This work highlights the power of coronal line emission to find black holes (BH) in dwarf galaxies missed by other selection techniques and to probe the BH popu

This work highlights the power of coronal line emission to find black holes (BH) in dwarf galaxies missed by other selection techniques and to probe the BH population in bluer, lower-mass dwarf galaxies. This is one of the papers that the article could be based off of [1]. [1] https://iopscience.iop.org/article/10.3847/1538-4357/ac1ffa https://iopscience.iop.org/article/10.3847/1538-4357/ac1ffa