This work has been carried out within the framework of the NCCR PlanetS supported by the Swiss National Science Foundation under grants 51NF40_182901 and 51NF40_205606. RA acknowledges the Swiss National Science Foundation (SNSF) support under the Post-Doc Mobility grant P500PT_222212 and the support of the Institut Trottier de Recherche sur les Exoplanetes (IREx). RA, JPW, EA, FBa, BB, NJC, RD, LMa & CC acknowledge the financial support of the FRQ-NT through the Centre de recherche en astrophysique du Quebec as well as the support from the Trottier Family Foundation and the Trottier Institute for Research on Exoplanets. ML, HC & BA acknowledge support of the Swiss National Science Foundation under grant number PCEFP2_194576. DE and MS acknowledge support from the Swiss National Science Foundation for project 200021_200726. VV, SP, DE, &MS acknowledge the financial support of the SNSF. NN, JIGH, RR, ASM & AKS acknowledge financial support from the Spanish Ministry of Science, Innovation and Universities (MICIU) projects PID2020-117493GB-I00 and PID2023-149982NB-I00. NN acknowledges financial support by Light Bridges S.L, Las Palmas de Gran Canaria. NN acknowledges funding from Light Bridges for the Doctoral Thesis "Habitable Earth-like planets with ESPRESSO and NIRPS", in cooperation with the Instituto de Astrofisica de Canarias, and the use of Indefeasible Computer Rights (ICR) being commissioned at the ASTRO POC project in the Island of Tenerife, Canary Islands (Spain). The ICR-ASTRONOMY used for his research was provided by Light Bridges in cooperation with Hewlett Packard Enterprise (HPE). XDu acknowledges the support from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement SCORE No. 851555) and from the Swiss National Science Foundation under the grant SPECTRE (No 200021_215200). This work was supported by grants from eSSENCE (grant number eSSENCE@LU 9:3), the Swedish National Research Council (project number 2023 05307), The Crafoord foundation and the Royal Physiographic Society of Lund, through The Fund of the Walter Gyllenberg Foundation. EA, FBa, RD & LMa acknowledges support from Canada Foundation for Innovation (CFI) program, the Universite de Montreal and Universite Laval, the Canada Economic Development (CED) program and the Ministere of Economy, Innovation and Energy (MEIE). SCB, ED-M, NCS & ARCS acknowledge the support from FCT - Fundacao para a Ciencia e a Tecnologia through national funds by these grants: UIDB/04434/2020, UIDP/04434/2020. SCB acknowledges the support from Fundacao para a Ciencia e Tecnologia (FCT) in the form of a work contract through the Scientific Employment Incentive program with reference 2023.06687.CEECIND and DOI 10.54499/2023.06687.CEECIND/CP2839/CT0002. XB, XDe and TF acknowledge funding from the French ANR under contract number ANR24-CE493397 (ORVET), and the French National Research Agency in the framework of the Investissements d'Avenir program (ANR-15-IDEX-02), through the funding of the "Origin of Life" project of the Grenoble-Alpes University. The Board of Observational and Instrumental Astronomy (NAOS) at the Federal University of Rio Grande do Norte's research activities are supported by continuous grants from the Brazilian funding agency CNPq. This study was partially funded by the Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior - Brasil (CAPES) - Finance Code 001 and the CAPES-Print program. BLCM acknowledge CAPES postdoctoral fellowships. BLCM acknowledges CNPq research fellowships (Grant No. 305804/2022-7). NBC acknowledges support from an NSERC Discovery Grant, a Canada Research Chair, and an Arthur B. McDonald Fellowship, and thanks the Trottier Space Institute for its financial support and dynamic intellectual environment. JRM acknowledges CNPq research fellowships (Grant No. 308928/2019-9). ED-M further acknowledges the support from FCT through Stimulus FCT contract 2021.01294.CEECIND. ED-M acknowledges the support by the Ramon y Cajal contract RyC2022-035854-I funded by MICIU/AEI/10.13039/501100011033 and by ESF+. ICL acknowledges CNPq research fellowships (Grant No. 313103/2022-4). CMo acknowledges the funding from the Swiss National Science Foundation under grant 200021_204847 "PlanetsInTime". Co-funded by the European Union (ERC, FIERCE, 101052347). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. GAW is supported by a Discovery Grant from the Natural Sciences and Engineering Research Council (NSERC) of Canada.