The work took advantage of the huge 3-D galaxy map called Mega Z. Because there are so many neutrinos , their tiny masses add up to influence the overall distribution of galaxies .
这项研究利用了MegaZ这个巨大的三维星图。原因在于,星系中有众多的中微子,而当这些微不足道的质量加在一起时,其总和就会影响整个星系的分布。