[PDF] Top 20 SDSS IV MaNGA : spatially resolved star formation histories and the connection to galaxy physical properties

... in star formation from the fossil record provided by local galaxies alone, since many processes will have acted upon each galaxy over cosmic ...of star formation via feedback gives rise ... See full document

... the spatially resolved excitation properties of the ionized gas in a sample of 646 galaxies using integral field spectroscopy data from the Sloan Digital Sky Survey IV Mapping Nearby Galaxies ... See full document

... like SDSS ( ...of star formation cessation in galaxies thus requires spatially resolved measurements of stellar and gaseous components to be obtained for a large sample of galaxies ... See full document

... the spatially-resolved history of stellar mass as- sembly for galaxies beyond the Local Group, demon- strating how massive galaxies grow their stellar mass inside-out (P´erez et ...of galaxy ... See full document

... different formation mechanisms of fast and slow rotators produce an observable difference in their star formation histories? To study this we identify quenching slow rotators in the ... See full document

... of star formation cessation in galaxies, one would need spatially resolved spectrosc- opy to measure the stellar and gaseous components for a large sample of galaxies covering a wide range of ... See full document

... among star-forming galaxies ( Sánchez et ...the spatially resolved growth history ( Pérez et ...the spatially resolved stellar mass – metallicity relation ( González Delgado et ...the ... See full document

... ber SDSS spectroscopy, which lacks spatial information and covers only the central part of nearby ...the star formation histories ( including recent and on-going SFR ) of galaxies can be ... See full document

... and star formation ...among star-forming galaxies (Sánchez et ...the spatially-resolved growth history (Pérez et ...the spatially-resolved stel- lar mass-metallicity ... See full document

... the MaNGA prototype instrument in Belfiore et al. (2015). By using spatially resolved maps of nebular diagnostics and stellar popula- tion ages, this work has added substantial support to the notion ... See full document

... at spatially resolved scales and identify the signals for both the mass based and environment based quenching ...in MaNGA through stellar population analysis by Goddard et ...reduced star ... See full document

... a galaxy to be passive (Cheung et ...host galaxy are, however, not currently un- ...of star formation, as radiative-mode AGN are often associated with the presence of star ... See full document

... Survey IV has been provided by the Alfred ...Institutions. SDSS- IV acknowledges support and resources from the Center for High-Performance Computing at the University of ...The SDSS web site ... See full document

... each galaxy is a statistical sample per se, and even if the results for single spaxels (or zones) are uncertain, the overall trends should be ...population properties with ... See full document

... the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon Uni- versity, the Chilean Participation Group, the French Par- ticipation Group, ... See full document

... All science-ready data products are produced by the Data Reduction Pipeline (DRP; Law et al. 2016), a semi- automated procedure that performs the reduction, calibra- tion and sky-subtraction for MaNGA ... See full document

... the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institu- tion for Science, Carnegie Mellon University, the Chilean Participa- tion Group, the French Participation Group, ... See full document

... calculated using the ONS calibration (Pilyugin, V´ılchez & Thuan 2010). The red dashed line represents the N/O expected when nitrogen is only a primary nucleosynthetic product, while the blue dashed line represents a ... See full document

... the SDSS are significantly larger than those reported by the Sloan Digital Sky Survey (SDSS) ...the SDSS sky biases luminosities by more than a few tenths of a magnitude for objects with half-light ... See full document

... three star formation relations, consistent with the Chabrier ...other star formation relations based on gas surface density [Bigiel et ...Other star formation relations shown in ... See full document