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Software Developer – Infrastructure and Systems Support at EGO, Pisa

The European Gravitational Observatory (EGO) is seeking a Software Developer-Infrastructure and Systems Support to join Information Technology Department. Application Deadline: 25 June 2025.

Activities

The selected candidate will be part of the team that supports the software development and the system and infrastructure

About Software Development (Core Focus)

  • Design, develop, and maintain backend applications including APIs, web services, and client/server tools.
  • Implement robust, scalable, and maintainable code using Python, Bash, or similar languages.
  • Contribute to the evolution of services through continuous integration and deployment pipelines.
  • Ensure high code quality with testing, documentation, and collaborative development practices (e.g., GitLab).

About Systems and Infrastructure Support

  • Participate in the configuration and maintenance of infrastructure components supporting the developed software (e.g., databases, web services).
  • Support the development and operation of data ingestion pipelines and automated workflows.
  • Assist in managing MS-Windows services (such as AD domain services) as needed for integrated infrastructure support.

About Operations and Monitoring

  • Set up and manage tools for system monitoring, logging, and alerting.
  • Perform performance tuning, availability checks, and system diagnostics.
  • Maintain service reliability through automation and preventive maintenance.

Essential skills

  • Master’s degree in a technical or scientific discipline.
  • Demonstrated experience in software development for backend or infrastructure-related applications.
  • Proficiency with Python and/or Bash for scripting and application development.
  • Familiarity with Linux and Windows server environments.
  • Understanding of relational databases and API-based architectures.
  • Experience with Git version control.
  • Knowlegde of English

Other desired skills

One or more of the following will be an asset:

  • Experience with MS-Windows Active Directory Domain management and services.
  • Familiarity with identity and access management concepts (e.g., SSO, MFA, token-based auth).
  • Hands-on experience with configuration management tools like Puppet or Ansible.
  • Experience supporting user environments in research or collaborative scientific computing.

Work Context

EGO is an international consortium, founded by INFN and CNRS to foster European collaboration in gravitational-wave research. EGO is located in Cascina, near Pisa – Italy, and hosts and operates the gravitational-wave detector Virgo, a 3 km-long laser interferometer (ITF). The Virgo project involves the participation of about 130 institutions with more than 800 scientists, engineers and technicians from France, Italy, the Netherlands and other 13 European countries.

EGO welcomes applications from all suitably-qualified candidates, irrespective of gender, disability, marital or parental status, racial, ethnic or social origin, color, religion, belief, or sexual orientation.

Selection procedure

Only candidates who meet the above essential required qualifications and experience are admitted to the selection procedure. The evaluation of the candidates admitted to the procedure is assigned to a Selection Board appointed by the Director of EGO. The Selection Board will determine the evaluation criteria in the first meeting. The first phase of the selection will be based on a review of the Application Forms and other documents received in line with the above-mentioned essential and desired requirements. Only candidates who have obtained the minimum score established by the Selection Board in the first meeting will be able to access to the second phase of the selection, which will consist of an interview. During the interview the Selection Board will verify the knowledge of the English language, and the other desired qualifications and experience.

At the end of the interviews the Selection Board will draw up a ranking of the candidates who obtained at least the minimum score established during the first meeting.

The completion of the hiring is subject to Italian law D.Lgs. 81/08 art.41 “Sorveglianza Sanitaria”.

The EGO Consortium has the free right not to proceed with the recruitment.

Application Procedure:

Candidates have to send their CV and the EGO Application Form (to be found here) together with a cover letter and eventual reference letters, to jobs(at)ego-gw.it quoting the reference number of this vacancy notice.

Please find here details.

Positions at EGO

EGO is opening new positions. Application deadlines from June 25th to July 8th. Available job opportunities: 1) Software Developer, 2) Mechanical Designer, 3) Quality Assurance / Quality Control Engineer, 4) Control Physicist, 5) Integration Physicist, 6) Optics Physicist.

Find here details

LIGO Laboratory Job Opening: Senior Vacuum Engineer at LHO (CEBEX)

Caltech’s Laser Interferometer Gravitational-wave Observatory (LIGO) seeks a highly motivated and skilled Senior Vacuum Engineer to join its Cosmic Explorer Beamtube Experiment (CEBEX) team at the Richland, Washington observatory site. LIGO Laboratory is a major National Science Foundation facility dedicated to observing the newly discovered gravitational-wave universe. Jointly operated by the California Institute of Technology and the Massachusetts Institute of Technology, LIGO operates the world’s leading gravitational observatories near Richland, WA and Baton Rouge, LA, as well as campus R&D centers in Pasadena, CA and Cambridge, MA.

To learn more about LIGO Laboratory, please visit LIGO.caltech.edu. The Laboratory’s mission supports the young science of gravitational-wave physics and astronomy and includes observatory operations, analysis and dissemination of astrophysical observations, detector science and technology R&D, gravitational-wave astrophysics, and education and public outreach.

LIGO now also leads the effort to expand humanity’s gravitational wave horizon with a next-generation observatory, Cosmic Explorer (CE). Slated for construction in the 2030’s, CE will be ten times the size and reach of LIGO, able to gather signals from the edge of the observable universe.

The selected applicant will join an elite team charged with conceiving, designing, building, and testing advanced technology for the CE vacuum systems, destined to be the largest ultrahigh vacuum systems ever built. We will exercise and develop this technology in a new, purpose-built UHV research facility, the Cosmic Explorer Beamtube Experiment (CEBEX) Laboratory, located at LIGO Hanford.

Current Washington and Louisiana LIGO installations occupy 4 km scale, 10 million-liter UHV systems operating at one trillionth of atmospheric pressure (10-9 millibar), making them the two largest contiguous UHV volumes ever constructed. To further expand sensitivity, a new observatory will be constructed: Cosmic Explorer (CE). This observatory will require beamtubes 10x longer, up to 40 km in length. This will multiply CE’s detectable source range by ten, increasing the accessible volume of space thousandfold. However, UHV structures of this size and volume have never been attempted.

As a key member of the Cosmic Explorer Beamtube Experiment (CEBEX) team, the selectee will contribute to the modeling, trade study, design, fabrication, installation, bakeout and characterization of engineering prototypes and technology demonstrators for CE beamtubes up to 40 km in length. Tests will include industrial fabrication and qualification of a planned 1.2-meter diameter, 120-meter-long demonstration tube, to be erected in the new purpose-built CEBEX laboratory at the LIGO Hanford Observatory (LHO). In parallel, the chosen candidate will take a lead role in forging results of these investigations into a conceptual reference design, construction plan, and parametric cost estimate for CE. These will form the core of our future CE Observatory construction proposal.

This is a Campus Critical position. An employee designated as campus critical is expected to be aware of the campus emergency management plan and to report to Campus as soon as possible in the event of an emergency to assist in campus wide response and recovery efforts.

Essential Job Duties

  • Collaborate with research scientists and engineers in modeling and investigation of UHV techniques, welding and fabrication technology, structural statics and dynamics, thermal processing, surface preparation, residual gas characterization, material surface analysis, and related disciplines.
  • Establish, track, and maintain team workplans, schedules and budgets to accomplish mission objectives.
  • Supervise and mentor junior engineering and technical staff.
  • Plan and oversee specification and procurement of instruments and equipment, including budget development, scheduling, technical requirement definition, competitive vendor selection, contract monitoring, and quality assurance.
  • Responsible for professional communication (written and verbal) internally within the organization and externally to parties outside the organization. This includes liaising and interacting with US and international collaborators, contributors, and industrial partners.
  • Liaising, collaborating, and exchanging information with LIGO Laboratory vacuum teams concerning best practices, organization standards and methods.
  • Serve as a contributing member or chair on Design, Technical, Installation and other internal Review panels as may be required.
  • Initiate and collaborate in writing and delivering research papers and technical presentations.
  • Develop, oversee, and evaluate UHV material preparation and test facilities, including cleaning plants, bake ovens, and outgassing test chambers used to prepare or characterize UHV components and instrumentation.
  • Travel as requested to other LIGO campus and observatory sites, major vendor facilities, and collaborating institutions, both domestic and international.
  • Undertake additional leadership or contributing responsibilities as needs of the program may require.
  • Other duties as assigned.

Basic Qualifications

  • BS degree in Mechanical, Aerospace, Chemical or Systems Engineering, Physics, Material Science, or a related scientific or engineering field.
  • 8 or more years of direct vacuum engineering or research work experience in relevant industrial or scientific applications.
  • Demonstrated proficiency in practical design, analysis, and performance characterization of high- or ultra-high vacuum systems, including structural and safety analysis, pressure measurement, pump and valve selection, surface preparation, bakeout, and seal technology.
  • Thorough knowledge and experience in selection and application of UHV-compatible materials, material processes (welding, surface preparation, etc.)
  • Demonstrated proficiency in application and interpretation of spectra from residual gas analyzers.
  • Experience in application of helium mass‐spectrometer leak detection (MSLD) apparatus.
  • Effective English‐language written and verbal communication skills and habits.
  • Proven ability to mentor junior engineering and technical staff.
  • Level-headed professionalism and excellent interpersonal and team skills.
  • An automobile driver’s license valid in the United States, or ability to obtain one once employment begins.
  • Ability to lift at least 20 pounds.

Preferred Qualifications

  • Master’s or Doctoral graduate degree in Mechanical, Aerospace, Chemical or Systems Engineering, Physics, Material Science, or a related scientific or engineering field.
  • Certificate, coursework, or other professional qualification in Project Management.
  • Demonstrated expertise in application of industrial automation to large-scale vacuum systems.
  • Hands-on experience in building, improving, and maintaining high- or ultra- high vacuum systems.
  • Experience related to fluid, cryogen, pressure, flow rate, and gas sensors and instrumentation.
  • Computer-aided design (CAD) experience and demonstrated proficiency (SolidWorks™ preferred).
  • Finite-element analysis (FEA) experience and demonstrated proficiency (e.g., Ansys™, COMSOL™ or equivalent).
  • Gas dynamical modeling expertise (e.g., using MOLFLOW™ or equivalent Monte Carlo codes).

Required Documents

  • Cover Letter summarizing your relevant experience to this role and also your interest in LIGO Lab.
  • Resume.

Please find here full details.

Senior Vacuum Engineer at LHO

Caltech’s Laser Interferometer Gravitational-wave Observatory (LIGO) seeks a highly motivated and skilled Senior Vacuum Engineer to join its Cosmic Explorer Beamtube Experiment (CEBEX) team at the Richland, Washington observatory site.

LIGO Laboratory is a major National Science Foundation facility dedicated to observing the newly discovered gravitational-wave universe. Jointly operated by the California Institute of Technology and the Massachusetts Institute of Technology, LIGO operates the world’s leading gravitational observatories near Richland, WA and Baton Rouge, LA, as well as campus R&D centers in Pasadena, CA and Cambridge, MA.

This position is a fulltime in-person role located at LIGO Hanford in Richland, WA.

To learn more about LIGO Laboratory, please visit LIGO.caltech.edu. The Laboratory’s mission supports the young science of gravitational-wave physics and astronomy and includes observatory operations, analysis and dissemination of astrophysical observations, detector science and technology R&D, gravitational-wave astrophysics, and education and public outreach.

LIGO now also leads the effort to expand humanity’s gravitational wave horizon with a next-generation observatory, Cosmic Explorer (CE). Slated for construction in the 2030’s, CE will be ten times the size and reach of LIGO, able to gather signals from the edge of the observable universe.

The selected applicant will join an elite team charged with conceiving, designing, building, and testing advanced technology for the CE vacuum systems, destined to be the largest ultrahigh vacuum systems ever built. We will exercise and develop this technology in a new, purpose-built UHV research facility, the Cosmic Explorer Beamtube Experiment (CEBEX) Laboratory, located at LIGO Hanford.

Current Washington and Louisiana LIGO installations occupy 4 km scale, 10 million-liter UHV systems operating at one trillionth of atmospheric pressure (10-9 millibar), making them the two largest contiguous UHV volumes ever constructed. To further expand sensitivity, a new observatory will be constructed: Cosmic Explorer (CE). This observatory will require beamtubes 10x longer, up to 40 km in length. This will multiply CE’s detectable source range by ten, increasing the accessible volume of space thousandfold. However, UHV structures of this size and volume have never been attempted.

As a key member of the Cosmic Explorer Beamtube Experiment (CEBEX) team, the selectee will contribute to the modeling, trade study, design, fabrication, installation, bakeout and characterization of engineering prototypes and technology demonstrators for CE beamtubes up to 40 km in length. Tests will include industrial fabrication and qualification of a planned 1.2-meter diameter, 120-meter-long demonstration tube, to be erected in the new purpose-built CEBEX laboratory at the LIGO Hanford Observatory (LHO). In parallel, the chosen candidate will take a lead role in forging results of these investigations into a conceptual reference design, construction plan, and parametric cost estimate for CE. These will form the core of our future CE Observatory construction proposal.

This is a Campus Critical position. An employee designated as campus critical is expected to be aware of the campus emergency management plan and to report to Campus as soon as possible in the event of an emergency to assist in campus wide response and recovery efforts.

Essential Job Duties

  • Collaborate with research scientists and engineers in modeling and investigation of UHV techniques, welding and fabrication technology, structural statics and dynamics, thermal processing, surface preparation, residual gas characterization, material surface analysis, and related disciplines.
  • Establish, track, and maintain team workplans, schedules and budgets to accomplish mission objectives.
  • Supervise and mentor junior engineering and technical staff.
  • Plan and oversee specification and procurement of instruments and equipment, including budget development, scheduling, technical requirement definition, competitive vendor selection, contract monitoring, and quality assurance.
  • Responsible for professional communication (written and verbal) internally within the organization and externally to parties outside the organization. This includes liaising and interacting with US and international collaborators, contributors, and industrial partners.
  • Liaising, collaborating, and exchanging information with LIGO Laboratory vacuum teams concerning best practices, organization standards and methods.
  • Serve as a contributing member or chair on Design, Technical, Installation and other internal Review panels as may be required.
  • Initiate and collaborate in writing and delivering research papers and technical presentations.
  • Develop, oversee, and evaluate UHV material preparation and test facilities, including cleaning plants, bake ovens, and outgassing test chambers used to prepare or characterize UHV components and instrumentation.
  • Travel as requested to other LIGO campus and observatory sites, major vendor facilities, and collaborating institutions, both domestic and international.
  • Undertake additional leadership or contributing responsibilities as needs of the program may require.

Basic Qualifications

  • BS degree in Mechanical, Aerospace, Chemical or Systems Engineering, Physics, Material Science, or a related scientific or engineering field.
  • 8 or more years of direct vacuum engineering or research work experience in relevant industrial or scientific applications.
  • Demonstrated proficiency in practical design, analysis, and performance characterization of high- or ultra-high vacuum systems, including structural and safety analysis, pressure measurement, pump and valve selection, surface preparation, bakeout, and seal technology.
  • Thorough knowledge and experience in selection and application of UHV-compatible materials, material processes (welding, surface preparation, etc.)
  • Demonstrated proficiency in application and interpretation of spectra from residual gas analyzers.
  • Experience in application of helium mass‐spectrometer leak detection (MSLD) apparatus.
  • Effective English‐language written and verbal communication skills and habits.
  • Proven ability to mentor junior engineering and technical staff.
  • Level-headed professionalism and excellent interpersonal and team skills.
  • An automobile driver’s license valid in the United States.
  • Ability to lift at least 20 pounds.

Preferred Qualifications

  • Master’s or Doctoral graduate degree in Mechanical, Aerospace, Chemical or Systems Engineering, Physics, Material Science, or a related scientific or engineering field.
  • Certificate, coursework, or other professional qualification in Project Management.
  • Demonstrated expertise in application of industrial automation to large-scale vacuum systems.
  • Hands-on experience in building, improving, and maintaining high- or ultra- high vacuum systems.
  • Experience related to fluid, cryogen, pressure, flow rate, and gas sensors and instrumentation.
  • Computer-aided design (CAD) experience and demonstrated proficiency (SolidWorks™ preferred).
  • Finite-element analysis (FEA) experience and demonstrated proficiency (e.g., Ansys™, COMSOL™ or equivalent).
  • Gas dynamical modeling expertise (e.g., using MOLFLOW™ or equivalent Monte Carlo codes).

Required Documents

  • Cover Letter summarizing your relevant experience to this role and also your interest in LIGO Lab.
  • Resume.

Pease find here full details.

Three ET positions at RWTH Aachen

The successful candidates will be employed under a regular employment contract. The positions are to be filled at the earliest possible date and offered for a fixed term of two years. If the Einstein Telescope in the NL-B-D border region is approved, RWTH will attempt to continue the contract. The fixed-term employment is possible as it constitutes one of the fixed-term options of the Wissenschaftszeitvertragsgesetz (German Act on Fixed-term Scientific Contracts). This is a full-time position. The salary is based on the German public service salary scale (TV-L). The position corresponds to a pay grade of EG 13 TV-L. Application time: 18.07.2024

Please find here full details: