You can lead a theorist to data, but you can't make him think. - Stacy McGaugh

The current cosmological paradigm, the cold dark matter model with a cosmological constant, requires that the mass-energy of the Universe be dominated by invisible components: dark matter and dark energy. An alternative to these dark components is that the law of gravity be modified on the relevant scales. A test of these ideas is provided by the baryonic Tully-Fisher relation (BTFR), an empirical relation between the observed mass of a galaxy and its rotation velocity. Here, I report a test using gas rich galaxies for which both axes of the BTFR can be measured independently of the theories being tested and without the systematic uncertainty in stellar mass that affects the same test with star dominated spirals. The data fall precisely where predicted a priori by the modified Newtonian dynamics.

A long time ago when I first got interested in MOND, having come from the background where I believed in dark matter, I wrote a proposal saying, "Gee, this theory had its predictions come true, ... we should look into that" and it was rejected, you know, very harshly. And I thought "OK, the community is not willing to fund this kind of thing" — this was almost twenty years ago. And so I basically did a global substitute, replaced MOND with dark matter, resubmitted, and I got my money. ... Pavel is totally correct that scientists are focused on getting grants, because that's what you need to support your students, and your postdocs, and getting the data, and all those sort of things. And I would like to believe that that was an anecdote from the distant past, but I am aware of a colleague who had this experience very recently where this person did not even mention MOND in the proposal, but the panel came back saying "MOND is no good — you must not spend money on this." ... the panel had associated ... this person's name with having at some point written a paper about MOND and projected that onto this proposal that ... did not mention MOND. And so it really is that bad.

The concordance model of cosmology, ΛCDM, provides a satisfactory description of the evolution of the universe and the growth of large scale structure. Despite considerable effort, this model does not at present provide a satisfactory description of small scale structure and the dynamics of bound objects like individual galaxies. In contrast, MOND provides a unique and predictively successful description of galaxy dynamics, but is mute on the subject of cosmology. … it is far from obvious that the mass spectrum of galaxy clusters or the power spectrum of galaxies can be explained in MOND, two things that ΛCDM does well. Critical outstanding issues are the development of an acceptable relativistic parent theory for MOND, and the reality of the non-baryonic dark matter of ΛCDM. Do suitable dark matter particles exist, or are they a modern aether?