101 citations · 484 across the 15 of their papers we have counts for
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Simultaneous H alpha and dust reverberation mapping of 3C120: Testing the bowl-shaped torus geometry
Michael Ramolla, Martin Haas, Christian Westhues +8
At the Universitaetssternwarte Bochum near Cerro Armazones we have monitored the Seyfert-1 galaxy 3C 120 between September 2014 and March 2015 in BVRI and a narrow band filter cove…
Galaxy overdensities around 3C radio galaxies and quasars at revealed by Spitzer m and Pan-STARRS
Z. Ghaffari, Ch. Westhues, M. Haas +4
Luminous radio sources are thought to lie in galaxy clusters or proto-clusters. The complete sample of 64 high-redshift 3C sources at has been mapped with the Spitzer Spa…
Star formation in 3CR radio galaxies and quasars at z < 1
Christian Westhues, Martin Haas, Peter Barthel +8
Using the Herschel Space Observatory we have observed a representative sample of 87 powerful 3CR sources at redshift z < 1. The far-infrared (FIR, 70-500 micron) photometry is comb…
The stability of the optical flux variation gradient for 3C120
Michael Ramolla, Francisco Pozo Nuñez, Christian Westhues +2
New - and -band monitoring in 2014 2015 reveals that the Seyfert 1 Galaxy, 3C120, has brightened by a magnitude of , compared to our campaign that took place in 2009…
The broad-line region and dust torus size of the Seyfert 1 galaxy PGC50427
F. Pozo Nuñez, M. Ramolla, C. Westhues +10
We present the results of a three years monitoring campaigns of the type-1 active galactic nucleus (AGN) PGC50427. Through the use of Photometric Reverberation Mapping…
Star formation in z>1 3CR host galaxies as seen by Herschel
P. Podigachoski, P. D. Barthel, M. Haas +15
We present Herschel (PACS and SPIRE) far-infrared (FIR) photometry of a complete sample of z>1 3CR sources, from the Herschel GT project The Herschel Legacy of distant radio-loud A…
Dust reverberation-mapping of the Seyfert 1 galaxy WPVS48
F. Pozo Nuñez, M. Haas, R. Chini +7
Using robotic telescopes of the Universitatssternwarte Bochum near Cerro Armazones in Chile, we monitored the z=0.0377 Seyfert 1 galaxy WPVS48 (2MASX J09594263-3112581) in the opti…