A colour-excess extinction map of the southern Galactic disc from the VVV and GLIMPSE surveys

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dc.creator Soto, M.
dc.creator Barbá, R.
dc.creator Minniti, D.
dc.creator Kunder, A.
dc.creator Majaess, Daniel J
dc.creator Nilo-Castellón, J. L.
dc.creator Alonso-García, J.
dc.creator Leone, G.
dc.creator Morelli, L.
dc.creator Haikala, L.
dc.creator Firpo, V.
dc.creator Lucas, P.
dc.creator Emerson, J.P.
dc.creator Moni Bidin, C.
dc.creator Geisler, D.
dc.creator Saito, R.K.
dc.creator Gurovich, S.
dc.creator Contreras Ramos, R.
dc.creator Rejkuba, M.
dc.creator Barbieri, M.
dc.creator Roman-Lopes, A.
dc.creator Hempel, M.
dc.creator Alonso, M. V.
dc.creator Baravalle, L. D.
dc.creator Borissova, J.
dc.creator Kurtev, R.
dc.creator Milla, F.
dc.date.accessioned 2022-04-26T13:53:34Z
dc.date.available 2022-04-26T13:53:34Z
dc.date.issued 2019-09-11
dc.identifier.issn 1365-2966
dc.identifier.issn 0035-8711
dc.identifier.uri http://library2.smu.ca/xmlui/handle/01/30878
dc.description Published version en_CA
dc.description.abstract An improved high-resolution and deep A<sub>Ks</sub> foreground dust extinction map is presented for the Galactic disc area within 295&deg; ≲ l ≲ 350&deg;, &minus;1.0&deg; ≲ <em>b</em> ≲ +1.0&deg;. At some longitudes the map reaches up to |<em>b</em>| &sim; 2.25&deg;, for a total of &sim;148&thinsp;deg<sup>2</sup>. The map was constructed via the Rayleigh&ndash;Jeans colour excess (RJCE) technique based on deep near-infrared (NIR) and mid-infrared (MIR) photometry. The new extinction map features a maximum bin size of 1', and relies on NIR observations from the Two Micron All-Sky Survey (2MASS) and new data from ESO&rsquo;s Vista Variables in the V&iacute;a L&aacute;ctea (VVV) survey, in concert with MIR observations from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire. The VVV photometry penetrates &sim;4&thinsp;mag fainter than 2MASS, and provides enhanced sampling of the underlying stellar populations in this heavily obscured region. Consequently, the new results supersede existing RJCE maps tied solely to brighter photometry, revealing a systematic underestimation of extinction in prior work that was based on shallower data. The new high-resolution and large-scale extinction map presented here is readily available to the community through a web query interface. en_CA
dc.description.provenance Submitted by Sherry Briere (sherry.briere@smu.ca) on 2022-04-26T13:53:34Z No. of bitstreams: 1 Majaess_D_article_2019.pdf: 9479002 bytes, checksum: e6c87f343ec3173f407f0a3336993855 (MD5) en
dc.description.provenance Made available in DSpace on 2022-04-26T13:53:34Z (GMT). No. of bitstreams: 1 Majaess_D_article_2019.pdf: 9479002 bytes, checksum: e6c87f343ec3173f407f0a3336993855 (MD5) Previous issue date: 2019-09 en
dc.language.iso en_CA en_CA
dc.publisher Oxford University Press (OUP) en_CA
dc.relation.uri https://arxiv.org/pdf/1909.03131.pdf
dc.rights This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2019 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.subject.lcsh Extinction (Biology)
dc.title A colour-excess extinction map of the southern Galactic disc from the VVV and GLIMPSE surveys en_CA
dc.type Text en_CA
dcterms.bibliographicCitation Monthly Notices of the Royal Astronomical Society 488(2): 2650-2657. (2019) en_CA
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This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2019 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
 
Published Version: https://arxiv.org/pdf/1909.03131.pdf
 
 

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