papers

Publications (13)

astro-ph.GA2022

The Close AGN Reference Survey (CARS): Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044

N. Winkel, B. Husemann, T. A. Davis +11

The host galaxy conditions for rapid supermassive black hole growth are poorly understood. Narrow-line Seyfert 1 (NLS1) galaxies often exhibit high accretion rates and are hypothes…

astro-ph.GA2021

The Close AGN Reference Survey (CARS): IFU survey data and the BH mass dependence of long-term AGN variability

B. Husemann, M. Singha, J. Scharwächter +19

[Abridged] AGN are thought to be intimately connected with their host galaxies through feeding and feedback processes. A spatially resolved multiwavelength survey is required to ma…

astro-ph.GA2019

The GIST Pipeline: A Multi-Purpose Tool for the Analysis and Visualisation of (Integral-field) Spectroscopic Data

A. Bittner, J. Falcón-Barroso, B. Nedelchev +16

We present a convenient, all-in-one framework for the scientific analysis of fully reduced, (integral-field) spectroscopic data. The GIST pipeline (Galaxy IFU Spectroscopy Tool) is…

astro-ph.GA2021

The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends

I. Smirnova-Pinchukova, B. Husemann, T. A. Davis +17

[Abridged] Active Galactic Nuclei (AGN) are thought to be responsible for the suppression of star formation in massive ~10 M galaxies. While this process is a key fe…

astro-ph.GA2025

The PHANGS-MUSE/HST-Halpha Nebulae Catalogue

A. T. Barnes, R. Chandar, K. Kreckel +38

We present the PHANGS-MUSE/HST-Halpha nebulae catalogue, comprising 5177 spatially resolved nebulae across 19 nearby star-forming galaxies (< 20 Mpc), based on high-resolution Halp…

astro-ph.GA2020

The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies

D. Rosado-Belza, J. Falcón-Barroso, J. H. Knapen +12

Studying the stellar kinematics of galaxies is a key tool in the reconstruction of their evolution. However, the current measurements of the stellar kinematics are complicated by s…