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Progress Meeting no. 3 took place at LAM (Marseille) in december 2023

Progress Meeting no. 2 took place at ESO (Garching) in september 2023

 

Registration to the MOSAIC Science Working Groups

(*) : compulsory field/choice.

Please complete the form below to officially register for one or more MOSAIC science working groups.

Your registration will be carefully reviewed and processed by the MOSAIC science team, and it is the first step toward fostering a productive collaboration with us. Additionally, you will be included in our Science or Instrument mailing lists.

We eagerly anticipate the opportunity to collaborate with you !

Code of Conduct

Please read through the MOSAIC Code of Conduct first.
Please agree to the MOSAIC Code of Conduct

Privacy Policy

Please agree to the privacy policy

Registration form

Please describe in a few lines your research interests, expertise, and anticipated contribution to the project.
Please indicate the name or role of the person nominating you to join the Science Team
Please select both if you need to be included in both the Science and Technical mailing lists
Please select the working groups you want to be included in.

Artistic depiction of a supermassive black hole accreting material from a disk. Gaseous outflows from these SMBHs can heat and even expel the surrounding interstellar medium, thus halting any subsequent star formation in the galaxy. Credit: NASA/JPL-Caltech. Artistic depiction of a supermassive black hole accreting material from a disk. Gaseous outflows from these SMBHs can heat and even expel the surrounding interstellar medium, thus halting any subsequent star formation in the galaxy. Credit: NASA/JPL-Caltech.

Do not hesitate to contact us if you have any question or require further information.

MOSAIC Consortium

INSU - CNRS

Lead Technical Institute
3 rue Michel-Ange
75794 Paris Cedex 16
France
This email address is being protected from spambots. You need JavaScript enabled to view it.

 

 

 

 

Consortium

The workhorse instruments of the current 8-10m class observatories are multi-object spectrographs (MOS), providing comprehensive follow-up of ground-based and space-borne imaging data. With the advent of even deeper imaging surveys from, e.g., HST, VISTA, JWST and Euclid, many science cases require complementary spectroscopy with high sensitivity and good spatial resolution to identify the objects and to measure their astrophysical parameters. The light-gathering power of the 39m ELT and its spatial resolution, combined with a MOS, will enable the large samples necessary to tackle some of the key scientific drivers of the ELT project, ranging from studies of stellar populations out to the highest-redshift galaxies. Consequently, a MOS-facility is foreseen within the ELT instrumentation plan.

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