Found: 11
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Reclassification of the nearest quasar pair candidate: SDSS J15244+3032-RXS J15244+3032.
- Published in:
- Astrophysics & Space Science, 2013, v. 345, n. 1, p. 199, doi. 10.1007/s10509-013-1387-4
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- Article
Dust physics in the nucleus of NGC 4151.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 557, n. 1, p. 1, doi. 10.1051/0004-6361/201321802
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- Article
On the redshift of the bright BL Lacertae object PKS 0048-097.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 543, n. 2, p. A116-1, doi. 10.1051/0004-6361/201219114
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- Article
On the redshift of the bright BL Lacertae object PKS 0048-097.
- Published in:
- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 543, n. 1, p. 1, doi. 10.1051/0004-6361/201219114
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- Publication type:
- Article
The discovery of eight z ~ 6 quasars from Pan-STARRS1.
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- Proceedings of the International Astronomical Union, 2013, v. 9, n. S304, p. 19, doi. 10.1017/S1743921314003172
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- Article
The extended gas halo of QSO host galaxies.
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- Proceedings of the International Astronomical Union, 2013, v. 8, n. S295, p. 56, doi. 10.1017/S1743921313004262
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- Article
Co-Evolution of Supermassive Black Holes and Their Host Galaxies.
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- Proceedings of the International Astronomical Union, 2009, v. 5, n. S267, p. 34, doi. 10.1017/S1743921310005533
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- Article
Unveiling multiple AGN activity in galaxy mergers.
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- Astronomische Nachrichten, 2017, v. 338, n. 2/3, p. 262, doi. 10.1002/asna.201713340
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- Article
Massive Black Hole Binaries: Dynamical Evolution and Observational Signatures.
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- Advances in Astronomy, 2012, p. 1, doi. 10.1155/2012/940568
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- Article
Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies' interstellar medium.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2022, v. 666, p. 1, doi. 10.1051/0004-6361/202243708
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- Article
ALMA multiline survey of the ISM in two quasar host–companion galaxy pairs at z > 6.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2021, v. 652, p. 1, doi. 10.1051/0004-6361/202039696
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- Article