Back to Search Start Over

The SAMI Galaxy Survey : Data Release Two with absorption-line physics value-added products

Authors :
Sarah Brough
Christoph Federrath
Samuel N. Richards
M. L. P. Gunawardhana
Simon P. Driver
Jon Lawrence
Mathew R. Varidel
Scott M. Croom
Francesco D'Eugenio
Henry Poetrodjojo
Matt S. Owers
Sarah M. Sweet
Andrew W. Green
Jesse van de Sande
Dan S. Taranu
Luca Cortese
Joss Bland-Hawthorn
Michael J. Drinkwater
Anne M. Medling
Katrina Sealey
Brent Groves
Sebastián F. Sánchez
Elizabeth Mannering
Sree Oh
Yifei Jin
Caroline Foster
Lloyd Harischandra
Simon J. O'Toole
Nicholas Scott
Dilyar Barat
Michael Goodwin
Rob Sharp
A. L. Schaefer
Nuria P. F. Lorente
Tania M. Barone
Matthew Colless
Julia J. Bryant
University of St Andrews. School of Physics and Astronomy
Source :
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 481(2), 2299-2319
Publication Year :
2018

Abstract

We present the second major release of data from the SAMI Galaxy Survey. Data Release Two includes data for 1559 galaxies, about 50% of the full survey. Galaxies included have a redshift range 0.004 < z < 0.113 and a large stellar mass range 7.5 < log (M_star/M_sun) < 11.6. The core data for each galaxy consist of two primary spectral cubes covering the blue and red optical wavelength ranges. For each primary cube we also provide three spatially binned spectral cubes and a set of standardised aperture spectra. For each core data product we provide a set of value-added data products. This includes all emission line value-added products from Data Release One, expanded to the larger sample. In addition we include stellar kinematic and stellar population value-added products derived from absorption line measurements. The data are provided online through Australian Astronomical Optics' Data Central. We illustrate the potential of this release by presenting the distribution of ~350,000 stellar velocity dispersion measurements from individual spaxels as a function of R/R_e, divided in four galaxy mass bins. In the highest stellar mass bin (log (M_star/M_sun)>11), the velocity dispersion strongly increases towards the centre, whereas below log (M_star/M_sun)<br />22 pages, 14 figures. Accepted for publication in MNRAS. See the SAMI Data Release 2 website (https://sami-survey.org/abdr) for current status. The data can be accessed via Australian Astronomical Optics' Data Central service (https://datacentral.org.au/)

Details

Language :
English
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, 481(2), 2299-2319
Accession number :
edsair.doi.dedup.....ab7bf445d43eafc7db56235c7a4c55f5