Completing the 3CR Chandra Snapshot Survey: Extragalactic Radio Sources at High Redshift
| Autor: | Francesco Massaro, William R. Forman, V. Missaglia, R. P. Kraft, Joanna Kuraszkiewicz, C. P. O'Dea, C. Stuardi, Alessandro Paggi, Belinda Jane Wilkes, M. A. Prieto, Federica Ricci, D. E. Harris, A. Jimenez-Gallardo, Stefi A. Baum, Elisabetta Liuzzo, Grant R. Tremblay |
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| Přispěvatelé: | Jimenez-Gallardo A., Massaro F., Prieto M.A., Missaglia V., Stuardi C., Paggi A., Ricci F., Kraft R.P., Liuzzo E., Tremblay G.R., Baum S.A., O'Dea C.P., Wilkes B.J., Kuraszkiewicz J., Forman W.R., Harris D.E., Jimenez-Gallardo, A., Massaro, F., Prieto, M. A., Missaglia, V., Stuardi, C., Paggi, A., Ricci, F., Kraft, R. P., Liuzzo, E., Tremblay, G. R., Baum, S. A., O’Dea, C. P., Wilkes, B. J., Kuraszkiewicz, J., Forman, W. R., Harris, D. E. |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
Active galactic nucleus
Radio sources High-energy astronomy Astrophysics::High Energy Astrophysical Phenomena astro-ph.GA Astrophysics::Cosmology and Extragalactic Astrophysics 01 natural sciences High energy astrophysic Active galaxie 0103 physical sciences 010303 astronomy & astrophysics Physics astro-ph.HE Active galactic nuclei X-ray active galactic nuclei 010308 nuclear & particles physics Astronomy Astronomy and Astrophysics Redshift Active galaxies High energy astrophysics Radio active galactic nuclei 13. Climate action Space and Planetary Science Snapshot (computer storage) |
| Zdroj: | The Astrophysical Journal Supplement Series |
| ISSN: | 0004-637X 0004-6361 0369-1829 0067-0049 1538-3873 1286-4846 |
| Popis: | We present the analysis of nine radio sources belonging to the Third Cambridge Revised catalog (3CR) observed with Chandra during Cycle 20 in the redshift range between 1.5 and 2.5. This study completes the 3CR Chandra Snapshot Survey thus guaranteeing the X-ray coverage of all 3CR sources identified to date. This sample lists two compact steep spectrum sources, four radio galaxies, and three quasars. We detected X-ray emission from all nuclei, with the only exception of 3C 326.1 and 3C 454.1 and from radio lobes in six out of nine sources at a level of confidence larger than similar to 5 sigma. We measured X-ray fluxes and luminosities for all nuclei and lobes in the soft (0.5-1 keV), medium (1-2 keV), and hard (2-7 keV) X-ray bands. Since the discovered X-ray extended emission is spatially coincident with the radio structure in all cases, its origin could be due to inverse Compton (IC) scattering of the cosmic microwave background (CMB) occurring in radio lobes. |
| Databáze: | OpenAIRE |
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