학술논문
PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain Field
Document Type
Working Paper
Author
Willner, S. P.; Gim, H. B.; Polletta, M. del Carmen; 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 III, R.; Pirzkal, N.; Robotham, A.; Rutkowski, M. J.; Ryan, Jr., 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.; Yun, M. S.
Source
Subject
Language
Abstract
The Time Domain Field (TDF) near the North Ecliptic Pole in JWST's continuous-viewing zone will become a premier "blank field" for extragalactic science. JWST/NIRCam data in a 16 arcmin$^2$ portion of the TDF identify 4.4 $\mu$m counterparts for 62 of 63 3 GHz sources with S(3 GHz) > 5 {\mu}Jy. The one unidentified radio source may be a lobe of a nearby Seyfert galaxy, or it may be an infrared-faint radio source. The bulk properties of the radio-host galaxies are consistent with those found by previous work: redshifts range from 0.14 to 4.4 with a median redshift of 1.33. The radio emission arises primarily from star formation in $\sim 2/3$ of the sample and from an active galactic nucleus in $\sim 1/3$, but just over half the sample shows evidence for an AGN either in the spectral energy distribution or by radio excess. All but three counterparts are brighter than magnitude 23 AB at 4.4 $\mu$m, and the exquisite resolution of JWST identifies correct counterparts for sources for which observations with lower angular resolution would mis-identify a nearby bright source as the counterpart when the correct one is faint and red. Up to 11% of counterparts might have been unidentified or misidentified absent NIRCam observations.
Comment: Accepted for publication in ApJ. V2 adds an author and some acknowledgments inadvertently omitted
Comment: Accepted for publication in ApJ. V2 adds an author and some acknowledgments inadvertently omitted