Author dc.contributor.author | Perger, Krisztina | |
Author dc.contributor.author | Frey, Sándor | |
Author dc.contributor.author | Gabányi, Krisztina É. | |
Availability Date dc.date.accessioned | 2020-08-08T19:34:14Z | |
Availability Date dc.date.available | 2020-08-08T19:34:14Z | |
Release dc.date.issued | 2019 | |
uri dc.identifier.uri | http://hdl.handle.net/10831/49118 | |
Language dc.language | Angol | |
Title dc.title | Is There a Blazar Nested in the Core of the Radio Galaxy 3C411? | |
Type dc.type | folyóiratcikk | |
Date Change dc.date.updated | 2020-06-05T07:33:30Z | |
Note dc.description.note | Funding Agency and Grant Number: EVN project [EP104]; Hungarian National Research, Development and Innovation Office [OTKA NN110333]; Janos Bolyai Research Scholarship of the Hungarian Academy of Sciences; European Union's Horizon 2020 research and innovation programme [730562] Funding text: We thank the anonymous referee for valuable suggestions that improved the discussion. The EVN is a joint facility of independent European, African, Asian and North American radio astronomy institutes. Scientific results from data presented in this publication are derived from the following EVN project code: EP104. The NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This publication made use of the Astrogeo VLBI FITS image database. (http://astrogeo.org/vlbi_ images/) and the authors thank Leonid Petrov for placing results of 3C411 observations online prior to publication. We thank the Hungarian National Research, Development and Innovation Office (OTKA NN110333) for support. K.E.G. was supported by the Janos Bolyai Research Scholarship of the Hungarian Academy of Sciences. This publication has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No. 730562 (RadioNet). This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. eprint: arXiv:1902.00266 | |
Doi ID dc.identifier.doi | 10.3847/1538-4357/ab040f | |
Wos ID dc.identifier.wos | 000460449000008 | |
MTMT ID dc.identifier.mtmt | 30548764 | |
Issue Number dc.identifier.issue | 1 | |
abbreviated journal dc.identifier.jabbrev | ASTROPHYS J | |
Journal dc.identifier.jtitle | ASTROPHYSICAL JOURNAL | |
Volume Number dc.identifier.volume | 873 | |
Release Date dc.description.issuedate | 2019 | |
department of Author dc.contributor.institution | MTA-BME Fizikai Geodézia és Geodinamikai Kutatócsoport | |
department of Author dc.contributor.institution | MTA-ELTE Extragalaktikus Asztrofizikai Kutatócsoport | |
department of Author dc.contributor.institution | Konkoly Thege Miklós Csillagászati Intézet | |
department of Author dc.contributor.institution | Csillagászati Tanszék | |
department of Author dc.contributor.institution | Fizika Doktori Iskola | |
department of Author dc.contributor.institution | MTA-BME Fizikai Geodézia és Geodinamika Kutatócsoport | |
Author institution dc.contributor.department | Konkoly Thege Miklós Csillagászati Intézet | |
Author institution dc.contributor.department | Csillagászati Tanszék | |
Author institution dc.contributor.department | Konkoly Thege Miklós Csillagászati Intézet | |
Author institution dc.contributor.department | Konkoly Thege Miklós Csillagászati Intézet | |
Author institution dc.contributor.department | MTA-ELTE Extragalaktikus Asztrofizikai Kutatócsoport |
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