Photometry and Spectroscopy of Distant Galaxy Samples

对遥远射电星系样本的研究将继续进行。 的 主要研究目标是完成形态学， 光度学和光谱学的研究 第三次剑桥射电巡天（3CR）样本中的射电星系 并接近出色的完成水平， 1 Jansky通量射电源。 这些来源是6 - 10倍 比以前观测到的源弱，主要是星系。 大的红移范围覆盖到z的红移 约1.8。 对年轻星系的进一步探索， “几乎原始的”窄氢莱曼α线发射器， 也将包括大于1.5的红移z。 的推动 因为这项研究发现了类恒星物体 (QSO)伴星PKS 1614 + 051 B，红移z = 3.21，和3C3326.1， 一个可能正在形成的大星系，在红移为 z = 1.825。

Research on distant radio galaxy samples will be continued. The primary research objectives are to complete the morphologic, photometric, and spectroscopic studies on the remaining faint radio galaxies in the third Cambridge Radio Survey (3CR) samples and to approach that excellent level of completion for the 1 Jansky flux radio sources. These sources are 6 - 10 times weaker than previously observed sources and are mainly galaxies. The large redshift range covered is up to a redshift of z approximately 1.8. Further exploration of young galaxies, which are luminous and "almost-pristine" narrow hydrogen Lyman-alpha line emitters with redshift z greater than 1.5 will also be included. The impetus for this research is the discoveries of the quasi-stellar object (QSO) companion PKS1614+051B at a redshift z = 3.21, and 3C3326.1, a likely large galaxy in formation, seen at a redshift of z = 1.825.