no code implementations • 11 Aug 2022 • Fabian Parzer, Prashin Jethwa, Alina Boecker, Mayte Alfaro-Cuello, Otmar Scherzer, Glenn van de Ven
In this context, blobs may correspond to stars born in-situ versus those accreted from satellites, and the task of blob detection is to disentangle these components.
no code implementations • 14 Jan 2021 • Alan H. Su, Heikki Salo, Joachim Janz, Eija Laurikainen, Aku Venhola, Reynier F. Peletier, Enrica Iodice, Michael Hilker, Michele Cantiello, Nicola Napolitano, Marilena Spavone, Maria A. Raj, Glenn van de Ven, Steffen. Mieske, Maurizio Paolillo, Massimo Capaccioli, Edwin A. Valentijn, Aaron E. Watkins
Overall, we find significant differences in the distributions of quantities derived from S\'ersic profiles ($g'-r'$, $r'-i'$, $R_e$, and $\bar{\mu}_{e, r'}$), and non-parametric indices ($A$ and $S$) between the Fornax main cluster and Fornax A group.
Astrophysics of Galaxies
no code implementations • 1 May 2020 • Gauri Sharma, Paolo Salucci, C. M. Harrison, Glenn van de Ven, Andrea Lapi
We do not see any change in the shape of RCs with respect to the local star-forming disk-type galaxies.
Astrophysics of Galaxies