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PhD Opportunity in Gravitational-Wave Astronomy and Next-Generation Detectors in Valencia/Barcelona

The Instituto de Física Corpuscular (IFIC, Valencia), a joint Universitat de València–CSIC research centre, and the Institute of Space Sciences (ICE-CSIC, Bellaterra, Barcelona), invite applications for a PhD opportunity in gravitational-wave astronomy, with a focus on next-generation detectors such as LISA, Einstein Telescope, and Cosmic Explorer. Application deadline: July 19th 2026.

The project will focus on the development and application of advanced data-analysis techniques for gravitational-wave science, including machine learning and deep learning methods, classical and quantum computing approaches, and global-fit techniques for complex astrophysical signals. Research activities will be carried out jointly between the Universitat de València and the Institute of Space Sciences, with collaborations involving the Barcelona Supercomputing Center.

We welcome applications from candidates with backgrounds in physics, astrophysics, cosmology, data science, computer science, or related disciplines. Experience in scientific programming, machine learning, statistics, or gravitational-wave physics will be particularly welcome.

Interested candidates should submit a CV, a short statement of research interests, academic transcripts, and the names and contact details of two referees.

Contact:Sopuerta, Carlos F. (carlos.f.sopuerta(at)csic.es); Ruiz de Austri, Roberto (rruiz(at)ific.uv.es)

Please find here details.

Expression of interest for postdoctoral positions in GW tests of general relativity, Rome, Italy

We invite expressions of interest for postdoctoral positions at the Italian Institute for Nuclear Physics (INFN) in Rome, Italy. The postdoctoral positions will be funded under the Italian Fund for Science (FIS) Starting Grant Eyes-on-GR, whose goal is testing general relativity with multiband gravitational-wave observations.

We are particularly eager to receive expressions of interest from candidates with experience in (i) data analysis with current and next-generation detectors (ii) modeling deviations from general relativity in modified theories of gravity and horizonless compact objects.

The postdocs will join the new research group Eyes-on-GR led by Dr. Elisa Maggio at INFN Rome, Italy. INFN Rome is located inside Sapienza University, one of the largest Universities in Europe. The postdocs will have the possibility to join the Virgo, Einstein Telescope and LISA groups in Rome. The INFN Virgo Rome group has about 35 researchers including PhD students, postdocs and 18 faculty.

The postdoctoral positions are expected to start between Fall 2026 and Spring 2027 and can last 2+1 years. All candidates must hold or soon be completing a Ph.D. in Physics, Astronomy or Astrophysics. Interested candidates should send (i) a motivation letter, (ii) a curriculum vitae, indicating the date the PhD was or will be awarded (iii) a research statement, and (iv) two contacts for reference letters.

Expressions of interest should be sent via the Google Form in the external link, and reference letters should be sent to Elisa Maggio (elisa.maggio[AT]roma1.infn.it).
Candidates are encouraged to apply as soon as possible. The deadline for full consideration of the expressions of interest including reference letters is June 19th, 2026.

Please, fell free to forward this announcement to potential candidates. For any other information, please do not hesitate to reach out to Elisa Maggio (elisa.maggio[AT]roma1.infn.it).

Please find here details.

Research Postdoctoral Position at Maynooth University, Ireland

We are seeking a Post Doctoral Researcher to work in Dr. John Regan’s research group conducting high quality research in astrophysics in the field of massive black hole formation at high redshift.  Specifically, the role will require the candidate to actively analyse and disseminate data from the SEEDZ datasets. This will require the candidate to have existing skills in computational astrophysics, high redshift astrophysics, galaxy formation and massive black hole formation and growth. The successful candidate will also be expected to interact with other member of Dr. Regan's group furthering the group's research Goals. 

The successful candidate will also be expected to interact with other member of Dr. Regan’s group furthering the group’s research goals

Salary: Post Doctoral Researcher (2026) € 46,805– 49,395 p.a. (3 points – with increments)

Appointments will be made in accordance with public sector pay provisions.

Closing Date: 23:30hrs (local Irish time) on Sunday, 21st of June 2026.

Applications must be submitted by the closing date and time specified above. Any applications which are still in progress at the closing time on the specified closing date will be cancelled automatically by the system.

Late applications will not be accepted.

Please find here full details.

Director Position at Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo

The Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU) invites applications for the position of Director for a five-year term starting on April 1, 2028.

Kavli IPMU has ambitious goals to discover the fundamental laws of nature and to understand the universe from synergistic perspectives of mathematics, theoretical and experimental physics, cosmology, and astrophysics. Kavli IPMU is an international research institute established in October 2007 with English as its official language. Its annual budget is approximately $11M. Kavli IPMU is on the Kashiwa campus of the University of Tokyo and has a branch in Kamioka. More than half of all scientific members come from outside Japan. We aim to maintain and strengthen our diverse and highly interactive membership.

The successful candidate is expected to carry out the following:

(i) actively manage research activities across the fields of mathematics, theoretical and experimental physics, and cosmology/astrophysics,
(ii) be responsible for the operation of the institute, efforts of the administrative staff, handling of reviews, reporting, and running committees,
(iii) interact and negotiate with the headquarters of the University of Tokyo,
(iv) lead efforts on establishing a longer term research plan beyond the term of the Director and
(v) if desired, continue to carry out their own scientific research programs.

Candidates are further required to have a high integrity of character, excellent academic knowledge, and strong leadership skills. In case of joint appointments, the Director must be effectively acting as a University of Tokyo employee for at least half of each year. The appointment comes with the title of Full Professor with tenure until the retirement age set by the University of Tokyo. Salary will be negotiated within the bounds set by the University of Tokyo system. The steering committee of Kavli IPMU retains the ability to impose additional requirements, if needed.

Interested and qualified candidates are encouraged to apply including underrepresented minorities, female scientists, and international applicants. For prescreening, the application should simply include a CV, including a date of birth if there are no legal or ethical reasons to not do so. The CV should be uploaded through Academic Jobs Online at https://academicjobsonline.org/ajo/jobs/32058/apply. Applications received before July 24, 2026 will receive full consideration.

Please find here details.

Research Position at INAF – Arcetri Astrophysical Observatory in Florence, Italy

Observations of massive black hole binaries for the LISA mission
Application deadline: 7 June 2026, 23:59 Italian time

The Istituto Nazionale di Astrofisica (INAF) has opened a public competition for 1 fixed-term Researcher position (Third Professional Level) at the Osservatorio Astrofisico di Arcetri in Florence, Italy.

Main Information

Position: Researcher (full-time, fixed-term)
Contract duration: 12 months, with possible extension
Research topic: Multiwavelength observations of dual and binary AGN as precursors of gravitational wave events detectable by LISA; study of merger rates of massive black holes and comparison between observations and theoretical predictions. Participation to the Italian LISA low-latency WG.
Workplace: INAF – Arcetri Astrophysical Observatory, Florence, Italy
Gross salary: about 38.000 Euro
Competition code: 2026INAFRIC-OAA-LISA-003
Official call for applications (in Italian): http://www.inaf.it/it/lavora-con-noi/concorsi-e-selezioni/posizioni-a-tempo-determinato/ricercatori/2026inafric-oaa-lisa-003

Required qualifications

Applicants must have:

  • A Master’s degree (or equivalent) in Physics, Astronomy, Astrophysics, or related fields
  • A PhD in Physics, Astronomy, or Astrophysics OR at least 3 years of documented post-graduate research experience in related topics

Applicants with foreign degrees are eligible to apply. Degrees obtained abroad will be accepted provided they are equivalent to the required Italian qualifications. The formal recognition process is required only for the selected candidate.

Citizenship requirements

The call is open to:

  • EU citizens
  • Non-EU citizens with long-term EU residence permits
  • Refugees or individuals with subsidiary protection status
  • Family members of EU citizens with residence rights in the EU

Application Procedure

Applications must be submitted online only through the Italian public recruitment portal: inPA Recruitment Portal

The application platform used is PICA/CINECA: PICA Platform

For more information please write to Filippo Mannucci filippo.mannucci(at)inaf.it

Fellow position in the Intelligent Hardware Lab (IHL) of the Cluster of Excellence Color meets Flavor in Germany

We would like to draw your attention to a newly opened Fellow position in the Intelligent Hardware Lab (IHL) of the Cluster of Excellence Color meets Flavor in Germany.

The position focuses on FPGA-based systems, intelligent detector electronics, and AI/ML-driven real-time processing for physics applications, including low-latency and resource-efficient hardware implementations.

Given the overlap with topics relevant to real-time data processing and intelligent instrumentation, I thought this position might also be of interest within the ET community.

The full advertisement is available on INSPIRE:

https://inspirehep.net/jobs/3154506

Research associate in GW instrumentation at ULiege

Open position for: Research associate (“logisticien.ne de Recherche”) (Gravitational waves instrumentation) University of Liège for a permanent contract (full time) starting ideally start on the 1st of September 2026. Application deadline: May 30th, 2026.

Context and missions
The Einstein Telescope (ET) will be Europe’s most advanced observatory for gravitational waves. It will allow researchers to hear black holes mergers and learn about the early universe.

The department of aerospace and mechanical engineering of University of Liège hosts the ET-CRISTAL facilities. ET-CRISTAL is an R&D facility for demonstrating crucial aspects of ET-Low Frequency. It uses innovative approaches for seismic isolation, i.e. an inverted pendulum stage on top of active seismic isolation platform and contact-free radiative cryogenic cooling of a large-scale cryogenic mirror. ET-CRISTAL is a Center of Excellence for the sub-system comprising the mirror, its suspension system, the vibration Isolation system, and cryogenic cooling of the mirror.

The Precision Mechatronics Laboratory within the Department of Aerospace and Mechanics (A&M) and from the School of Engineering at the University of Liège invites applications for an open position as a research associate in gravitational wave instrumentation at ET-CRISTAL. The facilities are installed at the Space Center (CSL) of the University of Liège and the main research offices of the Precision Mechatronics Laboratory are located within the Department.

As a Research Associate, you will have as missions to:

  • Lead the management of ET-CRISTAL facilities together with the Scientific Director (Prof. C. Collette), including research logistics, participation and tutoring of Master and PhD students as well as fellow researchers.
  • Develop and support research activities in fields relevant to ET-CRISTAL
  • Contribute to securing new funding and develop new collaborations

Application requirements

  • To hold a PhD in engineering, or an equivalent experience.
  • To have proven experience in one or several of these fields:
    • cryogenic inertial sensors
    • low frequency seismic isolation
    • radiative cooling
    • thermal noise modeling
    • Newtonian noise

You must also have strong project management skills, as well as excellent written and oral communication skills in English and, if possible, in French. You should be able to take the initiative and be skilled in negotiation and consensus-building.

We offer

  • A pleasant and dynamic work environment with a wide variety of assignments
  • Significant freedom in how you organize your work and a degree of autonomy in decision-making
  • Salary based on established pay scales and pre-determined pay Progression plans
  • The opportunity to support fundamental and applied research related to a Major Big Science instrument in an international Environment

Additional information
Prof. Dr. Ir. christophe.collette(at)uliege.be

ET-CRISTAL: https://www.etest-emr.eu
Precision Mechatronics Laboratory: https://www.pml.uliege.be
Liège Space Center: https://www.csl.uliege.be/cms/c_10241774/en/csl?id=c_10241774
University of Liège: https://www.uliege.be/cms/c_8699436/en/uliege

Application modalities
Applications should include a complete curriculum vitae, a personal motivation letter, and the name of three references in a single PDF file which should be sent by email to Prof. Christophe Collette (christophe.collette(at)uliege.be ) by the 30th of May 2026.

Please find here full details.

PhD position in GW instrumentation at ULiege

PhD position in GW instrumentation at University of Liège Precision Mechatronics Laboratory (PML) invites applications for a PhD position in gravitational wave instrumentation at University of Liège. PML is an active member of the LIGO Scientific Collaboration, and of the Einstein Telescope Collaboration. The group is coordinating ET-CRISTAL, a full-scale prototype of large cryogenic mirror, demonstrating sub-Hertz seismic isolation, and cryogenic cooling using purely radiative technology.
Application deadline May 30th, 2026.

The prototype is installed at the Space Center (CSL) of the University of Liège. University of Liège is a Belgian public university located at the heart of Europe in the cross-border region between the Netherlands and Germany, counting 11 faculties and nearly 30 000 students.

Capitalizing on this unique facility, the objective of this PhD is to develop an interferometric gradiometer that will be validated as a probe of Newtonian noise in the prototype. The project will be realized in close collaboration with the EPFL in Switzerland.

Applicants should hold a Master degree in engineering, physics or equivalent. The position is fully funded for a duration of four years and should ideally start on the 1st of September 2026. Applications should include a curriculum vitae, a personal motivation letter, and the name of three references. Applications should be sent by email to Prof. Christophe Collette (christophe.collette(at)uliege.be ) by the 30th of May 2026.

For more information:
ET-CRISTAL: https://www.etest-emr.eu
Precision Mechatronics Laboratory: https://www.pml.uliege.be
Liège Space Center: https://www.csl.uliege.be/cms/c_10241774/en/csl?id=c_102417
University of Liège https://www.uliege.be/cms/c_8699436/en/uliege

Please find here full details.

The RING project in Germany: 1 Postdoc and 14 PhD positions in Physics, Geophysics, Geodesy

we would like to draw your attention to the 4-year RING project recently funded by the German Research Foundation (extendable to 8 years). The project has strong overlap with gravitational wave detection research on instrumentation.

The project aims at pushing the sensitivity and stability limits of rotational motion sensing with ring laser technology into new realms using approaches from quantum optics and metrology. The ultimate goal is to enable ring laser observations as a complement to classic space-geodetic methods towards more precise, high-rate estimation of Earth Orientation Parameters (EOP). Furthermore, we plan to develop (trans-) portable ring lasers fit for weak, broadband 6 degree-of-freedom ground motion observations towards better understanding of atmosphere-solid Earth coupling (also relevant for seismic decoupling of gravitational wave detection facilities).

The project offers postdoctoral and PhD topics in laser physics, geodesy, geophysics, hydrology, and seismology. The successful candidates will be part of a multi-disciplinary research team at various institutions in Germany with excellent training and experimental facilities.

More information, links to the individual research projects and open positions can be found here:
https://www.ringlaser.de


Prof. Dr. Katharina Isleif
https://www.hsu-hh.de/karriere/wp-content/uploads/sites/658/2026/04/Reference-Number-MB-0926.pdf

Prof. Dr. Oliver Gerberding
https://www.physik.uni-hamburg.de/en/iexp/gruppe-gerberding/offene-stellen.html

Call for postdoctoral positions at Université Paris-Saclay

The Graduate School of Physics at Université Paris-Saclay, France, is launching the second call of its new postdoctoral fellowship program: UPSaclay-STAR-φ, supported by the EU Marie Skłodowska-Curie COFUND. The program will recruit up to 41 international postdoctoral researchers over two calls, for 24-month projects in one of the 40 laboratories of the Graduate School, working on various fields from fundamental to applied physics. The CMS group of CEA-Saclay IRFU (contact: julie.malcles(at)cea.fr) is a possible host group, among others. The application deadline for the first call is July 15, 2026 at 5pm and the expected start of fellowships early 2027 (flexible).

Applicants will have to propose their own research project, with freedom of choice (in agreement with the thematics of interest of the CEA-Saclay/IRFU CMS team).

The CMS CEA-Saclay group has contributed to the design, construction and operation of the ECAL of CMS and is involved in the upgrades of the CMS detector (ECAL, MTD and HGCal).
The group is involved in the ECAL calibration and our analysis activities in Run3 include Higgs to Zy, double Higgs in the bb tautau channel, deep learning for ECAL and MTD reconstruction and various topics related to the diphoton channel (ttH/tH and its CP properties, high mass searches, interference to constraint the Higgs boson natural width with the mass measurement).

To be eligible, applicants must not have resided or carried out their main activity in France for more than 12 months during the 3 years preceding the deadline for applications.

For further information, please visit: http://www.cofund-physics.universite-paris-saclay.fr/