The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products
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...
Published in: | Monthly Notices of the Royal Astronomical Society |
---|---|
Main Authors: | , |
Format: | Article in Journal/Newspaper |
Language: | unknown |
Published: |
Royal Astronomical Society
2018
|
Subjects: | |
Online Access: | https://doi.org/10.1093/mnras/stx3135 |
id |
ftcaltechauth:oai:authors.library.caltech.edu:7vtx8-bba92 |
---|---|
record_format |
openpolar |
spelling |
ftcaltechauth:oai:authors.library.caltech.edu:7vtx8-bba92 2024-10-13T14:10:33+00:00 The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products Green, Andrew W. Medling, Anne M. 2018-03-21 https://doi.org/10.1093/mnras/stx3135 unknown Royal Astronomical Society https://arxiv.org/abs/1707.08402 https://doi.org/10.1093/mnras/stx3135 eprintid:85780 info:eu-repo/semantics/openAccess Other Monthly Notices of the Royal Astronomical Society, 475(1), 716-734, (2018-03-21) surveys galaxies: general info:eu-repo/semantics/article 2018 ftcaltechauth https://doi.org/10.1093/mnras/stx3135 2024-09-25T18:46:36Z 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 ∼10^1M⊙ 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. © 2017 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2017 December 1. Received 2017 November 30; in original form 2017 May 16. Published: 11 December 2017. The SAMI Galaxy Survey is based on observations made at the Anglo-Australian Telescope. The Sydney/AAO Multi-object Integral-field spectrograph (SAMI) was developed jointly by the University of Sydney and the Australian Astronomical Observatory. The SAMI input catalogue is based on data taken from the Sloan Digital Sky Survey, the GAMA survey, and the VST ATLAS survey. The SAMI Galaxy Survey is funded by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions. The SAMI Galaxy Survey website is ... Article in Journal/Newspaper sami Caltech Authors (California Institute of Technology) Monthly Notices of the Royal Astronomical Society 475 1 716 734 |
institution |
Open Polar |
collection |
Caltech Authors (California Institute of Technology) |
op_collection_id |
ftcaltechauth |
language |
unknown |
topic |
surveys galaxies: general |
spellingShingle |
surveys galaxies: general Green, Andrew W. Medling, Anne M. The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products |
topic_facet |
surveys galaxies: general |
description |
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 ∼10^1M⊙ 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. © 2017 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2017 December 1. Received 2017 November 30; in original form 2017 May 16. Published: 11 December 2017. The SAMI Galaxy Survey is based on observations made at the Anglo-Australian Telescope. The Sydney/AAO Multi-object Integral-field spectrograph (SAMI) was developed jointly by the University of Sydney and the Australian Astronomical Observatory. The SAMI input catalogue is based on data taken from the Sloan Digital Sky Survey, the GAMA survey, and the VST ATLAS survey. The SAMI Galaxy Survey is funded by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions. The SAMI Galaxy Survey website is ... |
format |
Article in Journal/Newspaper |
author |
Green, Andrew W. Medling, Anne M. |
author_facet |
Green, Andrew W. Medling, Anne M. |
author_sort |
Green, Andrew W. |
title |
The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products |
title_short |
The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products |
title_full |
The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products |
title_fullStr |
The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products |
title_full_unstemmed |
The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products |
title_sort |
sami galaxy survey: data release one with emission-line physics value-added products |
publisher |
Royal Astronomical Society |
publishDate |
2018 |
url |
https://doi.org/10.1093/mnras/stx3135 |
genre |
sami |
genre_facet |
sami |
op_source |
Monthly Notices of the Royal Astronomical Society, 475(1), 716-734, (2018-03-21) |
op_relation |
https://arxiv.org/abs/1707.08402 https://doi.org/10.1093/mnras/stx3135 eprintid:85780 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1093/mnras/stx3135 |
container_title |
Monthly Notices of the Royal Astronomical Society |
container_volume |
475 |
container_issue |
1 |
container_start_page |
716 |
op_container_end_page |
734 |
_version_ |
1812817875076907008 |