A generalization of the self-calibration tactic could also help us in the future to cross-calibrate among diverse surveys that have various selection features and for this reason unique biases—and stars in different evolutionary states—within their claimed stellar abundances. In practise, not all these elements could be measured in stellar spectra https://billionairebrainwaverevie17092.bloguetechno.com/the-stellar-abundance-can-be-fun-for-anyone-67898984