Andrea Merloni
Max Planck Society
399 Papers
9.7K Citations
Andrea Merloni is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 89, co-authored 323 publications. Previous affiliations of Andrea Merloni include Maine Principals' Association & University of Cambridge.
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Papers
Peer Review
The eROSITA Final Equatorial-Depth Survey (eFEDS): Host-galaxy Demographics of X-ray AGNs with Subaru Hyper Suprime-Cam
LLAGN and jet-scaling probed with the EVN
Zsolt Paragi,Z. Q. Shen,F. de Gasperin,Jun Yang,Andrea Merloni,Z. X. Li +5 more
- 22 Jan 2016
TL;DR: In this paper, the authors present results from EVN observations of a sample of low-luminosity AGN (LLAGN) with known mass that have unusually high radio powers when compared with their X-ray luminosity.
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The eROSITA Final Equatorial-Depth Survey (eFEDS): A multiwavelength view of WISE mid-infrared galaxies/active galactic nuclei
Yoshiki Toba,Teng Liu,Tanya Urrutia,Mara Salvato,Junyao Li,Yoshihiro Ueda,Marcella Brusa,Naomichi Yutani,Keiichi Wada,Atsushi J. Nishizawa,Johannes Buchner,Tohru Nagao,Andrea Merloni,Masayuki Akiyama,R. Arcodia,Bau-Ching Hsieh,Kohei Ichikawa,Masatoshi Imanishi,Kaiki Taro Inoue,Toshihiro Kawaguchi,Georg Lamer,Kirpal Nandra,John D. Silverman,Yuichi Terashima +23 more
TL;DR: In this paper, the authors investigated the physical properties of MIR galaxies and AGNs at the WISE W4 sample, and showed that approximately 5% of the sources in the sample are likely to be in an AGN-feedback phase, where strong radiation pressure from the AGN blows out the surrounding material from the nuclear region.
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Quiescent Times in Gamma-Ray Bursts
Andrea Merloni,Enrico Ramirez-Ruiz +1 more
- 01 Jan 2001
TL;DR: In this paper, the authors studied the internal-external shocks model for γ-ray bursts and found a quantitative proportionality relation between the duration of an emission episode and the quiescent time elapsed since the previous episode.
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Rapid evolution of the recurrence time in the repeating partial tidal disruption event eRASSt J045650.3-203750
Zhu Liu,Taeho Ryu,A. Goodwin,A. Rau,D. Homan,Mirko Krumpe,Andrea Merloni,I. Grotova,G. Anderson,A. Malyali,James Miller-Jones +10 more
- 25 Jan 2024
TL;DR: Rapid evolution of the recurrence time in the repeating partial tidal disruption event eRASSt J045650.3-203750, observed with X-ray and UV light, suggests high mass loss and potential for exploring dynamics around SMBHs beyond our own Galaxy.
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