4MOST - 4-metre Multi-Object Spectroscopic Telescope
4-m Multi-Object Spectroscopic Telescope


Science Team Meeting 2024


The University Hall of Uppsala University.

The next 4MOST Science Team Meeting is now open for registration. It will take place in Uppsala on 12-16 February 2024. Participants can follow the sessions online or in person. Please see http://4mmosst.wikidot.com/science-team-meeting-february-2024 for more details.

The science that 4MOST will enable is at the core of this meeting. We therefore invite all participants (online and in-person) to submit suggestions for contributed talks, including title and abstract, using a Google form. These should not be the usual survey-presentation talks, but rather focus on a specific science question that 4MOST data will help address, and can be connected to ongoing research projects with other surveys and instruments. There is also a possibility to submit general suggestions for the meeting agenda using the same Google form. Your input will help us develop the programme, so we kindly request that abstracts/feedback are sent before 8 January.

Congratulations to Kate Maguire


Kate Maguire

The 4MOST Project congratulates Kate Maguire from Trinity College Dublin for being awarded an ERC Consolidator Grant, CosmicLeap, to explore the deaths of white dwarfs, mapping the full diversity of ways in which these bodies explode. This will be crucial for defining new precision samples for cosmology, as well as determining the rates and contributions of white dwarf explosions to the origin of the elements.

"One of the key aims of the project is to obtain rapid spectroscopy of the largest sample of white-dwarf transients to date," explains Kate. "The first days after explosion are when the signatures of their diversity is greatest and these spectra will be crucial for distinguishing between explosion scenarios. I'm excited to work closely with the 4MOST team and members of the S10 Time Domain Extragalactic Survey (TiDES) to achieve my research aims."

Kate obtained her PhD from Queen's University Belfast before taking up a post-doctoral research position at the University of Oxford. She held Marie Skłodowska-Curie and ESO fellowships at the European Southern Observatory headquarters in Munich from 2013-2015 and an Ernest Rutherford Fellowship at Queen's University Belfast from 2015-2019. She is currently an Associate Professor at Trinity College Dublin.

Congratulations to Ása Skúladóttir


Ása Skúladóttir

The 4MOST Project congratulates Ása Skúladóttir from the University of Florence for being awarded an ERC Starting Grant for her research project studying the origin of the Milky Way and its chemical elements. Ása is the Survey PI of 4DWARFS (4MOST survey of dwarf galaxies and their stellar streams) and this ERC Starting Grant will enable her to build a strong team to analyse the 4MOST data of her Survey.

"Like all larger galaxies, the present Milky Way was formed through a sequence of mergers of smaller dwarf galaxies over its lifetime," explains Ása. "Around our galaxy there are now dozens of known dwarf galaxies as well as 'stellar streams' – streams of stars that we think are associated with old dwarf galaxies that were destroyed during their interaction with the Milky Way."

Ása's ERC project, 'TREASURES', will combine data from Gaia and from the 4DWARFS Survey to study individual stars of various ages, thereby tracking the evolution of the Milky Way and its chemical enrichment throughout cosmic time. "The data," Ása further explains, "will also provide an opportunity to investigate the hierarchical formation of the Milky Way and provide the most complete overview of the evolution of dwarf galaxies, reconstructing their histories: from formation to disintegration."

Ása Skúladóttir is from Iceland. After obtaining her PhD in Astronomy in 2016 at the Kapteyn Institute of the University of Groningen, she worked as a post-doc at the Max Planck Institute for astronomy (MPIA) in Heidelberg, Germany, from 2016-2019. She then joined the University of Florence, first as a post-doc, and since early 2021 as RTD-A (equivalent to an Assistant Professor).

Long Fibre Feed installation at CTS and connection to AESOP


The 4MOST Fibre System, deployed at the Cassegrain Test Stand (CTS) at AIP. On the ground is the fibre strain relief assembly and the three transport cases for the slit assemblies. The elevation chain connects to the CTS structure and the fibre route continues inside the cable rotator.

The 4MOST System Integration is proceeding nicely according to plan. On 19 July 2023, the final optical fibre relay with all the science and auxiliary fibres (aka, the Long Fiber Feed or LFF) was connected to the Fibre Positioner AESOP. This is an important milestone on the path towards full system integration in Potsdam. Please see the attached photos courtesy of Andreas Kelz (AIP).

"After the Fibre-Feed system has been built and assembled, it successfully passed Local Acceptance Review in May 2023," said LFF Workpackage Manager, Andreas Kelz. "Subsequently, the fibre system was folded, packed and transported across the AIP campus to the main integration hall, where it has been integrated into the Cassegrain Cable Wrap and mounted onto the Cassegrain Test Stand. The fibre elevation chain and strain relief units are mounted in the same positions as on VISTA. Finally, all 181 fibre connectors have been plugged to the backside of the AESOP positioner."

All fibre connectors (i.e., the 168 for science fibres, 12 guide cables and 1 fiducial connector) are plugged to the backside of the AESOP positioner. Also, all service cables and cooling lines (three o'clock) are connected to AESOP and the limit switches.

Unique view of the 4MOST focal plane


Amazing view of the 4MOST focal plane as seen through the Wide Field Corrector. You can access here a high-resolution version of the image.
Courtesy of Michael Schroeck (AIP)

This photo was taken in the AIP Integration hall on 19 July 2023. It shows an amazing view of the 4MOST focal plane as seen through the Wide Field Corrector (WFC) from the perspective of the telescope’s secondary mirror. The hexagonal pattern of bright dots in the centre shows the area of the AESOP spines. Just outside the spines, visible as bright squares,  one can recognise the six technical CCDs (guiders and wavefront sensors) through their pickup prisms. The bright rings are the fiducials used by the 4MOST metrology system to precisely measure the position of the spines. One can also spot the baffles inside the WFC as faint concentric rings outside the focal plane.  

This is a rare occasion to enjoy such a view. It further demonstrates that 4MOST is complete and ready for verification in the AIP Integration hall!

Statement on TRR


On July 3 and 4, the 4MOST Test Readiness Review (TRR) was held in Potsdam between ESO and the 4MOST Project Office. This review is an official major project milestone that manifests the transition from the system integration phase to the system verification phase. In broad strokes, the scope of the TRR is to verify that the hardware is available and working, and that documentation is complete before launching formal verification.

Not unexpectedly, the weeks leading up to the TRR were extremely busy. The effort that was put in by the 4MOST team was nothing short of amazing. Hardware was installed and tested, minor hardware issues were corrected, formal action items were addressed, documentation was updated and released. The sum of all these activities brought 4MOST a huge step forward towards completion.

On the second day of the TRR review, the ESO chair of the 4MOST PAE process summarized the findings and recommendations. Without going into too much detail, ESO was very impressed by the status of the HW in the integration hall. On subsystem level, the readiness was found to be adequate. There were however parts of the system level documentation that needs update and more detail to allow for an efficient execution of the verification activities. The PAE chair believed that the project will benefit from developing these documents further before proceeding with verification, and the decision was to postpone the TRR.

What is happening now is that some already scheduled verification activities will nevertheless proceed as planned. In parallel, the Project Office has made some internal priority changes with the goal of finishing the missing documentation as soon as possible. This includes a re-planning effort that will require some time to sort out before we can provide a new project schedule. We hope that we are able to finish this activity and present an updated project schedule in the next coming weeks. The PO believes that the overall delay triggered by the postponed TRR milestone will be quite moderate. Stay tuned!

Revised Code of Conduct


At the recommendation of the Project Culture Working group, a few changes to the 4MOST Code of Conduct (CoC) were implemented by including the word "caste" in the example lists on discrimination and equity of opportunity and treatment. This new version has been endorsed by the 4MOST Executive Board, the Science Coordination Board and by ESO's Director for Science.

Every member of member of 4MOST is expected to know the 4MOST CoC and hence also this change, effective immediately. The new CoC is on DocuShare and on the web site.

Special issue of the Messenger


Cover of ESO Messenger 190

The March 2023 issue of the Messenger (190) is a special edition, dedicated to the 4MOST Community Surveys. This complements the presentation of the 4MOST consortium's ten survey proposals in issue 175 of The Messenger.

In the issue, available here, each of the 15 Community Surveys is presented in a three-page article. A necessary reading for everyone interested in 4MOST!

Seeking second IWG6 lead


The 4MOST Project seeks a second lead for IWG6 (Data Curation and Quality Control) with scientific background in Galactic astronomy to work together with the current lead on developing the 4MOST Quality Control pipeline (4QP) and coordinating the activities of Infrastructure Working Group 6 "Data Quality Control".

Job summary: The main responsibility of IWG6 is to ensure that appropriate quality control procedures are in place where needed in the many interfaces of the 4MOST data flow.

QC happens at several levels:

  1. All the data processing and analysis pipelines should make sure that any data products have been submitted to quality control before being transmitted ahead in the data flow. IWG6 conducts active discussions with the appropriate work packages to ensure this is the case.
  2. IWG6 runs its own QC pipeline (after the L1 and L2 pipelines) and adds QC parameters to the data flow as needed.
  3. IWG6 will visually examine the data and conduct trending analysis to catch any QC issues not uncovered by the previous two activities. In time, it is expected that such additional QC checks lead to improvements in the pipelines and in the QC pipeline.

The two leads of IWG6 work together to ensure that these tasks are addressed. They work with all members of IWG6, staffed from the different surveys. Time commitment is around 20%, likely to increase to 50% in the first year of operations.

Main tasks:

  • advise IWG1 on measures to QC the input survey catalogues
  • collaborate with OpSys in putting QC measures in place for OBs
  • work together with DMS to define appropriate QC measures and procedures to check L1 data
  • develop and maintain 4QP, which checks the L2 data
  • work with the 4MOST archive teams to ensure proper data curation ahead of data releases
  • coordinate efforts of IWG6, from distributing the (mock) data to collating any identified issues, communicating them to source nodes, and advising on solutions.

Selection criteria:

  • background in Galactic astronomy
  • experience with data reduction and analysis of spectra
  • experience with python programming
  • good communication skills
  • collaborative and inclusive mindset

Applications are reviewed by a selection panel that contains at least the 4MOST Operations Manager and the current IWG6 co-leads and is chaired by the 4MOST PI.

Beside the competence, motivation and availability of candidates, the selection committee will also pay attention to gender and diversity balance and implications for early career scientists. We encourage all interested individuals, especially from underrepresented minorities, to apply.

Performing the IWG6 co-lead responsibilities will normally allow one to qualify for a permanent 4MOST Science Team membership.

Please see the 4MOST wiki for information on how to apply.

Introducing the new leader of the Communication and Education WG


Henri Boffin

The 4MOST Principal Investigator, Roelof de Jong, is very pleased to announce Henri Boffin as our new lead for the Communication and Education Working Group (formerly called Outreach WG). Henri is a Full Astronomer at ESO, working on binary stars, exoplanets, and clusters. Within the 4MOST Project, he is a member of the Survey 4SYS (S12).

Next to having a PhD in astronomy, Henri has a formal training as journalist from the École supérieure de journalisme de Lille, France. He joined ESO in 2003 as Astronomer and Press Officer, dealing with communication about all telescopes and projects of ESO, and became the Deputy Head of the ESO Public Affairs Department. There he dealt with all aspects of communication: writing press releases; communicating with journalists, the public, and politicians; being the technical editor of the Messenger; taking care of the web site; and producing press kits, exhibitions, and education material.

Henri is looking forward to working with all 4MOST members and the institutional Communication groups to develop an encompassing science communication strategy for the Project with the aim to develop the internal newsletter, develop the web site for astronomers, journalists, and the public, and its associated blog, write press releases and interact with journalists, develop educational material, and ensure a social media presence, among others.

Executing such an ambitious programme requires a large team and we are in the process of creating a new Science Communication and Education WG. We expect to issue a call for membership of this new WG in the next few weeks for all those 4MOST members with a keen interest in the area of science communication and education. Please consider joining Henri in this important effort.