Preparing for LSST Data: in Search of Main Physical Properties of the Main Sequence Galaxies

Gabriele Riccio (1) , Katarzyna Małek (2) , Ambra Nanni (2) , Médéric Boquien (3) , Véronique Buat (2) , Denis Burgarella (2) , Darko Donevski (4) , Mahmoud Hamed (1) , Peter Hurley (5) , Raphael Shirley (5) , Agnieszka Pollo (6)

1 National Centre for Nuclear Research [Otwock]
2 LAM - Laboratoire d'Astrophysique de Marseille
3 CITEVA - Centro de Astronomia [Antofagasta]
4 SISSA / ISAS - Scuola Internazionale Superiore di Studi Avanzati / International School for Advanced Studies
5 University of Sussex
6 UJ - Uniwersytet Jagielloński w Krakowie = Jagiellonian University

The main goal of the Vera C. Rubin observatory is to perform the 10 year Legacy Survey of Space and Time (LSST). This future state-of-art observatory will open the new window to study billions of galaxies from Local Universe as well as the high redshift objects. To get ready to work with the petabytes of data collected by the LSST we performed a simulation of future observations and uncertainties based on the 50,385 real galaxies within the redshift range 0

Domaines: Planète et Univers [physics]

Gabriele Riccio, Katarzyna Małek, Ambra Nanni, Médéric Boquien, Véronique Buat, et al.. Preparing for LSST Data: in Search of Main Physical Properties of the Main Sequence Galaxies. XL Polish Astronomical Society Meeting, held 13-17 Sept. 2021 at University of Szczecin, Poland. Proceedings of the Polish Astronomical Society, 2022, à renseigner, Unknown Region. pp.85-88. ⟨insu-03938271⟩