A generalization of this self-calibration method could also help us in the future to cross-calibrate amid distinctive surveys that have different selection capabilities and as a result different biases—and stars in various evolutionary states—within their described stellar abundances. which might be quickly seen in the APOGEE DR16 abundances appreciably lessen https://billionairebrainwaverevie50481.blogstival.com/54741787/the-stellar-abundance-can-be-fun-for-anyone