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I will present two new techniques in indirect detection of dark matter. I will first talk about the technique of velocity spectroscopy. I will show that the measurement of energy shifts induced by relative motion of source and observer can separate signal and background with minimal theoretical uncertainty and can act as a new signature of dark matter. In the second part of my talk, I will discuss a new method to search for axion-like particles (ALPs) based on the gamma-rays produced concomitant with high-energy astrophysical neutrinos. I will show that searching for these gamma-rays will probe new parts of the parameter space of axion-like particles.