PEARLS: JWST counterparts of Microjansky radio sources in the time domain field

Author(s):
Willner, S.P.; Gim, H.B.; Carmen Polletta, M. del; Cohen, S.H.; Willmer, C.N.A.; Zhao, X.; D'Silva, J.C.J.; Jansen, R.A.; Koekemoer, A.M.; Summers, J.; Windhorst, R.A.; Coe, D.; Conselice, C.J.; Driver, S.P.; Frye, B.; Grogin, N.A.; Marshall, M.A.; Nonino, M.; Ortiz, R.; Pirzkal, N.; Robotham, A.; Rutkowski, M.J.; Ryan, R.E.; Tompkins, S.; Yan, H.; Hammel, H.B.; Milam, S.N.; Adams, N.J.; Beacom, J.F.; Bhatawdekar, R.; Cheng, C.; Civano, F.; Cotton, W.; Hyun, M.; Kikuta, S.; Nyland, K.E.; Peters, W.M.; Petric, A.; Röttgering, H.J.A.; Shimwell, T.W.; Yun, M.S.
Published
2023
Publication type
Article / Letter to editor
AGN host galaxiesExtragalactic radio sourcesHigh-redshift galaxiesRadio galaxies20175087341343Astrophysics - Astrophysics of Galaxies
Date issued
2023
Language
English
Is part of
The Astrophysical Journal (2023), No. 2, 176
hdl
1887/3716170
doi
10.3847/1538-4357/acfdfb
URL
https://iopscience.iop.org/article/10.3847/1538-4357/acfdfb