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

News

Top-level schedule update

An announcement from the Project Manager, Joar Brynnel:

I would like to communicate a schedule adjustment for the 4MOST project. At its meeting on 23 September 2021 the 4MOST Executive Board (EXB) was presented with a new top-level milestone schedule. After some discussion, the new schedule was acknowledged by the EXB. In summary, we are forced to delay both the Preliminary Acceptance Europe (PAE) and Preliminary Acceptance Chile (PAC) milestones by 6+1 months. Six months of delay come from various delays at subsystem level. The additional one month delay is caused by having to re-integrate the fibre positioner AESOP at the AIP with only remote help from the AAO engineers who cannot travel to Potsdam due to the Australian Corona-related travel restrictions. PAE is therefore now scheduled for May 2023, while PAC is now scheduled for March 2024.

Consortium members can download the updated top-level schedule from DocuShare.

4MOST All Hands Meeting 2021

The 4MOST Consortium came together on 13 – 17 September 2021 for the seventh installment of the annual All Hands Meeting (AHM). Again, as in 2020, this AHM was originally planned to be held at ESO in Garching, but the continuing Corona pandemic forced the event to be held entirely online once more, using a combination of zoom (see above) and gather.town (see below). With 147 registered participants from across the Consortium, the meeting was very well attended. The meeting’s programme can be found here and all presentations are available on DocuShare.

Below we have collected some impressions from various corners of the project.

Here are some thoughts from Jenny Sorce, a very active member of the Cosmology Redshift Survey (S8): “With the meeting being entirely online again, I found that gather.town permitted interactions with one (a few) person(s) at a time in a very convenient way. It was very easy to switch from a session to a “private” conversation in an instant and to find the people I needed to talk to.”

“The programme was very well set up. I particularly enjoyed the two plenary summary sessions that permitted catching up with the sessions I was not able to attend. Otherwise I mostly attended IWG and extragalactic survey sessions. I must say that contrary to the main sessions, there was no (clear) agenda for most of these sessions. Perhaps it would have been useful to have one in order to be better prepared for the discussions and to stay focused (at least that was my impression). I also really appreciated the afternoon on Project Culture and Values for 4MOST. It was also a special meeting in the sense that some PIs of prospective Community Surveys attended, and it was great to meet some of them. Finally, I was glad to hear that after 2 years of CoViD-19, 4MOST is still reasonably on track. All in all, this meeting was a success and I got all the information I needed to conduct my main tasks for the next year.”

The Project Office System Engineer, Olga Bellido Tirado, commented: “Despite of the regular videoconferences I have with our partners, the AHM is an annual event I really look forward to. It is certainly an intense week that requires preparation but, from my point of view, the effort is worthwhile. It’s an exceptional moment of exchange of knowledge and experiences in all the project areas. Concerning the facility side of the project, learning about the progress of the individual subsystems in their manufacturing and testing phase has been really exciting. In this second virtual AHM, I think that the use of gather.town has been a great success. It has made all the interaction during the coffee breaks much more enjoyable; giving us back the nice and missed feeling of meeting and chatting with colleagues in the corridor.”

David Murphy, a key developer of the Data Management System (DMS) had this to say: “I confess I let out a small groan when I discovered this year’s meeting would be held predominantly on gather.town. I’d had a mixed experience with it at last year’s AHM, and didn’t think it would work very well. Turns out I was completely wrong! An inspired decision by the LOC that really helped to stimulate group discussions and even socialising.”

“I was encouraged by how much the project had moved on, despite all the challenges of the past year. From the Operations perspective, we’ve managed to start analysing engineering data to get a real feel for how the instrumentation will perform. We are now in the process of establishing a dedicated 4MOST Processing Centre for handling all the data that will be generated. A lot of discussions centred around how this will work for various contributors, including the rapidly-developing Public Archive and the target classifier under IWG9. There’s still lots for us to do, but I left the meeting full of enthusiasm for the coming year.”

“It was only during the final “group photo” on gather.town (see below) that I discovered how to make my avatar “dance” – if we are indeed able to meet in-person next year, I promise that’s something I won’t replicate in-person!”

Finally, the Project Manager, Joar Brynnel, reflected: “Personally, I have learned a lot during the week, and I am very pleased to note that no unexpected or surprising issues have surfaced. I liked the format of the meeting, and as far as online meetings go I don’t think it gets much better than this. An event like this requires good preparation and tight organization. The LOC has done a great job with the preparation and running of the meeting and I would be remiss if I didn’t mention the individuals involved: Roelof, Silke, Christine, Diana and Jakob, many thanks for your competent and wonderful support!”

“I am truly looking forward to the AHM 2022, which in the best of worlds will be held as a traditional face-to-face meeting. At that time, we will hopefully be able to present real results from real hardware in the AIP integration hall!”

Final 4MOST Wide Field Corrector lens delivered

The Project Manager, Joar Brynnel, is very happy to report that on 2021-07-15 the large lens “L1” for the 4MOST Wide Field Corrector (WFC) arrived safely at the UCL laboratory. Being the largest (900 mm diameter) and most expensive optical element in 4MOST, this is the final WFC lens to arrive in London.

The raw material (so-called “blank”) for this lens was procured from a US vendor in 2017, and then shipped to an optics manufacturer in New Zealand. Here the lens was machined, and in August 2018 it was shipped to a specialist in the US for the so-called aspherisation. This is a difficult manufacturing step that only very few suppliers worldwide are capable of, especially for a lens of this size. For various reasons, the aspherisation took much longer than anticipated, and the lens was returned to New Zealand only in November 2020. Here, the lens was thoroughly tested and found to be in spec. In December 2020, the lens started its next overseas journey, this time to a coating facility in the US. The optical coating was completed and accepted in July 2021, and the lens was then shipped to London where it is now safely stored and waiting to be integrated into the WFC. We are relieved to finally see this beautiful lens finished and having survived the long journeys across the planet!

The L1 lens in its shipping box during its incoming inspection at UCL.

4MOST Cassegrain Cable Wrap arrives in Potsdam

The Project Manager, Joar Brynnel, reports that on 2021-06-16 the 4MOST Cassegrain Cable Wrap (CaCW) was delivered to the AIP in Potsdam. The unit was transported from the manufacturer Kinkele in Bavaria on an over-wide transport truck. After unloading and unpacking in the 4MOST integration hall, the CaCW (white structure in the photos below) was mounted in its orange handling frame. Everything went smooth and without incidents.


4MOST Cassegrain Cable Wrap Factory Acceptance

The production of hardware for 4MOST is in full swing. One of the major electro-mechanical systems in production is the 4MOST Cassegrain Cable Wrap (CaCW). This system is required to de-rotate not only electrical, network, and cooling supplies to the fiber positioner AESOP, but also all optical fibers connecting AESOP to the three spectrographs. On the telescope, we have to rotate AESOP to track the stars on sky, and we need a way to safely manage all these connections to the Azimuth platform. The way we do this is through an electrically driven de-rotator. The detailed design, analysis, parts machining and assembly was contracted to the company Kinkele in the north of Bavaria. After completion, staff from the AIP spent three weeks on site at Kinkele to inspect and verify the CaCW. The campaign was successful and concluded with a punch list of issues to resolve before shipping to the AIP, which is scheduled for the first half of June 2021.

Allar Saviauk, CaCW lead engineer: “I was happy to see the CaCW structure finally in front of us after so many years of development and hard work. This system took several design revisions and tweaks before we were confident submitting it for manufacturing. We showed up at the manufacture’s plant with our long test plan, and over a two and a half week period we were able to check all the dimensions, welds, load testing and of course the functionality itself. The first time we rotated the fully loaded system with chains was quite exiting! Fortunately, the CaCW works as intended and we were able to rotate this Stargate-like system by +/-200 deg in various telescope pointing angles. Some optimization is still required in the fibre cable configuration inside the energy chain. Our fibre team is currently working on a solution. The company is also re-manufacturing one of the welded assemblies to improve the dimensional fit to other components. In general I’m very pleased about the results and want to thank everybody involved with this system over the years: A. Kelz, J. Brynnel, S. Bauer, T. Jahn, L. Wagner, J. Paschke, R. Haynes, T. Liebner (AIP), M. Lehmitz (MPIA), and A. Jost (ESO).”

The CaCW in its handling frame hanging from the crane hook during flipping to vertical position.

The CaCW fully integrated in horizontal position during dimensional verification.

Close-up of the cable chain (black part) and the chain separator (structure with yellow wheels).

The CaCW in its handling frame parked in two large “feet”. The CaCW control electronics provided by MPIA and ESO can be seen at the lower left.

First LRS spectra

The first 4MOST Low-Resolution Spectrograph (LRS-A) has now reached “first light” (or first spectra) in the CRAL integration hall in Lyon, France. These first exposures were taken through the blue channel. The most important parameters – image quality, wavelength range and spectral resolution – are all very close to those necessary to meet our goal of doing world class astrophysical research. The LRS opto-mechanical design preforms well, giving us confidence that similar performance will be achieved when assembling the green and red channels of LRS-A, and the second LRS.

Florence Laurent, the head of engineering at CRAL: “I am happy to say that the first arm of LRS-A has been integrated and aligned and we succeeded in making the first exposures. Most importantly, the blue channel already performs close to its scientific and technical specifications. I would like to express my sincerest thanks to the team, Karen Disseau, Jean-Emmanuel Migniau, Didier Boudon, Diane Chapuis, Eric Daguisé, Aurélien Jarno, Arlette Pécontal, Johan Richard, and Alban Remillieux, all of whom overcame many challenges to reach this milestone.”

Matthew Lehnert, the director of CRAL, added: “It’s wonderful to see these results and imagine the exciting scientific results and breakthroughs we will be capable of making with this extremely capable instrument. Without the hard work of the dedicated team at CRAL, imagining these goals would not even be possible. Thank you to everyone for their hard work!”

The blue arm of the LRS-A bench which enabled the first LRS “lab light”.

Exposure of a continuum lamp showing the spectrum across the blue detector (370 – 554 nm). Only six groups of fibres across the slit are illuminated for these tests.

Zoom-in on a few spectral lines of a Mercury lamp, demonstrating the overall image quality of the blue channel. With further work on the alignment and other optimizations, we are confident of being able to reach even better performance.

4MOST proposals submitted to ESO

On 15 December 2020 the 4MOST consortium and the ESO community successfully submitted their proposals for ESO Public Surveys to be carried out with 4MOST during its first five years of operations. While the consortium submitted 10 proposals for its guaranteed time (corresponding to the 10 Consortium Surveys), the community submitted 18 proposals to compete for the “open” time available to the community.

The proposal submission marks the culmination of many months of preparation. The community proposals were invited by ESO following a pre-selection based on Letters of Intent previously submitted by the community in February 2020. While honing their own proposals over the past months, the 4MOST Science Team also supported their colleagues in the ESO community to get ready and plan for the exciting scientific opportunities offered by 4MOST, e.g. by organising two workshops. The proposal submission thus represents yet another major milestone for the 4MOST project and the Principal Investigator, Roelof de Jong, would like to thank everyone involved for their hard work and strong commitment.

ESO’s Public Survey Panel (PSP) will now review all proposals received and judge the community proposals in terms of their complementarity and possible synergies with the Consortium Surveys before recommending the final, joint 4MOST Survey Programme.

4MOST first spectra

The 4MOST High-Resolution Spectrograph (HRS) has now reached “first light” (or first spectra) in the Landessternwarte (Heidelberg) lab for the green channel with an engineering grade detector. This is not only a major and exciting milestone for the project in general, but it also means that for the first time we have real HRS data to work with after many years of working with simulated data. It is also a validation of many aspects of the 4MOST opto-mechanical design, which allows the project to move forward with the remaining MAIT activities with increased confidence.

Walter Seifert (HRS Lead Engineer) reports: “The basic alignment of the channel with regard to wavelength range, image quality and spectral resolution has been performed in two days without any issues. Further iterations on optimising the performance will be done with the actual science detector in place. Nevertheless, the spots are already in or close to specification. Apart from flatfield and spectral arc exposures using the lab calibration unit, we also took a spectrum of the sun by holding an auxiliary fibre out of the window towards the sky.”

Roelof de Jong (4MOST PI) commented: “I am very excited to see these first spectra from the High-Resolution Spectrograph. It is wonderful to see that within a few days of effort the team is already meeting most specifications. This gives great credit to the many excellent people involved from across the consortium: the HRS team of course, but also the detector and control hardware teams, the fibre team, and now the data management system team. I want to thank them all for their dedicated efforts.”

 HRS spots

Left: HRS spectrum of a ThAr lamp. The full wavelength range of the green channel (516 – 573 nm) is shown for a few central fibres. Right: image quality test using the ThAr spectra. Shown are 100 × 100 px at the four corners of the detector as well as some intermediate points.

HRS solar spectrum. The full wavelength range of the green channel (516 – 573 nm) is shown for a few central fibres.

4MOST Wide Field Corrector optics delivered

The 4MOST Wide Field Corrector (WFC) and Atmospheric Dispersion Corrector lenses have been manufactured and tested at KiwiStar Optics, New Zealand. These are large lenses that represent a significant part of the overall hardware budget for 4MOST. The Project Manager, Joar Brynnel, is pleased to report that five of the six WFC lenses have just arrived safely at the UCL laboratory, where they will be integrated with the WFC mechanics and aligned with high precision in order to meet their tight specifications. The sixth lens is still at KiwiStar in the final stage of manufacturing. It is a great relief for the project that the lenses have arrived without damage. Peter Doel (UCL) reports: “The crates have arrived safely and are under lock and key in the lab. No external shock indicators were triggered and there was no visual damage of the boxes. We very briefly (and without taking them out of the boxes) did a visual inspection of the lenses before resealing them. The lenses look fine.”

This picture shows the lens “L3” in its transport box during incoming inspection at UCL.

Changes to Survey leadership

The science programme of 4MOST is driven by its individual Surveys, each pursuing different science cases. Currently, there are ten such Surveys to fill the Guaranteed Time Observations of the Consortium, each under the leadership of one or more Survey Principal Investigators (PIs). After 10 years of serving as Survey co-PI of the Milky Way Halo Low-Resolution Survey (S1), Prof. Amina Helmi has unfortunately decided to resign from this position. The 4MOST Project is very grateful for her leadership since the start of the project and for bringing the Survey to its current excellent state together with her S1 co-PI Prof. Mike Irwin. Amina is looking forward to seeing data arrive in a few years’ time and will remain involved in the further development and exploitation of the Survey. We wish Amina all the best for her other endeavours and the responsibilities she has taken on.

Fortunately, Amina’s resignation will not leave a vacancy. The Project is extremely pleased that the 4MOST Executive Board has approved the nomination of Prof. Else Starkenburg as the new co-PI of the Milky Way Halo Low-Resolution Survey at its meeting on 15 October 2020. This is expected to be a fairly smooth leadership transition, as Else already served as one of the co-PIs of S3, the Milky Way Disc and Bulge Low-Resolution Survey (4MIDABLE-LR), in the past, and is hence already familiar with the required background. While Else will remain active within 4MIDABLE-LR, its leadership is now in the hands of the remaining S3 Co-PIs Dr. Cristina Chiappini and Dr. Ivan Minchev.

The Project would like to thank everyone involved in this transition for the excellent leadership provided so far, and is looking forward to the continued collaboration toward the final development of the survey programme, science operations and data exploitation.