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LIGO/Virgo Collaboration has published 11 detections from the first two observational campaigns (O1/O2) and results from first half of the third campaign (O3) are also already available. I will first discuss the landscape of O1/O2 detections and their implications for stellar evolutionary modeling. Broadly speaking the basic observational properties of detected double black hole mergers are consistent with predictions of the classical isolated binary evolution of massive stars. These early detections constrain some aspects stellar physics that is unaccessible by electromagnetic observations. On the other hand, the first results from O3 campaign seem to challenge classical binary evolution with black holes found in lower and upper mass gaps. These are regions in which black holes are not expected to form from stars, but rather form via dynamic interactions of stars in dense clusters. I will discuss these curious events in context of their most likely formation sites.