On 10 – 11 July 2019 the Project Office visited CRAL in Lyon to meet with the Low Resolution Spectrograph (LRS) team for the project-internal Mid-Term Review (MTR). This was the fifth MTR with more to follow. The purpose of this review is to assess the status of the work package – schedule, finances, product assurance, MAIT, interfaces, technical performance, and compliance matrix – approximately half-way between the Final Design Review and the Local Acceptance Review. The review panel (Brynnel, Giannone, Bellido, Frey, and Johl) concluded that the work package is in general performing very well, and no major issues were identified. During the mandatory lab visit, the review panel could see the two LRS optical tables assembled and integration and verification of the mounts for the optics in progress. ESO has already delivered the cryo-vacuum system and MPIA has delivered the control electronics. AIP will deliver three science-grade detectors in late July. The delivery of optics from various vendors remains on the critical path for the MAIT of the two LRSs. CRAL is actively monitoring these deliveries, and in spite of some delays the dates for the Local Acceptance Reviews of LRS-A and LRS-B were confirmed.
The Project Office would like to warmly thank the CRAL team for the excellent preparation of the LAR and for hosting us during the review.
Participants of the LRS Mid-Term Review (from left to right): Arlette Pecontal, Diana Johl, Domenico Giannone, Olga Bellido, Karen Disseau, Diane Chapuis, Johan Richard, Joar Brynnel, Florence Laurent, Alban Remillieux, Eric Daguise, Aurelien Jarno.
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Between 2019-06-21 and 2019-07-01, the 4MOST project visited the Paranal Observatory. The overall purpose of this mission was to verify the VISTA telescope interfaces, to hone the AIV plan, and to discuss technical issues with the relevant Paranal staff. The mission was quite successful, and all the items on the list could be checked off. The team, consisting of Jeff, Marco and Christophe from ESO, Michael from MPIA, and Steffen, Allar, and Joar from the AIP were able to witness the removal of the VISTA primary and secondary mirrors for re-coating. To this end the telescope top end plus VIRCAM with its cable de-rotator had to be removed, which allowed us to access all relevant interfaces and to make laser tracker measurements. In addition, the HRS and LRS interfaces were inspected and surveyed. We were able to present 4MOST and discuss the project with several Paranal staff members. Special thanks to Jeff and Christophe for their great support before and during the visit!
In front of the VISTA telescope, from left to right: Allar Saviauk, Joar Brynnel, Steffen Frey (all AIP), Michael Lehmitz (MPIA), Jeff Pirard, Christophe Dupuy, and Marco Quattri (all ESO). In the background to the right you can see the VLT.
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On 9 May 2019 the Local Acceptance Review (LAR) for the 4MOST Detector Systems was held at ESO in Garching. The LAR is the final official milestone for facility subsystems, where the hardware is formally accepted, compliance with requirements and (not the least) documentation is reviewed between the 4MOST Project Office and the delivering partner, in this case ESO. The 4MOST Detector subsystem encompasses not only the 9 science-grade CCDs in their dewars, but also readout electronics and the complete cryo-vacuum system. A spare science-grade CCD and two engineering-grade CCDs are also part of the deliverables.
The performance of the CCDs is excellent, exceeding requirements in almost all areas, and the delivery schedule is very well aligned with the rest of the project. During the LAR, Joar Brynnel stated on behalf of the 4MOST project that this has been a very successful collaboration, not only from a technical/performance perspective, but it has also been carried out in a very productive and collaborative spirit.
Jeff Pirard (ESO) added: “The LAR also gave the opportunity to warmly thank Jean-Louis Lizon, Gero Rupprecht and Roland Reiss, all three retiring in 2019. They have strongly contributed to the success of the 4MOST Detector System development. The Detector System LAR is a first step of 4MOST subsystem completion which shall open the path for system integration at AIP in the coming months. The project is moving forward. Science data are getting closer!”
Participants of the LAR (from left to right): Patrick Caillier (ESO Product Assurance Manager), Domenico Giannone (4MOST Product Assurance Manager), Joar Brynnel (4MOST Project Manager), Isabella Cesarini (on screen, 4MOST Project Controller), Olga Bellido (on screen, 4MOST Systems Engineer), Josh Hopgood (ESO Detectors), Jean-Louis Lizon (ESO Cryo/vacuum), Gero Rupprecht (ESO Product Assurance Manager), Roland Reiss (ESO Detectors), Jeff Pirard (ESO Project Manager).
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On 6 – 8 May 2019, the workshop Preparing for 4MOST: A community workshop introducing ESO’s next-generation spectroscopic survey facility took place at ESO in Garching, Germany. It was organised jointly by ESO and the 4MOST Consortium to prepare the ESO community for the upcoming “Call for Letters of Intent for Public Spectroscopic Surveys with 4MOST” (currently planned for Q4 2019). This Call will represent the start of the process by which ESO will select the Community Surveys to be carried out in the 30% of the observing time of the first 5 years of operations that will be available to the community.
In a total of 17 presentations, the 4MOST Consortium provided the participants with up-to-date information on the 4MOST facility, its capabilities, survey strategy, data reduction and science pipelines, as well as the 4MOST Consortium’s scientific plans, while ESO described the application and selection process. The community, in turn, presented its ideas for Community Surveys in 16 talks, covering a wide range of scientific topics, from exoplanets, to stellar clusters, galaxy evolution, and AGN.
A number of question and discussion sessions provided the opportunity for participants to clarify any remaining issues, and to jointly discuss the connections between the scientific ideas presented by the community and the plans of the Consortium.
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Sam Barden reports that previous to the application of an anti-reflection coating an inspection and review of the five smaller (650 mm diameter) lenses of the Wide Field Corrector (WFC) was held last week at KiwiStar Optics. They are shown below. The purple colour is due to a protective layer of photo-resist applied to protect the lens surfaces. The clear lens (L4) was undergoing final measurements, so it is uncoated.
On the left is Malcolm Young (the project manager), next to him is Jin Zhang (mechanical engineer). To the right of Joar Brynnel is Abe (one of the optical techs), Graeme Jonas (optics expert), Dijana Bogunovic (Optical Engineer with the unenviable job of stitching the test data together), Sandra Ramsay (KSO upper management), and Dave Cochrane (technical leader) to the far right.
The L4 test data are still being reviewed, but the go-ahead to have all of the lenses shipped to Quantum Coating in the USA to receive their anti-reflecting coating is expected by the end of the week. The largest WFC lens, L1, is already in the USA for aspherisation. Due to the time it takes to do the aspherisation, L1 will actually be the last one to be coated, but all should be finished by the end of this year.
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A message from the Principal Investigator, Roelof de Jong:
The new extragalactic dPS: Luke Davies
The new Galactic dPS: Diane Feuillet
It gives me great pleasure to announce a few new appointments in the 4MOST organisation.
As announced a few months ago, it was decided that the 4MOST Project Scientists needed extra support for their many tasks in the form of deputy Project Scientists. The selection has now been completed and I am pleased to announce that the new Galactic deputy Project Scientist is Diane Feuillet and the extragalactic dPS is Luke Davies, effective immediately. The different roles and responsibilities of the PSs and dPSs will be worked out in more detail in the coming months, so stay tuned for more information.
The new Galactic IWG2 leader: Jesper Storm
The new extragalactic IWG2 leader: Peder Norberg
I am also announcing a transition in leadership of IWG2. As confirmed by the SCB, the new Galactic IWG2 lead will be Jesper Storm, while the new extragalactic lead will be Peder Norberg. This leadership transition will become effective after the CfPRR review at ESO, i.e., on 22 March 2019. I hereby want to thank Thomas Boller and Cristina Chiappini for their hard work and great dedication as IWG2 leads in the past years. You have made important contributions towards establishing the foundations of the 4MOST survey strategy.
Please be extra supportive towards the newly appointed people while they are ramping up to their new tasks!
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In early May 2018 the Final Design Review (FDR) for 4MOST was held. In this review, most of the system and subsystem design and analysis was presented and thoroughly reviewed by a panel of ESO and external experts. Following FDR, the subsystems that were reviewed entered the manufacturing and assembly (MAIT) phase. However, some of the subsystems were not ready for review at that point in time, and it was agreed between ESO and the 4MOST Project Office to schedule a second review dubbed FDR-2.
FDR-2 was held on 6-7 March 2019 at ESO in Garching. Participants included Project Office members, subsystem Work Package managers and engineers, Review Panel members from ESO, and invited external experts. The scope of the review was to review the final design of the Long Fiber Feed, Metrology, and Cooling subsystems, the Acquisition & Guiding MAIT, the Wide Field Corrector verification, as well as some system aspects, such as assembly, integration, test and verification, including the Focal Surface Test Tools (FSTT). The meeting was held in a very constructive, open and collaborative spirit, and the preliminary feedback from the panel was quite positive. In particular, for all the subsystems listed above, early feedback was very encouraging and preparations for entering the MAIT phase can now commence. The FSTT will be subject of a dedicated review meeting this summer.
This means that, with a few exceptions, the 4MOST facility is now in full production mode. The character of the project is changing quite substantially, which takes some time to get used to, but at the same time it is very motivating to see the facility hardware and software taking shape. To keep track of the rapid developments, the Project Office is now quite busy working with the partners through many Work Package Mid-Term Reviews and Lab Acceptance Reviews.
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The March 2019 issue of ESO’s The Messenger, published today, is dedicated entirely to 4MOST. It contains 13 articles, written by the 4MOST Consortium, which introduce 4MOST to the ESO community. Three overview articles describe the 4MOST project and instrument, the 4MOST science operations and its current survey plan, while another ten articles, one for each of the Consortium Surveys, describe the scientific plans of the 4MOST Consortium.
This special 4MOST issue of The Messenger was published in preparation of the joint ESO/4MOST workshop Preparing for 4MOST: A community workshop introducing ESO’s next-generation spectroscopic survey facility. This workshop, in turn, is meant to help the community prepare for a Call for Letters for Intent for Public Surveys with 4MOST, expected to be issued by ESO in mid-2019. The publication of the 4MOST Messenger issue thus marks the beginning of an exciting process, at the end of which a number of Community Surveys will join the Consortium Surveys to form the final 4MOST Survey Programme for the first 5 years of operations.
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Joar Brynnel reports that on 21 February 2019, 4MOST engineering staff from the Georg-August-Universität in Göttingen verified and accepted the support structures for the two low-resolution spectrographs (LRS) at the manufacturer Windelband. In the photo below you can see Heiko Anwand using a laser tracker to verify dimensions with high accuracy and Katja Hauptner holding the retro. The support structures will now be sent for painting. Two of the three supports will then be sent to CRAL for LRS integration activities, and the third structure will be sent to ESO Chile for interface verification on the VISTA telescope.
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The Project Office would like to introduce the new 4MOST Instrument Scientist, Genoveva Micheva, who has replaced Ollie Schnurr in the AIP/4MOST Project Office. Genoveva’s most recent position was in the InnoFSpec group at the AIP, and she joined the 4MOST team on 1 December 2018.
Genoveva earned her PhD in Astronomy at the Department of Astronomy, Stockholm University, Sweden. Her professional background is that of both an astronomer and an engineer. Her many years of experience in working at observatories (NOT, La Palma, and SUBARU, Hawaii) provide her with a good foundation for understanding the importance of being the interface between the instrument builder team and future users.
We would like to welcome Genoveva on board, and we are looking forward to working with her towards the completion of 4MOST!
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