Measuring the H I mass function below the detection threshold

We present a Bayesian stacking technique to directly measure the H i mass function (HIMF) and its evolution with redshift using galaxies formally below the nominal detection threshold. We generate galaxy samples over several sky areas given an assumed HIMF described by a Schechter function and simul...

Полное описание

Библиографические подробности
Главные авторы: Pan, H, Jarvis, MJ, Allison, JR, Heywood, I, Santos, MG, Maddox, N, Frank, BS, Kang, X
Формат: Journal article
Язык:English
Опубликовано: Oxford University Press 2019