P Salucci - The Astronomy and Astrophysics Review, 2019 - Springer
The distribution of the non-luminous matter in galaxies of different luminosity and Hubble type is much more than a proof of the existence of dark particles governing the structures of …
E Emsellem, E Schinnerer, F Santoro, F Belfiore… - Astronomy & …, 2022 - aanda.org
We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field spectrograph at the ESO VLT to map 19 massive (9.4< log (M⋆/M⊙)< 11.0) nearby (D≲ 20 …
M Cappellari - Monthly Notices of the Royal Astronomical …, 2017 - academic.oup.com
I start by providing an updated summary of the penalized pixel-fitting (ppxf) method that is used to extract the stellar and gas kinematics, as well as the stellar population of galaxies …
K Bundy, MA Bershady, DR Law, R Yan… - The Astrophysical …, 2014 - iopscience.iop.org
We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the …
DR Law, B Cherinka, R Yan, BH Andrews… - The Astronomical …, 2016 - iopscience.iop.org
ABSTRACT Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs …
T Naab, JP Ostriker - Annual review of astronomy and …, 2017 - annualreviews.org
Numerical simulations have become a major tool for understanding galaxy formation and evolution. Over the decades the field has made significant progress. It is now possible to …
M Cappellari - Annual review of astronomy and astrophysics, 2016 - annualreviews.org
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
Abstract The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi- object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey …
The final product of galaxy evolution through cosmic time is the population of galaxies in the local universe. These galaxies are also those that can be studied in most detail, thus …