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|Title:||The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5||Authors:||Stuardi, C.
LIUZZO, Elisabetta Teodorina
Kraft, R. P.
Tremblay, G. R.
Baum, S. A.
O'Dea, C. P.
Wilkes, B. J.
Forman, W. R.
Harris, D. E.
|Issue Date:||2018||Journal:||THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES||Number:||235||Issue:||2||First Page:||32||Abstract:||The aim of this paper is to present an analysis of newly acquired X-ray observations of 16 extragalactic radio sources listed in the Third Cambridge Revised (3CR) catalog and not previously observed by Chandra. Observations were performed during Chandra Cycle 17, extending X-ray coverage for the 3CR extragalactic catalog up to z = 1.5. Among the 16 targets, two lie at z < 0.5 (3CR 27 at z = 0.184 and 3CR 69 at z = 0.458) all of the remaining 14 have redshifts between 1.0 and 1.5. In the current sample, there are three compact steep spectrum (CSS) sources, three quasars, and an FR I radio galaxy, while the other nine are FR II radio galaxies. All radio sources have an X-ray counterpart. We measured nuclear X-ray fluxes as well as X-ray emission associated with radio jet knots, hotspots, or lobes in three energy bands: soft (0.5-1 keV), medium (1-2 keV), and hard (2-7 keV). We also performed standard X-ray spectral analysis for the four brightest nuclei. We discovered X-ray emission associated with the radio lobe of 3CR 124, a hotspot of the quasar 3CR 220.2, another hotspot of the radio galaxy 3CR 238, and the jet knot of 3CR 297. We also detected extended X-ray emission around the nuclear region of 3CR 124 and 3CR 297 on scales of several tens of kiloparsecs. Finally, we present an update on the X-ray observations performed with Chandra and XMM-Newton on the entire 3CR extragalactic catalog.||URI:||http://hdl.handle.net/20.500.12386/29338||URL:||https://iopscience.iop.org/article/10.3847/1538-4365/aaafcf||ISSN:||0067-0049||DOI:||10.3847/1538-4365/aaafcf||Bibcode ADS:||2018ApJS..235...32S||Fulltext:||open|
|Appears in Collections:||1.01 Articoli in rivista|
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