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Fast Machine Learning for Science Conference 2024, October 15-18 at Purdue University

The first three days will be workshop-style with invited and contributed talks. The last day will be dedicated to technical demonstrations and satellite meetings. The event will be hybrid with an in-person, on-site venue and the possibility to join virtually.  For those attending in person, there will be a social reception during the evening of Tuesday, October 15, and a dinner on Thursday, 17th.

As advances in experimental methods create growing datasets and higher resolution and more complex measurements, machine learning (ML) is rapidly becoming the major tool to analyze complex datasets over many different disciplines. Following the rapid rise of ML through deep learning algorithms, the investigation of processing technologies and strategies to accelerate deep learning and inference is well underway. We envision this will enable a revolution in experimental design and data processing as a part of the scientific method to accelerate discovery greatly. This workshop is aimed at current and emerging methods and scientific applications for deep learning and inference acceleration, including novel methods of efficient ML algorithm design, ultrafast on-detector inference and real-time systems, acceleration as-a-service, hardware platforms, coprocessor technologies, distributed learning, and hyper-parameter optimization.

Abstract submission deadline: September 16th, 2024
Registration deadline: October 1st,2024

Organising Committee:

  • Mia Liu (Chair)
  • Maria Dadarlat (Co-chair)
  • Andy Jung
  • Norbert Neumeister
  • Wei Xie
  • Paul Duffel
  • Haitong Li
  • Guang Ling
  • Eugenio Culurciello
  • Yong Chen
  • Alexandra Boltasseva
  • Laimei Nie

Scientific Committee:

  • Thea Aarrestad (ETH Zurich)
  • Javier Duarte (UCSD)
  • Phil Harris (MIT
  • Burt Holzman (Fermilab)
  • Scott Hauck (U. Washington)
  • Shih-Chieh Hsu (U. Washington)
  • Sergo Jindariani (Fermilab)
  • Mia Liu (Purdue University)
  • Allison McCarn Deiana (Southern Methodist University)
  • Mark Neubauer (U. Illinois Urbana-Champaign)
  • Jennifer Ngadiuba (Fermilab)
  • Maurizio Pierini (CERN)
  • Sioni Summers (CERN)
  • Alex Tapper (Imperial College)
  • Nhan Tran (Fermilab)
  • Verena Martinez Outschoorn (UMass Amherst)

Workshop Website

Upcoming Job Opportunities at ESA

Pre-announcements of job opportunities at ESA: the actual openings are always very short (3 weeks) so  people can mentally prepare for those positions before they come out. One of them is the Research Fellowship. The other two are not LISA related but might interest some of you, nevertheless.
  1. Fellowships, the jobs application portal should open for submissions on 26 August with applications due 16 September.
  2. Science Education Scientist & Communications Coordinator — the ESA jobs application portal should open by ~1 September, with applications due 3 weeks later. Detailed description below.
  3. Project Scientist in Astronomy & RF Coordinator — the ESA jobs application portal should open mid-September with applications due 3 weeks later. Detailed description at end of text.

Early Career Opportunities at ESA

Calls open to nationals of ESA member & cooperating states only

Student internships (3-6 months)

  • applications due ~Oct
  • master students (penultimate/final year)

National trainee programme (1+1 year)

  • timelines determined by national agencies
  • master students (final year/recent graduates) from Belgium, Estonia, Germany, Ireland, Luxembourg, Portugal & Switzerland

Young graduate programme (1 year)

  • applications due ~Jan/Feb for start in Sep
  • master students (final year/recent graduates)

ESA co-funded research for PhD students & postdocs (1-1.5 years)

  • applications accepted throughout the year

ESA Research Fellowships for postdocs

ESA Science Research Fellowship

What?

  • independent postdoctoral fellowship for ESA State nationals
  • research project covering any topic in space science
  • 2 + 1 years (proposal for 3rd year extension)

Where?

  • ESTEC (Netherlands), ESAC (Spain) or STScI (USA)

Why?

  • 100% research time (optionally <20% functional work, e.g. archive/data
  • science, citizen science, operations, calibration, communication)
  • insights into ESA environment & activities
  • mentoring from senior ESA Science Faculty members
  • training available (e.g. spacecraft design, soft skills, management)
  • 3500-4600€ net monthly salary (depending on location & experience)
  • comprehensive health Coverage

contact: fellowship(at)cosmos.esa.int
Website: https://www.cosmos.esa.int/web/space-science-faculty/opportunities/research-fellowships


Science Education Scientist & Communications Coordinator

We are pleased to announce an exciting upcoming opportunity at ESA Directorate of Science for an experienced science communicator & educator, to be at the forefront of bringing space into education and inspire future generations into STEAM. Get in touch if you have questions!
This is a pre-announcement for a Science Education Scientist and Communication Coordinator. This opportunity is open to ESA Member State nationals and will be based in Spain (European Space Astronomy Centre).

The European Space Agency maintains a world-leading Science Programme with missions in heliophysics, planetary science, astrophysics and fundamental physics. Its mission is to ‘Empower Europe to lead space science’.
The Science Communication and Education Section (SCI-EC) in the Office of Science Engagement and Oversight (SCI-E) is responsible for defining and implementing the Communication and Education Strategy for the Science Directorate of the European Space Agency. It leverages the technological advances and scientific output enabled by the Space Science missions with the aim to inform, engage and inspire a range of stakeholders (ranging from advisory bodies, media, scientists, general public and future generations).
In this role you will be responsible for coordinating and managing the CESAR education initiative – a joint initiative by ESA, the Instituto Nacional de Técnica Aeroespacial (INTA) and the Ingeniería de Sistemas para la Defensa de España, S.A. (ISDEFE) – to promote and develop educational activities in Spain, Europe and beyond. In particular, you will be in charge of the definition, execution, monitoring and evaluation of education activities, getting to work in a dynamic team of science educators and communicators.
In addition, for up to 50% of your time, you will support the Head of the Science Communication and Education section in planning and implementing the optimal use of resources dedicated to communication and education, including placing contracts, defining and preparing clear procedures to ensure the smooth functioning and integration of our science communication and education activities.
Relevant technical competencies: experience in space science, experience in science communication and education, experience in project management. An advanced knowledge of Spanish and experience in international communications would be an asset.


Project Scientist in Astronomy & Research Fellows Coordinator

The European Space Agency maintains a world-leading Science Programme with missions in heliophysics, planetary science, astrophysics and fundamental physics. Its mission is to ‘Empower Europe to lead space science’. The Office of Science Engagement and Oversight (SCI-E) oversees the scientific content of the Science programme and providing scientific expertise to Science missions, across all phases, from studies to operations and beyond. The Office also manages scientific research, scientific community engagement activities as well as the communication and education efforts for the ESA Directorate of Science.

In this role, the Project Scientist will update and implement policies for guest proposal submission and peer review to ensure a rigorous, transparent, fair and consistent approach across missions. They will also be responsible for strengthening the Space Science Research Fellowship Programme.

This job is particularly well suited to a scientist with a good understanding of and experience in inclusive practices in astronomy and astrophysics communities (and beyond), and an interest in the evolution of these practices to ensure ESA Science missions remain at the forefront of best practice, in particular, regarding Open Science.
Relevant technical competencies: active researcher in a relevant field of space science, knowledge of latest developments in Open Science and/or Peer Review, knowledge and experience in scientific space missions and payloads. Experience in coordinating the scientific community and managing multiple interfaces at international levels and experience in pro

ESA: LISA Science Team selected

ESA has announced the members of its LISA Science Team (LST): 18 scientists were elected and appointed for the first term from 2024 to 2027. The role of the LST is to provide scientific advice during the development and operations of the LISA mission. The LST is co-chaired by the ESA and NASA Project Scientists and will support the ESA Project and Operations teams on all aspects related to the science return of the mission.

Find the LST here: https://www.cosmos.esa.int/web/lisa/lisa-science-team

LISA Data Generation and Analysis Workshop, Oktober 7-10 2024, Online

The LISA Consortium’s Simulation and LDC Groups are happy to invite you to the LISA Data Generation and Analysis Workshop, which will take place online October 7-10 2024. It is aimed at beginners to LISA data analysis (with hands-on getting-started sessions), as well as more expert individuals who want to learn more (with in-depth sessions on simulation and analysis of sources of various types).

Hands-on tutorial sessions on how to generate simulated datasets (similar to LDC datasets) and run parameter estimation on them. It will include 101-level sessions, as well as more in-depth sessions. The end-goal is to work towards including multiple types of sources in the mini-global fit pipeline.

The workshop will cover 4 sessions (European afternoons, North-American mornings), including

A 4-hour “getting started” hands-on tutorial, where we will generate of a simple LDC-like dataset with realistic instrumental noise and one MBHB signal, then run an MCMC on it to recover the source parameters. A 3-hour “in-depth simulation” hands-on tutorial, where the parametrization of the instrumental noise and various effects (such as nonstationary noise and data artifcats) will be demonstrated, as well as realistic time-domain EMRI, Galactic binary ensemble, and SGWB signals. Two 3-hour “in-depth analysis” hands-on tutorials, where a mini-global fit will be constructed, including inference for a Galactic binary population, MHBHs, and instrument noise.

This workshop is open to all. However, some tools might have restricted access to LISA Consortium associated or full members.

The workshop is organized by the junior chairs of the LISA Consortium Simulation Expert Group and the LISA Data Challenge Working Group. Many thanks to the speakers, who agreed to help with the organization of the tutorials, and in particular:

  • Jean-Baptiste Bayle (University of Glasgow)
  • Quentin Baghi (APC)
  • Eleonora Castelli (NASA GSFC)
  • Natalia Korsakova (APC)
  • Christian Chapman-Bird (University of Glasgow)
  • Henri Inchauspé (Universität Heidelberg)
  • Martin Staab (Observatoire de Paris)
  • Maude Le Jeune (APC)
  • Michael Katz (NASA Marshall)
  • Nikolaos Karnesis (AUTh)
  • Olaf Hartwig (AEI Hannover)
  • Senwen Deng (APC)
  • Sylvain Marsat (L2I Toulouse)

Workshop Website

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.

New Frontiers in NR 2025 – July 21-25 2025 at University of Balearic Islands

In the history of numerical (or computational) general relativity, the “Frontiers” meeting in 1988 at the University of Illinois, Urbana-Champaign (USA), played a pivotal role in establishing numerical relativity as a major topic in computational physics and simulation science. The “New Frontiers” meeting in 2006 at the AEI Potsdam convened following major breakthroughs in numerical simulations of binary systems. The most recent “Frontiers 2022” conference was instrumental in assessing the state-of-the-art and identifying future directions in numerical relativity. The upcoming “New Frontiers 2025: past, current and future challenges in Numerical Relativity” will emphasize the significant theoretical and computational challenges ahead, not only in understanding the observations of gravitational waves and electromagnetic counterparts but also in comprehending the nature of gravity at a more fundamental level. Reflecting on past adversities and how our community overcame them may guide us in current and future endeavors. 

Main topics:

  • Mathematical foundations
  • Numerical methods for the Einstein and the radiation MHD equations
  • High performance computing
  • Astrophysics (binary mergers, gravitational waves, electromagnetic counterparts,…)
  • Beyond current astrophysics and general relativity

The meeting will take place at the University of the Balearic Islands starting on July 21st and ending on July 25th, 2025. There is no registration fee.

Scientific Organizing Committee:

  • M.Bezares (University of Nottingham)
  • C.Bona (Universitat de les Illes Balears)
  • B.Bruegmann (University of Jena)
  • K.Clough (Queen Mary University of London)
  • J.A.Font (Universitat de València)
  • S.Husa (ICE-CSIC)
  • L.Lehner (Perimeter Institute)
  • C.Palenzuela (Universitat de les Illes Balears)
  • M.Shibata (Max Planck Institute for Gravitational Physics)

Conference Website

NEOSGrav2024, October 1-4, Goa, India

The international conference on Neutron star Equation of State and Gravitational Waves (NEOSGrav2024) shall take place in Goa, India during 01 - 04 October 2024. It is being organized by the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune.

The scientific programme shall consist of invited review talks and some short oral presentations.

The following areas in the neutron star physics will be covered in the meeting:

  • Fundamental Physics from Neutron stars
  • Constraining Neutron Star EoS with Electromagnetic observations
  • Constraining Neutron Star EoS with Gravitational waves
  • Numerical modelling of Neutron Stars

In addition to the science sessions, there will be two public talks during the week at the Birla Institute of Technology and Science, Pilani – Goa Campus and Goa Science Centre

Venue: All the scientific sessions shall be held at the Kenilworth Hotel, Goa.
Date: October 01 – 04, 2024

Scientific Organizing Committee:

Debarati Chatterjee (Chair) — IUCAA, Pune, India Prof. Dipankar Bhattacharya — Ashoka University, India Prof. Sukanta Bose — Washington State University, USA Prayush Kumar — ICTS, Bengaluru, India

Local Organizing Committee:

Debarati Chatterjee (IUCAA) M. S. Sahasrabudhe (IUCAA) S. Samuel (IUCAA) Yogesh Thakare (IUCAA) Kinjal Banerjee (BITS Pilani, Goa) Tarun Kumar Jha (BITS Pilani, Goa) Reshma Raut Dessai (Goa University) Ananthraman S.V. (Ashoka University)

IUCAA Advisory Committee:

Durgesh Tripathi — IUCAA, Pune, India Ranjeev Mishra — IUCAA, Pune, India

For any queries: Please write email to – neosgrav2024(at)iucaa.in

Conference Website

GRASS Trento, September 30th – October 2nd 2024

The GRAvitational - wave Science&technology Symposia (GRASS) are a series of meetings held in Padova and Trento and aimed at exploring the panorama of gravitational-wave related experimental science beyond the next decade; special emphasis is given to open issues and key enabling technologies at the forefront of the most advanced detection techniques. It represents an informal and unique meeting occasion for experts from different fields involved in experimental aspects of future gravitational-wave science and technology.

The GRASS 2024 edition will include topical sessions on Gravitational Waves and Multi-messenger Observational Science, Coatings and Materials, Perspectives for the Reduction of Quantum Noise and Stray Light mitigation for future GW detectors. A general session to discuss any other open issue is foreseen as well.

Attendance to the conference will be in person only. No video streaming of the conference is forseen at this time.

Meeting Website

Challenges and future perspectives in gravitational- wave astronomy: O4 and beyond, October 14-18, Leiden, NL

This workshop will foster an interdisciplinary discussion about how ongoing and future observations of gravitational and electromagnetic waves can be used to shed light on the physics of compact-object formation and evolution.

We will bring together experts on:

  • (i) parameter estimation from gravitational-wave data;
  • (ii) astrophysical modeling of gravitational-wave sources and their electromagnetic counterparts; and
  • (iii) gravitational-wave “data mining”.

This meeting will bring together astronomers and gravitational-wave scientists whose current research covers these three topics. The key questions we aim to address in the meeting are:

  • how can gravitational-wave parameter estimation be integrated with other forms of astronomy to gain a more comprehensive understanding of compact-object mergers?
  • How can gravitational-wave data help us understand the astrophysical processes and environments involved?
  • What improvements are required for stellar/binary evolution models, cluster dynamics, and galactic nuclei for a meaningful comparison to the data?
  • How can we use modern statistical tools to maximize the astrophysical information extracted from the gravitational-wave data?

This workshop accepts applicants! Application dadline: 21st of July 2024.

Workshop Website