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Bernd Husemann
Researcher at Leibniz Institute for Astrophysics Potsdam
Publications - 54
Citations - 4440
Bernd Husemann is an academic researcher from Leibniz Institute for Astrophysics Potsdam. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 30, co-authored 54 publications receiving 4081 citations. Previous affiliations of Bernd Husemann include Leibniz Institute for Neurobiology.
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Journal ArticleDOI
Ionized gas kinematics of galaxies in the CALIFA survey I: Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems
Begoña García-Lorenzo,I. Márquez,Jorge K. Barrera-Ballesteros,J. Masegosa,Bernd Husemann,Jesús Falcón-Barroso,Mariya Lyubenova,Sebastián F. Sánchez,J. Walcher,D. Mast,Rubén García-Benito,Jairo Méndez-Abreu,G. van de Ven,Kristine Spekkens,L. Holmes,Ana Monreal-Ibero,A. del Olmo,Bodo L. Ziegler,Joss Bland-Hawthorn,Patricia Sanchez-Blazquez,Jorge Iglesias-Páramo,J. A. L. Aguerri,P. Papaderos,J. M. Gomes,R. A. Marino,R. M. González Delgado,C. Cortijo-Ferrero,Angel R. Lopez-Sanchez,S. Bekeraite,Lutz Wisotzki,Dominik J. Bomans +30 more
TL;DR: In this paper, the authors used the cross-correlation technique to obtain the radial velocity of the dominant gaseous component and derived the main kinematic parameters directly from the radial velocities with no assumptions on the internal motions.
Journal ArticleDOI
The Close AGN Reference Survey (CARS) - What is causing Mrk1018's return to the shadows after 30 years?
Bernd Husemann,Tanya Urrutia,Grant R. Tremblay,Mirko Krumpe,Jason Dexter,Gerold Busch,Francoise Combes,Scott M. Croom,Timothy A. Davis,Andreas Eckart,R. McElroy,Miguel A. Pérez-Torres,Meredith Powell,J. Scharwächter +13 more
TL;DR: In this article, Chandra, NuStar, Swift, Hubble Space Telescope and ground-based observations were combined to explore the cause of the change in optical type of the active galactic nucleus (AGN) of Mrk 1018.
Journal ArticleDOI
Integral field spectroscopy of nearby quasi-stellar objects - II. Molecular gas content and conditions for star formation
Bernd Husemann,Timothy A. Davis,Knud Jahnke,Helmut Dannerbauer,Tanya Urrutia,Jacqueline Hodge +5 more
TL;DR: In this paper, the authors present single-dish 12CO(1 − 0) and 12 CO(2 − 1) observations for 14 low-redshift quasi-stellar objects (QSOs) and study how the cold gas content relates to the star formation rate and black hole accretion rate.
Journal ArticleDOI
Aperture corrections for disk galaxy properties derived from the CALIFA survey - Balmer emission lines in spiral galaxies
Jorge Iglesias-Páramo,José M. Vílchez,Lluís Galbany,Sebastián F. Sánchez,F. F. Rosales-Ortega,Damian Mast,Rubén García-Benito,Bernd Husemann,J. A. L. Aguerri,J. A. L. Aguerri,João Alves,S. Bekeraite,Joss Bland-Hawthorn,Cristina Catalán-Torrecilla,A. L. de Amorim,A. L. de Amorim,A. de Lorenzo-Cáceres,A. de Lorenzo-Cáceres,Simon Ellis,Jesús Falcón-Barroso,Jesús Falcón-Barroso,Hector Flores,Estrella Florido,Anna Gallazzi,Anna Gallazzi,J. M. Gomes,R. M. González Delgado,T. Haines,J. D. Hernández-Fernández,C. Kehrig,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Mariya Lyubenova,R. A. Marino,Mercedes Mollá,Ana Monreal-Ibero,A. Mourao,Polychronis Papaderos,Miguel Rodrigues,Patricia Sanchez-Blazquez,Kristine Spekkens,Vallery Stanishev,G. van de Ven,C. J. Walcher,Lutz Wisotzki,Stefano Zibetti,Bodo L. Ziegler +46 more
TL;DR: In this article, the effect of the aperture size on derived galaxy properties for which we H alpha ve spatially-resolved optical spectra was investigated, focusing on some indicators of star formation activity and dust attenuation for spiral galaxies.
Journal ArticleDOI
Aperture corrections for disk galaxy properties derived from the CALIFA survey. Balmer emission lines in spiral galaxies
Jorge Iglesias-Páramo,José M. Vílchez,Lluís Galbany,Sebastián F. Sánchez,F. F. Rosales-Ortega,Damian Mast,Rubén García-Benito,Bernd Husemann,J. A. L. Aguerri,J. Alves,S. Bekeraite,Joss Bland-Hawthorn,Cristina Catalán-Torrecilla,A. L. de Amorim,A. de Lorenzo-Cáceres,Simon Ellis,Jesús Falcón-Barroso,Hector Flores,Estrella Florido,Anna Gallazzi,J. M. Gomes,R. M. González Delgado,Tim Haines,Jonathan D. Hernández-Fernández,C. Kehrig,Angel R. Lopez-Sanchez,Mariya Lyubenova,R. A. Marino,M. Mollá,Ana Monreal-Ibero,A. Mourao,P. Papaderos,Patricia Sanchez-Blazquez,Kristine Spekkens,Vallery Stanishev,G. van de Ven,C. J. Walcher,Lutz Wisotzki,Stefano Zibetti,Bodo L. Ziegler +39 more
TL;DR: In this article, the effect of the aperture size on derived galaxy properties for which we have spatially-resolved optical spectra was investigated, focusing on some indicators of star formation activity and dust attenuation for spiral galaxies that have been widely used in previous work on galaxy evolution.