need facilities or adjustments to enable them to participate in the recruitment process, these will be provided.
|
| Postdoctoral Position in Fast Radio Burst Science | Closing date: 2020-01-05
Contact: Human Resources |
This post is a Postdoctoral research position in precision cosmology using fast radio bursts.
Click here to apply online via our recruitment portal: https://recruitment.skatelescope.org/vacancy/postdoctoral-position-in-fast-radio-burst-science-402213.html | | ▸ more | The Square Kilometre Array (SKA) is a global project to build a multi-purpose radio telescope that will play a major role in answering key questions in modern astrophysics and cosmology. Thirteen countries are now participating in the project, with others engaged in discussions regarding possible membership. Facilities for the new telescope will be located in South Africa and Australia, with our headquarters in a purpose-built building at Jodrell Bank, Cheshire, UK. SKA HQ currently houses around 90 staff but has just undergone a major expansion to accommodate up to 150 staff as the project moves towards construction and operation of the SKA telescopes.
Negotiations between the governments of SKA member countries to establish the SKA Observatory as an Inter-Governmental Organisation (IGO) have recently concluded; the IGO is expected to be established in late 2020.
This post is a Postdoctoral research position in precision cosmology using fast radio bursts.
The Role
This position will be a 3-year full-time 100-percent research role within the SKA Science Team, working with Dr. Evan Keane. The role involves research in the field of Fast Radio Burst (FRB) science as part of the SUPERHeRO project; this is funded by a grant from Fondation MERAC. The goals of this project are to increase the precision with which one can use FRBs as cosmological probes, with an emphasis on the Helium Epoch of Reionization. In particular three main lines of investigation will be pursued: 1. improving models of the Milky Way's electron density distribution; 2. understanding artefacts and biases in the observed FRB population as a result of the systems used to find them; 3. "FRB Origins" - understanding the progenitors of FRBs, e.g. through studies of their environments. Additionally, time will be available for the pursuit of other related research pursuits.
Key Responsibilities, Accountabilities and Duties
The main responsibility of the role is to perform research so as to progress the field of FRB cosmology towards being a precision science in pursuit of the goals of the SUPERHeRO project. It is expected that knowledge from traditional observational cosmology will be integrated with knowledge from traditional radio astronomy to improve the potential for performing FRB cosmology. The results obtained from this work will be published in the scientific literature. The role is based at SKA Headquarters at Jodrell Bank Observatory in Cheshire, UK. No travel is required as part of this role. Support for Carbon-offset travel is available for attendance at conferences, workshops, meetings and for collaborative visits, if desired.
Mandatory Knowledge, Skills and Experience
- PhD in radio astronomy, astrophysics or a closely related discipline
- A track record of publication in one or more of the following areas: fast radio bursts, interstellar medium, cosmology.
- Expertise in software programming, analytical and numerical modelling
- Excellent communication and inter-personal skills
- Familiarity with Milky Way electron density models
- Familiarity with time-domain radio astronomy observing systems
- Excellent communication and inter-personal skills
- Flexible team player who is adaptable to change, able to work independently and as part of a team.
Desirable Knowledge, Skills and Experience
- Experience in the quantification of cosmology foregrounds
- Experience in algorithms used to detect fast radio bursts
- Experience in radio frequency interference mitigation
- A track record of observations of fast radio burst sites
Equal Opportunities Statement
Equality, Diversity and Inclusion are at the core the SKA's agenda and we are committed to being an equal opportunities employer. Our aim to is recruit and retain the most talented individuals, regardless of gender, race, disability, age, sexual orientation, marital status, religion or nationality.
Women have traditionally been under-represented in the fields of science and engineering; SKA Organisation welcomes and encourages female applicants.
Where applicants with a disability need facilities or adjustments to enable them to participate in the recruitment process, these will be provided.
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