Revisiting the angular size--redshift cosmological test with milliarcsecond radio structures in active galactic nuclei
Mina Ghodsi Yengejeh·András Kovács·I. Leonid Gurvits·Sándor Frey·A. B. Pushkarev·A. V. Plavin·Kenneth I. Kellermann·Tatiana A. Koryukova
Very long baseline interferometry (VLBI) measurements of the sizes of compact extragalactic radio sources, jetted active galactic nuclei, provide data for probing the angular size--redshift relation, offering a classical cosmological test complementary to other distance--redshift methods. Aiming to update and extend previous studies conducted in the 1990s, we analyse a significantly expanded and improved dataset to reassess the angular size--redshift relation and its potential for constraining c
