Dissecting GAs Stripping Phenomena in galaxies with MUSE (GASP)
Creators
-
Poggianti, B.
Publication Year
2017
Publisher
European Southern Observatory (ESO)
Resource Type
Dataset/Dataset
Descriptions
Abstract: GASP (Gas Stripping Phenomena in galaxies) is an ESO Large Program (196.B-0578) using MUSE in wide-field mode with natural seeing to study a sample of 144 galaxies at z=0.04-0.07 in different environments. The release includes reduced data cubes and fits images with maps of Hα and Hβ emission-line fluxes, Hα radial velocity, average star formation rate in four age bins, luminosity-weighted stellar age and stellar mass density, as well as the integrated 1D spectrum of each galaxy.
Other: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
Other: This is a dynamic dataset; it is growing as new data is added. The DOI refers to the newest available dataset.
Contributors
DataCurator: Gullieuszik, M.
DataCurator: Poggianti, B.
DataCurator: Poggianti, B.
Subjects
collection_name:196.B-0578 collection_type:Large Programme instrument:MUSE
Related Identifiers
References:
https://archive.eso.org
(URL)
Dates
Issued: 2017-10-26
Format
FITS