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tokens: ACKNOWLEDGEMENTS This paper is based on observations collected with the MPG 2.2 m telescope, with the Danish 1.54 m telescope and with the Zeiss 1.23 m telescope. The first two telescopes are both located at the ESO Observatory in La Silla, Chile, while the latter is at the Centro Astronómico Hispano Alemán (CAHA) in Calar Alto, Spain. Operation of the MPG 2.2 m telescope is jointly performed by the Max Planck Gesellschaft and the European Southern Observatory. Operation of the Danish 1.54 m telescope in 2015 was financed by a grant to UGJ from the Danish Natural Science Research Council (FNU). Operations at the Calar Alto telescopes are jointly performed by the Max Planck Institute for Astronomy (MPIA) and the Instituto de Astrofísica de Andalucía (CSIC). GROND was built by the high-energy group of MPE in collaboration with the LSW Tautenburg and ESO, and is operated as a PI-instrument at the MPG 2.2 m telescope. The reduced light curves presented in this work will be made available at the CDS ( http://cdsweb.u-strasbg.fr/ ). LM acknowledges support from the Italian Minister of Instruction, University and Research (MIUR) through FFABR 2017 fund. LM acknowledges support from the University of Rome Tor Vergata through ‘Mission: Sustainability 2016’ fund. GC acknowledges the support by the National Natural Science Foundation of China (Grant No. 11503088, 11573073, 11573075) and the project ‘Technology of Space Telescope Detecting Exoplanet and Life’ from National Defense Science and Engineering Bureau civil spaceflight advanced research project (D030201). IJ acknowledges the Austrian Forschungsförderungsgesellschaft FFG project ‘RASEN’ P847963. TCH acknowledges financial support from KASI. DMB acknowledges the support of the NYU Abu Dhabi Research Enhancement Fund under grant RE124. MK acknowledges the support of the International Postdoctoral Fellow of Independent Research Fund Denmark. CITEUC is funded by National Funds through FCT – Foundation for Science and Technology (project: UID/ Multi/00611/2013) and FEDER – European Regional Development Fund through COMPETE 2020 – Operational Programme Competitiveness and Internationalisation (project: POCI-01-0145-FEDER-006922). We thank Fei Yan for useful discussion about the WASP-74 b transmission spectrum. The following internet-based resources were used in research for this paper: the ESO Digitized Sky Survey; the NASA Astrophysics Data System; the SIMBAD data base operated at CDS, Strasbourg, France; and the arXiv scientific paper preprint service operated by Cornell University. Based on data collected by MiNDSTEp with the Danish 1.54 m telescope at the ESO La Silla Observatory.