The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS

EMPhaSSiS is a photometric and spectroscopic survey of the disk of the Milky Way. The survey covers 33 fields in the 3rd quadrant of the Milky Way and probes every ten degrees in Galactic Longitude between l = 180∘ - 280∘ and at Galactic Latitudes of b = −20∘, − 30∘ and − 40∘. Each field is observed...

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Main Authors: Ibata R., Lane R., Lewis G., Bensby T., Noël N., Martin N., Rix H.-W., Ederoclite A., Conn B., Irwin M., Beers T., Lee Y.S.
Format: Article
Language:English
Published: EDP Sciences 2012-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20121909007
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spelling doaj-582abc2f80d54698a5ad58b84e91295d2021-08-02T05:47:37ZengEDP SciencesEPJ Web of Conferences2100-014X2012-02-01190900710.1051/epjconf/20121909007The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiSIbata R.Lane R.Lewis G.Bensby T.Noël N.Martin N.Rix H.-W.Ederoclite A.Conn B.Irwin M.Beers T.Lee Y.S.EMPhaSSiS is a photometric and spectroscopic survey of the disk of the Milky Way. The survey covers 33 fields in the 3rd quadrant of the Milky Way and probes every ten degrees in Galactic Longitude between l = 180∘ - 280∘ and at Galactic Latitudes of b = −20∘, − 30∘ and − 40∘. Each field is observed in four filters, U, B, V and R, reaching depths of 21.5, 24.0, 23.5 and 23.5 respectively. Spectroscopic observations have been carried out in 11 of these fields and in so doing, main sequence turn-off stars are being traced into the outer disk. This survey will provide metallicities and distances to the stellar populations that reside in the very outer disk of the Milky Way and help trace its evolution with increasing Galactic radius. http://dx.doi.org/10.1051/epjconf/20121909007
collection DOAJ
language English
format Article
sources DOAJ
author Ibata R.
Lane R.
Lewis G.
Bensby T.
Noël N.
Martin N.
Rix H.-W.
Ederoclite A.
Conn B.
Irwin M.
Beers T.
Lee Y.S.
spellingShingle Ibata R.
Lane R.
Lewis G.
Bensby T.
Noël N.
Martin N.
Rix H.-W.
Ederoclite A.
Conn B.
Irwin M.
Beers T.
Lee Y.S.
The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS
EPJ Web of Conferences
author_facet Ibata R.
Lane R.
Lewis G.
Bensby T.
Noël N.
Martin N.
Rix H.-W.
Ederoclite A.
Conn B.
Irwin M.
Beers T.
Lee Y.S.
author_sort Ibata R.
title The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS
title_short The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS
title_full The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS
title_fullStr The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS
title_full_unstemmed The ESO-Max Planck photometric and spectroscopic survey in the south: EMPhaSSiS
title_sort eso-max planck photometric and spectroscopic survey in the south: emphassis
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2012-02-01
description EMPhaSSiS is a photometric and spectroscopic survey of the disk of the Milky Way. The survey covers 33 fields in the 3rd quadrant of the Milky Way and probes every ten degrees in Galactic Longitude between l = 180∘ - 280∘ and at Galactic Latitudes of b = −20∘, − 30∘ and − 40∘. Each field is observed in four filters, U, B, V and R, reaching depths of 21.5, 24.0, 23.5 and 23.5 respectively. Spectroscopic observations have been carried out in 11 of these fields and in so doing, main sequence turn-off stars are being traced into the outer disk. This survey will provide metallicities and distances to the stellar populations that reside in the very outer disk of the Milky Way and help trace its evolution with increasing Galactic radius.
url http://dx.doi.org/10.1051/epjconf/20121909007
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