The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products
arXiv:1707.08402 · doi:10.1093/mnras/stx3135
Abstract
We present the first major release of data from the SAMI Galaxy Survey. This data release focuses on the emission-line physics of galaxies. Data Release One includes data for 772 galaxies, about 20% of the full survey. Galaxies included have the redshift range 0.004 < z < 0.092, a large mass range (7.6 < log(Mstellar/M) < 11.6), and star-formation rates of 10^-4 to 10^1\ M/yr. For each galaxy, we include two spectral cubes and a set of spatially resolved 2D maps: single- and multi-component emission-line fits (with dust extinction corrections for strong lines), local dust extinction and star-formation rate. Calibration of the fibre throughputs, fluxes and differential-atmospheric-refraction has been improved over the Early Data Release. The data have average spatial resolution of 2.16 arcsec (FWHM) over the 15~arcsec diameter field of view and spectral (kinematic) resolution R=4263 (sigma=30km/s) around Halpha. The relative flux calibration is better than 5\% and absolute flux calibration better than ~mag, with the latter estimate limited by galaxy photometry. The data are presented online through the Australian Astronomical Observatory's Data Central.
Submitted to MNRAS. SAMI DR1 data products available from http://datacentral.aao.gov.au/asvo/surveys/sami/
References in corpus (22)
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- The Host Galaxies and Classification of Active Galactic Nuclei
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
- Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
- Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System
- The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7
- The SAMI Galaxy Survey: instrument specification and target selection
- The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
- The Current Status of Galaxy Formation
- Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
- The SAMI Galaxy Survey: Shocks and Outflows in a normal star-forming galaxy
- The SAMI Galaxy Survey: the link between angular momentum and optical morphology
- The SAMI Galaxy Survey: Revisiting Galaxy Classification Through High-Order Stellar Kinematics
- The SAMI Galaxy Survey: Early Data Release
- The SAMI Galaxy Survey: Cubism and covariance, putting round pegs into square holes
- Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies
- LZIFU: an emission-line fitting toolkit for integral field spectroscopy data
- The SAMI Galaxy Survey: The discovery of a luminous, low-metallicity H II complex in the dwarf galaxy GAMA J141103.98-003242.3
- Replicated Spectrographs in Astronomy
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