The distance-measuring techniques, arranged in order of the distance for which they are MOST effective (from least to most) are
A) Cepheid variables, spectroscopic parallax, Type Ia supernovae, and Tully-Fisher relation.
B) spectroscopic parallax, Tully-Fisher relation, Cepheid variables, and Type Ia supernovae.
C) spectroscopic parallax, Cepheid variables, Tully-Fisher relation, and Type Ia supernovae.
D) Cepheid variables, spectroscopic variables, Type Ia supernovae, and Tully-Fisher relation.
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