What are six different methods to measure distances in Astronomy? What are six different methods to measure distances in Astronomy in regards of their respective range in terms of astronomical objects?

So far I can name 4: Parallax method, radar ranging, main-sequence fitting, cepheid variables.
Using type Ia supernova light curves.

The RR Lyrae period-luminosity relation.

Moving cluster statistical parallax.

Surface brightness fluctuations.

Redshift-distance relation.

Using merging gravitational wave sources as standard sirens.

These and more can be pursued following this link. https://en.m.wikipedia.org/wiki/Cosmic_distance_ladder