dc.creator |
Sawicki, Marcin, 1969- |
|
dc.creator |
Lemaux, Brian C. |
|
dc.creator |
Guhathakurta, Puragra |
|
dc.creator |
Kirby, Evan N. |
|
dc.creator |
Konidaris, Nicholas P. |
|
dc.creator |
Martin, Crystal L. |
|
dc.creator |
Cooper, Michael C. |
|
dc.creator |
Koo, David C. |
|
dc.creator |
Newman, Jeffrey A. |
|
dc.creator |
Weiner, Benjamin J. |
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dc.date.accessioned |
2015-10-19T15:45:45Z |
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dc.date.available |
2015-10-19T15:45:45Z |
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dc.date.issued |
2008-11-10 |
|
dc.identifier.issn |
0004-637X |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/26423 |
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dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
We present the first results of a search for Ly[alpha] emitters (LAEs) in the DEEP2 spectroscopic database that uses a search technique that is different from but complementary to traditional narrowband imaging surveys.We have visually inspected ~20% of the available DEEP2 spectroscopic data and have found nine high-quality LAEs with clearly asymmetric line profiles and an additional 10 objects of lower quality, some of which may also be LAEs. Our survey is most sensitive to LAEs at z = 4.4-4.9 and that is indeed where all but one of our high-quality objects are found. We find the number density of our spectroscopically discovered LAEs to be consistent with those found in narrowband imaging searches. The combined, averaged spectrum of our nine high-quality objects is well fit by a two-component model, with a second, lower amplitude component redshifted by ~420 km s[superscript -1] with respect to the primary Ly[alpha] line, consistent with large-scale outflows from these objects. We conclude by discussing the advantages and future prospects of blank-sky spectroscopic surveys for high-z LAEs. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2015-10-19T15:45:45Z
No. of bitstreams: 1
Sawicki_Marcin_article_2008_a.pdf: 1458799 bytes, checksum: d6801620ad2fbab91f01d05068402796 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2015-10-19T15:45:45Z (GMT). No. of bitstreams: 1
Sawicki_Marcin_article_2008_a.pdf: 1458799 bytes, checksum: d6801620ad2fbab91f01d05068402796 (MD5)
Previous issue date: 2008-11-10 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Astronomical Society |
en_CA |
dc.relation.uri |
http://iopscience.iop.org/article/10.1086/591779/meta;jsessionid=277D3CBEA961208E8968AC558F7D309B.c3.iopscience.cld.iop.org |
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dc.rights |
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user. |
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dc.title |
The DEEP2 redshift survey: Ly[alpha] emitters in the spectroscopic database |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Astrophysical Journal 687(2), 884-898. (2008) |
en_CA |
Copyright statement:
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.