An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8
In the last decade, the technique of finding Ly-alpha emitters through narrow-band imaging has become a promising method of detecting high redshift galaxies. Ly-alpha emitters have been found from redshifts z ~ 2, up to the highest redshift source known to date at z = 6.96. Several surveys are also...
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| creator | Nilsson, Kim K Fynbo, Johan P. U Moller, Palle Orsi, Alvaro |
| description | In the last decade, the technique of finding Ly-alpha emitters through
narrow-band imaging has become a promising method of detecting high redshift
galaxies. Ly-alpha emitters have been found from redshifts z ~ 2, up to the
highest redshift source known to date at z = 6.96. Several surveys are also
underway to find z = 7 - 9 sources. But these very high redshift sources are
too faint to be studied in great detail, and more information can be found from
studying the same class of objects at lower redshifts. Here we present our
survey strategy to determine the nature of Ly-alpha emitters at lower
redshifts, through multi-wavelength surveys, and our plans to extend the survey
to redshift z = 8.8. |
| doi_str_mv | 10.48550/arxiv.astro-ph/0611239 |
| format | Article |
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narrow-band imaging has become a promising method of detecting high redshift
galaxies. Ly-alpha emitters have been found from redshifts z ~ 2, up to the
highest redshift source known to date at z = 6.96. Several surveys are also
underway to find z = 7 - 9 sources. But these very high redshift sources are
too faint to be studied in great detail, and more information can be found from
studying the same class of objects at lower redshifts. Here we present our
survey strategy to determine the nature of Ly-alpha emitters at lower
redshifts, through multi-wavelength surveys, and our plans to extend the survey
to redshift z = 8.8.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0611239</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2006-11</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/astro-ph/0611239$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0611239$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Nilsson, Kim K</creatorcontrib><creatorcontrib>Fynbo, Johan P. U</creatorcontrib><creatorcontrib>Moller, Palle</creatorcontrib><creatorcontrib>Orsi, Alvaro</creatorcontrib><title>An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8</title><description>In the last decade, the technique of finding Ly-alpha emitters through
narrow-band imaging has become a promising method of detecting high redshift
galaxies. Ly-alpha emitters have been found from redshifts z ~ 2, up to the
highest redshift source known to date at z = 6.96. Several surveys are also
underway to find z = 7 - 9 sources. But these very high redshift sources are
too faint to be studied in great detail, and more information can be found from
studying the same class of objects at lower redshifts. Here we present our
survey strategy to determine the nature of Ly-alpha emitters at lower
redshifts, through multi-wavelength surveys, and our plans to extend the survey
to redshift z = 8.8.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotz7tqwzAUgGEtHUraZ-hZMiqxJFu2hg4h9AaGLNnNkX1sC3xDUtK6T19IM_3bDx9jLyLZpUWWJXv0P-66wxD9zJd-n2ghpDKP7HSYYJ54N7upg_EyRMe_8UoDTV3sIVz8lVaYWyhXjsPSI9DoYiQfACN4akLv2hjgF15BAofiiT20OAR6vnfDzu9v5-MnL08fX8dDyTE3hktVqDoRTa4TlNLIokFSSmuVG0tNkVuFZFKdK6GtrNNMZAJrra0Wba0tWbVh2__tzVUt3o3o1-rmq5a-uvvUH2K1TRE</recordid><startdate>20061108</startdate><enddate>20061108</enddate><creator>Nilsson, Kim K</creator><creator>Fynbo, Johan P. U</creator><creator>Moller, Palle</creator><creator>Orsi, Alvaro</creator><scope>GOX</scope></search><sort><creationdate>20061108</creationdate><title>An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8</title><author>Nilsson, Kim K ; Fynbo, Johan P. U ; Moller, Palle ; Orsi, Alvaro</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a799-2383c01d760a22928dae3366379bed87b3ae9467316b2c45151ac66b61fc6beb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Nilsson, Kim K</creatorcontrib><creatorcontrib>Fynbo, Johan P. U</creatorcontrib><creatorcontrib>Moller, Palle</creatorcontrib><creatorcontrib>Orsi, Alvaro</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Nilsson, Kim K</au><au>Fynbo, Johan P. U</au><au>Moller, Palle</au><au>Orsi, Alvaro</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8</atitle><date>2006-11-08</date><risdate>2006</risdate><abstract>In the last decade, the technique of finding Ly-alpha emitters through
narrow-band imaging has become a promising method of detecting high redshift
galaxies. Ly-alpha emitters have been found from redshifts z ~ 2, up to the
highest redshift source known to date at z = 6.96. Several surveys are also
underway to find z = 7 - 9 sources. But these very high redshift sources are
too faint to be studied in great detail, and more information can be found from
studying the same class of objects at lower redshifts. Here we present our
survey strategy to determine the nature of Ly-alpha emitters at lower
redshifts, through multi-wavelength surveys, and our plans to extend the survey
to redshift z = 8.8.</abstract><doi>10.48550/arxiv.astro-ph/0611239</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8 |
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