Measuring galaxy [O ii] emission line doublet with future ground-based wide-field spectroscopic surveys
Identifieur interne : 000360 ( France/Analysis ); précédent : 000359; suivant : 000361Measuring galaxy [O ii] emission line doublet with future ground-based wide-field spectroscopic surveys
Auteurs : Johan Comparat [France] ; Jean-Paul Kneib [Suisse] ; Roland Bacon [France] ; Nick J. Mostek [États-Unis] ; Jeffrey A. Newman [États-Unis] ; David J. Schlegel [États-Unis] ; Christophe Yèche [France]Source :
- Astronomy and Astrophysics - A&A [ 0004-6361 ] ; 2013-11.
English descriptors
- mix :
Abstract
The next generation of wide-field spectroscopic redshift surveys will map the large-scale galaxy distribution in the redshift range 0.7 ≤ z ≤ 2 to measure baryonic acoustic oscillations (BAO). The primary optical signature used in this redshift range comes from the [Oii] emission line doublet, which provides a unique redshift identification that can minimize confusion with other single emission lines. To derive the required spectrograph resolution for these redshift surveys, we simulate observations of the [Oii] (λλ 3727, 3729) doublet for various instrument resolutions, and line velocities. We foresee two strategies for the choice of the resolution for future spectrographs for BAO surveys. For bright [Oii] emitter surveys ([Oii] flux ~30 × 10-17 erg cm-2 s-1 like SDSS-IV/eBOSS), a resolution of R ~ 3300 allows the separation of 90 percent of the doublets. The impact of the sky lines on the completeness in redshift is less than 6 percent. For faint [Oii] emitter surveys ([Oii] flux ~10 × 10-17 erg cm-2 s-1 like DESi), the detection improves continuously with resolution, so we recommend the highest possible resolution, the limit being given by the number of pixels (4k by 4k) on the detector and the number of spectroscopic channels (2 or 3).
Url:
DOI: 10.1051/0004-6361/201322452
Affiliations:
- France, Suisse, États-Unis
- Auvergne-Rhône-Alpes, Canton de Vaud, Pennsylvanie, Rhône-Alpes
- Lausanne, Lyon, Pittsburgh
- Université Claude Bernard Lyon 1, Université de Lyon, Université de Pittsburgh, École polytechnique fédérale de Lausanne
Links toward previous steps (curation, corpus...)
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- to stream Hal, to step Curation: 000369
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- to stream Main, to step Curation: 005A14
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Hal:cea-01135472Le document en format XML
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<ref type="url">http://irfu.cea.fr</ref>
</desc>
<listRelation> <relation name="DRF/IRFU" active="#struct-300016" type="direct"></relation>
<relation active="#struct-419361" type="direct"></relation>
</listRelation>
</org>
</tutelle>
<tutelle name="DRF/IRFU" active="#struct-300016" type="indirect"><org type="institution" xml:id="struct-300016" status="VALID"> <orgName>Commissariat à l'énergie atomique et aux énergies alternatives</orgName>
<orgName type="acronym">CEA</orgName>
<desc> <address> <addrLine>Centre de SaclayCentre de GrenobleCentre de Cadaracheetc</addrLine>
<country key="FR"></country>
</address>
<ref type="url">http://www.cea.fr/</ref>
</desc>
</org>
</tutelle>
<tutelle active="#struct-419361" type="indirect"><org type="institution" xml:id="struct-419361" status="VALID"> <orgName>Université Paris-Saclay</orgName>
<desc> <address> <addrLine>Espace Technologique, Bat. Discovery - RD 128 - 2e ét., 91190 Saint-Aubin</addrLine>
<country key="FR"></country>
</address>
<ref type="url">https://www.universite-paris-saclay.fr/fr</ref>
</desc>
</org>
</tutelle>
</tutelles>
</hal:affiliation>
<country>France</country>
</affiliation>
</author>
</analytic>
<idno type="DOI">10.1051/0004-6361/201322452</idno>
<series><title level="j">Astronomy and Astrophysics - A&A</title>
<idno type="ISSN">0004-6361</idno>
<imprint><date type="datePub">2013-11</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
</fileDesc>
<profileDesc><textClass><keywords scheme="mix" xml:lang="en"><term>cosmology: observations</term>
<term>galaxies: statistics</term>
<term>instrumentation: spectrographs</term>
<term>techniques: spectroscopic</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">The next generation of wide-field spectroscopic redshift surveys will map the large-scale galaxy distribution in the redshift range 0.7 ≤ z ≤ 2 to measure baryonic acoustic oscillations (BAO). The primary optical signature used in this redshift range comes from the [Oii] emission line doublet, which provides a unique redshift identification that can minimize confusion with other single emission lines. To derive the required spectrograph resolution for these redshift surveys, we simulate observations of the [Oii] (λλ 3727, 3729) doublet for various instrument resolutions, and line velocities. We foresee two strategies for the choice of the resolution for future spectrographs for BAO surveys. For bright [Oii] emitter surveys ([Oii] flux ~30 × 10-17 erg cm-2 s-1 like SDSS-IV/eBOSS), a resolution of R ~ 3300 allows the separation of 90 percent of the doublets. The impact of the sky lines on the completeness in redshift is less than 6 percent. For faint [Oii] emitter surveys ([Oii] flux ~10 × 10-17 erg cm-2 s-1 like DESi), the detection improves continuously with resolution, so we recommend the highest possible resolution, the limit being given by the number of pixels (4k by 4k) on the detector and the number of spectroscopic channels (2 or 3).</div>
</front>
</TEI>
<affiliations><list><country><li>France</li>
<li>Suisse</li>
<li>États-Unis</li>
</country>
<region><li>Auvergne-Rhône-Alpes</li>
<li>Canton de Vaud</li>
<li>Pennsylvanie</li>
<li>Rhône-Alpes</li>
</region>
<settlement><li>Lausanne</li>
<li>Lyon</li>
<li>Pittsburgh</li>
</settlement>
<orgName><li>Université Claude Bernard Lyon 1</li>
<li>Université de Lyon</li>
<li>Université de Pittsburgh</li>
<li>École polytechnique fédérale de Lausanne</li>
</orgName>
</list>
<tree><country name="France"><noRegion><name sortKey="Comparat, Johan" sort="Comparat, Johan" uniqKey="Comparat J" first="Johan" last="Comparat">Johan Comparat</name>
</noRegion>
<name sortKey="Bacon, Roland" sort="Bacon, Roland" uniqKey="Bacon R" first="Roland" last="Bacon">Roland Bacon</name>
<name sortKey="Yeche, Christophe" sort="Yeche, Christophe" uniqKey="Yeche C" first="Christophe" last="Yèche">Christophe Yèche</name>
</country>
<country name="Suisse"><region name="Canton de Vaud"><name sortKey="Kneib, Jean Paul" sort="Kneib, Jean Paul" uniqKey="Kneib J" first="Jean-Paul" last="Kneib">Jean-Paul Kneib</name>
</region>
</country>
<country name="États-Unis"><noRegion><name sortKey="Mostek, Nick J" sort="Mostek, Nick J" uniqKey="Mostek N" first="Nick J." last="Mostek">Nick J. Mostek</name>
</noRegion>
<name sortKey="Newman, Jeffrey A" sort="Newman, Jeffrey A" uniqKey="Newman J" first="Jeffrey A." last="Newman">Jeffrey A. Newman</name>
<name sortKey="Schlegel, David J" sort="Schlegel, David J" uniqKey="Schlegel D" first="David J." last="Schlegel">David J. Schlegel</name>
</country>
</tree>
</affiliations>
</record>
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