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Journal Article

The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products

MPS-Authors

Green,  Andrew W.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Croom,  Scott M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Scott,  Nicholas
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cortese,  Luca
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Medling,  Anne M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

D'Eugenio,  Francesco
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bryant,  Julia J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bland-Hawthorn,  Joss
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Allen,  J. T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sharp,  Rob
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ho,  I. -Ting
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Groves,  Brent
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Drinkwater,  Michael J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mannering,  Elizabeth
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Harischandra,  Lloyd
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

van de Sande,  Jesse
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Thomas,  Adam D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

O'Toole,  Simon
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

McDermid,  Richard M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Vuong,  Minh
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sealey,  Katrina
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bauer,  Amanda E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Brough,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Catinella,  Barbara
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cecil,  Gerald
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Colless,  Matthew
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Couch,  Warrick J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Driver,  Simon P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Federrath,  Christoph
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Foster,  Caroline
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Goodwin,  Michael
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hampton,  Elise J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hopkins,  A. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jones,  D. Heath
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Konstantopoulos,  Iraklis S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lawrence,  J. S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Leon-Saval,  Sergio G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Liske,  Jochen
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

López-Sánchez,  Ángel R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lorente,  Nuria P. F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mould,  Jeremy
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Obreschkow,  Danail
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Owers,  Matt S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Richards,  Samuel N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Robotham,  Aaron S. G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Schaefer,  Adam L.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sweet,  Sarah M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Taranu,  Dan S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tescari,  Edoardo
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tonini,  Chiara
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Zafar,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018MNRAS.475..716G
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Citation

Green, A. W., Croom, S. M., Scott, N., Cortese, L., Medling, A. M., D'Eugenio, F., et al. (2018). The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products. Monthly Notices of the Royal Astronomical Society, 475, 716-734.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CD82-1
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 per cent of the full survey. Galaxies included have the redshift range 0.004 < z < 0.092, a large mass range (7.6 < log M*/ M☉ < 11.6), and star formation rates of ̃10-4 to ̃101M☉ yr-1. 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 (full width at half-maximum) over the 15 arcsec diameter field of view and spectral (kinematic) resolution of R = 4263 (σ = 30 km s-1) around H α. The relative flux calibration is better than 5 per cent, and absolute flux calibration has an rms of 10 per cent. The data are presented online through the Australian Astronomical Observatory's Data Central.