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| 001 | 453874 | ||
| 005 | 20250716151950.0 | ||
| 024 | 7 | _ | |a 10.3847/1538-4357/ab65f5 |2 doi |
| 024 | 7 | _ | |a Marcotulli:2020xgc |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:1774363 |2 inspire |
| 024 | 7 | _ | |a 0004-637X |2 ISSN |
| 024 | 7 | _ | |a 1538-4357 |2 ISSN |
| 024 | 7 | _ | |a 2041-8205 |2 ISSN |
| 024 | 7 | _ | |a 2041-8213 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2001.01956 |2 arXiv |
| 024 | 7 | _ | |a 10.3204/PUBDB-2021-00238 |2 datacite_doi |
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| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 520 |
| 088 | _ | _ | |a arXiv:2001.01956 |2 arXiv |
| 100 | 1 | _ | |a Marcotulli, L. |0 L.Marcotulli.1 |b 0 |e Corresponding author |
| 245 | _ | _ | |a NuSTAR perspective on high-redshift MeV blazars |
| 260 | _ | _ | |a Chicago, Ill. [u.a.] |c 2020 |b Univ.11032 |
| 264 | _ | 1 | |3 online |2 Crossref |b American Astronomical Society |c 2020-02-04 |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1611598204_20991 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a 17 pages, 7 figures, 8 tables, 1 appendix, accepted for publication in ApJ |
| 520 | _ | _ | |a With bolometric luminosities exceeding $10^{48}$ erg s$^{-1}$, powerful jets and supermassive black holes at their center, MeV blazars are some of the most extreme sources in the Universe. Recently, the Fermi-Large Area Telescope detected five new $\gamma$-ray emitting MeV blazars beyond redshift $z=3.1$. With the goal of precisely characterizing the jet properties of these extreme sources, we started a multiwavelength campaign to follow them up with joint NuSTAR, Swift and SARA observations. We observe six high-redshift quasars, four of them belonging to the new $\gamma$-ray emitting MeV blazars. Thorough X-ray analysis reveals spectral flattening at soft X-ray for three of these objects. The source NVSS J151002$+$570243 also shows a peculiar re-hardening of the X-ray spectrum at energies $E>6\,\rm keV$. Adopting a one-zone leptonic emission model, this combination of hard X-rays and $\gamma$-rays enables us to determine the location of the Inverse Compton peak and to accurately constrain the jet characteristics. In the context of the jet-accretion disk connection, we find that all six sources have jet powers exceeding accretion disk luminosity, seemingly validating this positive correlation even beyond $z>3$. Our six sources are found to have $10^9 \rm M_{\odot}$ black holes, further raising the space density of supermassive black holes in the redshift bin $z=[3,4]$. |
| 536 | _ | _ | |a 613 - Matter and Radiation from the Universe (POF3-613) |0 G:(DE-HGF)POF3-613 |c POF3-613 |f POF III |x 0 |
| 542 | _ | _ | |i 2020-02-04 |2 Crossref |u http://iopscience.iop.org/info/page/text-and-data-mining |
| 542 | _ | _ | |i 2020-02-04 |2 Crossref |u http://iopscience.iop.org/page/copyright |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-MLZ)External-20140101 |5 EXP:(DE-MLZ)External-20140101 |e Measurement at external facility |x 0 |
| 700 | 1 | _ | |a Paliya, Vaidehi Sharan |0 P:(DE-H253)PIP1086596 |b 1 |e Corresponding author |
| 700 | 1 | _ | |a Ajello, M. |0 M.Ajello.1 |b 2 |
| 700 | 1 | _ | |a Kaur, A. |b 3 |
| 700 | 1 | _ | |a Marchesi, S. |0 S.Marchesi.2 |b 4 |
| 700 | 1 | _ | |a Rajagopal, M. |0 M.Rajagopal.2 |b 5 |
| 700 | 1 | _ | |a Hartmann, D. |b 6 |
| 700 | 1 | _ | |a Gasparrini, D. |0 D.Gasparrini.2 |b 7 |
| 700 | 1 | _ | |a Ojha, R. |b 8 |
| 700 | 1 | _ | |a Madejski, G. |0 G.Madejski.1 |b 9 |
| 773 | 1 | 8 | |a 10.3847/1538-4357/ab65f5 |b American Astronomical Society |d 2020-02-04 |n 2 |p 164 |3 journal-article |2 Crossref |t The Astrophysical Journal |v 889 |y 2020 |x 1538-4357 |
| 773 | _ | _ | |a 10.3847/1538-4357/ab65f5 |g Vol. 889, no. 2, p. 164 - |0 PERI:(DE-600)2006858-X |n 2 |p 164 |t The astrophysical journal / 2 |v 889 |y 2020 |x 1538-4357 |
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