The Solar Orbiter Heliospheric Imager (SoloHI), developed and operated by the U.S. Naval Research Laboratory (NRL), is one of the six remote sensing instruments on board the Solar Orbiter Mission and observes the photospheric visible light scattered by electrons in the solar wind. This catalog is based on the SoloHI observations with a multi-viewpoint perspective. For each event detected by SoloHI, we present available in-situ data and remote sensing observations detected by other solar missions that help to understand the trajectory and evolution of it. When possible, we identify the source of th e CME and describe the main characteristics of it. We also track the CME throughout the different coronagraph and heliospheric imagers available. Additionally, we present a set of plots when the event is detected in-situ by the different missions. Finally, we complement the observations with the event described and modeled by the Space Weather Database Of Notifications, Knowledge, Information (DONKI) developed at the Community Coordinated Modeling Center (CCMC).