Selected Papers - Complete list of my publications on NASA/ADS

Winkel et al. (2025)Combining Direct Black Hole Mass Measurements and Spatially Resolved Stellar Kinematics to Calibrate the MBH − σ⋆ Relation of Active Galaxies ApJ, 115, 32

Winkel et al. (2023)The Close AGN Reference Survey (CARS). A parsec-scale multi-phase outflow in the super-Eddington NLS1 Mrk 1044 A&:A, 670, A3

Singha et al. (2023)The Close AGN Reference Survey (CARS): An interplay between radio jets and AGN radiation in the radio-quiet AGN HE 0040-1105 ApJ, 959, 107

Brogan et al. (2023)Still alive and kicking: A significant outburst in changing-look AGN Mrk 1018 A&A, 677, A116

McElroy et al. (2022)The Close AGN Reference Survey (CARS): Data Release 1 and Beyond Msngr, 187, 3

Smirnova-Pinchukova et al. (2022)The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends A&A 659A 125S

Winkel et al. (2022)The Close AGN Reference Survey (CARS). Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044 A&A, 663, A104

Winkel et al. (2021)The imprint of cosmic web quenching on central galaxies MNRAS 505, 4920

Siena3D: Spectroastrometry for Emission Lines in nearby AGNs

Siena3D is a tool to analyse the morphology of the ionised gas emission in 3D spectroscopic data cubes. It uses a set of emission lines to decompose an input spectrum and trace the components via their kinematics. This allows to resolve and characterize the individual components with a sub-pixel resolution, well below the width of the point spread function. Siena3D was originally developed to analyse the extended emission line region (EELR) in unobscured AGN obtained with ESO VLT/ MUSE. However, the method may also be applied to other science cases or IFU data that were aquired with other instruments.