Population synthesis of RR Lyrae stars in the original $Kepler$ and $K2$ Fields of View
It is interesting to ask what fraction of the total available RR Lyrae (RRL) sample that falls in the $Kepler$ and $K2$ Fields of View (FoV) is known or discovered. In order assess the completeness of our sample we compared the known RRL sample in the $Kepler$ and $K2$ fields with synthetic Galactic...
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| creator | Hanyecz, Ottó Szabó, Róbert |
| description | It is interesting to ask what fraction of the total available RR Lyrae (RRL)
sample that falls in the $Kepler$ and $K2$ Fields of View (FoV) is known or
discovered. In order assess the completeness of our sample we compared the
known RRL sample in the $Kepler$ and $K2$ fields with synthetic Galactic
models. The Catalina Sky Survey RRL sample was used to calibrate our method. We
found that a large number of faint RRL stars is missing from $Kepler$ and $K2$
fields. |
| doi_str_mv | 10.48550/arxiv.1603.02512 |
| format | Article |
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sample that falls in the $Kepler$ and $K2$ Fields of View (FoV) is known or
discovered. In order assess the completeness of our sample we compared the
known RRL sample in the $Kepler$ and $K2$ fields with synthetic Galactic
models. The Catalina Sky Survey RRL sample was used to calibrate our method. We
found that a large number of faint RRL stars is missing from $Kepler$ and $K2$
fields.</description><identifier>DOI: 10.48550/arxiv.1603.02512</identifier><language>eng</language><subject>Physics - Solar and Stellar Astrophysics</subject><creationdate>2016-03</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,781,886</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1603.02512$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1603.02512$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Hanyecz, Ottó</creatorcontrib><creatorcontrib>Szabó, Róbert</creatorcontrib><title>Population synthesis of RR Lyrae stars in the original $Kepler$ and $K2$ Fields of View</title><description>It is interesting to ask what fraction of the total available RR Lyrae (RRL)
sample that falls in the $Kepler$ and $K2$ Fields of View (FoV) is known or
discovered. In order assess the completeness of our sample we compared the
known RRL sample in the $Kepler$ and $K2$ fields with synthetic Galactic
models. The Catalina Sky Survey RRL sample was used to calibrate our method. We
found that a large number of faint RRL stars is missing from $Kepler$ and $K2$
fields.</description><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj01LxDAURbNxIaM_wJVv0W1rmqSvzVIGR8WCMgwzy_JsEg3UtiT1o__emerqcrmcC4exq5xnqioKfkPhx39lOXKZcVHk4pwdXobxs6PJDz3EuZ_ebfQRBgfbLdRzIAtxohDB93DcYAj-zffUQfJkx86GBKg3xyIS2HjbmQXde_t9wc4cddFe_ueK7TZ3u_VDWj_fP65v65SwFGkrHGIrjRbKoVbOuQKN5XmpsNSIXHD9qkk64pUzlWy5rLiRbWURNZFTcsWu_24Xs2YM_oPC3JwMm8VQ_gJ15UoC</recordid><startdate>20160308</startdate><enddate>20160308</enddate><creator>Hanyecz, Ottó</creator><creator>Szabó, Róbert</creator><scope>GOX</scope></search><sort><creationdate>20160308</creationdate><title>Population synthesis of RR Lyrae stars in the original $Kepler$ and $K2$ Fields of View</title><author>Hanyecz, Ottó ; Szabó, Róbert</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a672-c2f66c3d924f694fff56de0174679660209b9a3fa08fd83c0380d3c8e669aaf43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Hanyecz, Ottó</creatorcontrib><creatorcontrib>Szabó, Róbert</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Hanyecz, Ottó</au><au>Szabó, Róbert</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Population synthesis of RR Lyrae stars in the original $Kepler$ and $K2$ Fields of View</atitle><date>2016-03-08</date><risdate>2016</risdate><abstract>It is interesting to ask what fraction of the total available RR Lyrae (RRL)
sample that falls in the $Kepler$ and $K2$ Fields of View (FoV) is known or
discovered. In order assess the completeness of our sample we compared the
known RRL sample in the $Kepler$ and $K2$ fields with synthetic Galactic
models. The Catalina Sky Survey RRL sample was used to calibrate our method. We
found that a large number of faint RRL stars is missing from $Kepler$ and $K2$
fields.</abstract><doi>10.48550/arxiv.1603.02512</doi><oa>free_for_read</oa></addata></record> |
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| identifier | DOI: 10.48550/arxiv.1603.02512 |
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| subjects | Physics - Solar and Stellar Astrophysics |
| title | Population synthesis of RR Lyrae stars in the original $Kepler$ and $K2$ Fields of View |
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