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Items: 4

1.

Author Correction: A population of luminous accreting black holes with hidden mergers.

Koss MJ, Blecha L, Bernhard P, Hung CL, Lu JR, Trakhtenbrot B, Treister E, Weigel A, Sartori LF, Mushotzky R, Schawinski K, Ricci C, Veilleux S, Sanders DB.

Nature. 2019 Apr;568(7750):E1. doi: 10.1038/s41586-018-0827-2.

PMID:
30899103
2.

A population of luminous accreting black holes with hidden mergers.

Koss MJ, Blecha L, Bernhard P, Hung CL, Lu JR, Trakhtenbrot B, Treister E, Weigel A, Sartori LF, Mushotzky R, Schawinski K, Ricci C, Veilleux S, Sanders DB.

Nature. 2018 Nov;563(7730):214-216. doi: 10.1038/s41586-018-0652-7. Epub 2018 Nov 7. Erratum in: Nature. 2019 Apr;568(7750):E1.

PMID:
30405225
3.

The close environments of accreting massive black holes are shaped by radiative feedback.

Ricci C, Trakhtenbrot B, Koss MJ, Ueda Y, Schawinski K, Oh K, Lamperti I, Mushotzky R, Treister E, Ho LC, Weigel A, Bauer FE, Paltani S, Fabian AC, Xie Y, Gehrels N.

Nature. 2017 Sep 27;549(7673):488-491. doi: 10.1038/nature23906.

PMID:
28959966
4.

GALAXY EVOLUTION. An over-massive black hole in a typical star-forming galaxy, 2 billion years after the Big Bang.

Trakhtenbrot B, Urry CM, Civano F, Rosario DJ, Elvis M, Schawinski K, Suh H, Bongiorno A, Simmons BD.

Science. 2015 Jul 10;349(6244):168-71. doi: 10.1126/science.aaa4506.

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