IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER
In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-ty...
Gespeichert in:
Veröffentlicht in: | The Astronomical journal 2012-04, Vol.143 (4), p.1-9 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 9 |
---|---|
container_issue | 4 |
container_start_page | 1 |
container_title | The Astronomical journal |
container_volume | 143 |
creator | Vickers, John J Grebel, Eva K HUXOR, AVON P |
description | In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-type stars. Using the g, r, i, and ; bands, we demonstrate that extraction accuracies on a par with more traditional u, g, and r photometric selection methods may be achieved. We also show that the completeness necessary to probe major Galactic structure may be maintained. Our new method allows us to efficiently select BHB stars from photometric sky surveys that do not include a u-band filter such as the Panoramic Survey Telescope and Rapid Response System. |
doi_str_mv | 10.1088/0004-6256/143/4/86 |
format | Article |
fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22034668</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1660408460</sourcerecordid><originalsourceid>FETCH-LOGICAL-c341t-281cbb6fd9e950523804b922d322817b5618e3870b555e14e4d6700aada949843</originalsourceid><addsrcrecordid>eNqN0E1Lw0AQgOFFFKzVP-Ap4MVLzOxnd_HU1rQJhBTS9KCXJdlsMdI2NZse9NebUPHsaQ7zMAMvQvcYnjBIGQAA8wXhIsCMBiyQ4gKNMKfSp1LiSzT6A9foxrkPAIwlsBF6jl_CNI8Xr3G69GbJJvSiVRa_rdJ8mnizbJrOI2-dT7O1t1kPJI9C79tbxEkeZrfoalvsnL37nWO0WYT5PPKT1TKeTxPfUIY7n0hsylJsK2UVB05o_7hUhFSU9KtJyQWWlsoJlJxzi5lllZgAFEVVKKYko2P0cL7buK7WztSdNe-mORys6TQhQJkQslePZ3Vsm8-TdZ3e187Y3a442ObkNBZCScWYov-hwEAyAT0lZ2raxrnWbvWxrfdF-6Ux6CG9Hsrqoazu02umpaA_ee5tlQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1660408460</pqid></control><display><type>article</type><title>IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER</title><source>Institute of Physics Open Access Journal Titles</source><source>EZB-FREE-00999 freely available EZB journals</source><source>IOPscience extra</source><source>Alma/SFX Local Collection</source><creator>Vickers, John J ; Grebel, Eva K ; HUXOR, AVON P</creator><creatorcontrib>Vickers, John J ; Grebel, Eva K ; HUXOR, AVON P</creatorcontrib><description>In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-type stars. Using the g, r, i, and ; bands, we demonstrate that extraction accuracies on a par with more traditional u, g, and r photometric selection methods may be achieved. We also show that the completeness necessary to probe major Galactic structure may be maintained. Our new method allows us to efficiently select BHB stars from photometric sky surveys that do not include a u-band filter such as the Panoramic Survey Telescope and Rapid Response System.</description><identifier>ISSN: 0004-6256</identifier><identifier>ISSN: 1538-3881</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.1088/0004-6256/143/4/86</identifier><language>eng</language><publisher>United States</publisher><subject>ACCURACY ; ASTRONOMY ; ASTROPHYSICS ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Bands ; COLOR ; FILTERS ; Galactic structure ; GRAVITATION ; Horizontal branch stars ; MAIN SEQUENCE STARS ; MILKY WAY ; PHOTOMETRY ; PROBES ; QUASARS ; Sky surveys (astronomy) ; Stars ; WHITE DWARF STARS</subject><ispartof>The Astronomical journal, 2012-04, Vol.143 (4), p.1-9</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c341t-281cbb6fd9e950523804b922d322817b5618e3870b555e14e4d6700aada949843</citedby><cites>FETCH-LOGICAL-c341t-281cbb6fd9e950523804b922d322817b5618e3870b555e14e4d6700aada949843</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22034668$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Vickers, John J</creatorcontrib><creatorcontrib>Grebel, Eva K</creatorcontrib><creatorcontrib>HUXOR, AVON P</creatorcontrib><title>IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER</title><title>The Astronomical journal</title><description>In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-type stars. Using the g, r, i, and ; bands, we demonstrate that extraction accuracies on a par with more traditional u, g, and r photometric selection methods may be achieved. We also show that the completeness necessary to probe major Galactic structure may be maintained. Our new method allows us to efficiently select BHB stars from photometric sky surveys that do not include a u-band filter such as the Panoramic Survey Telescope and Rapid Response System.</description><subject>ACCURACY</subject><subject>ASTRONOMY</subject><subject>ASTROPHYSICS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Bands</subject><subject>COLOR</subject><subject>FILTERS</subject><subject>Galactic structure</subject><subject>GRAVITATION</subject><subject>Horizontal branch stars</subject><subject>MAIN SEQUENCE STARS</subject><subject>MILKY WAY</subject><subject>PHOTOMETRY</subject><subject>PROBES</subject><subject>QUASARS</subject><subject>Sky surveys (astronomy)</subject><subject>Stars</subject><subject>WHITE DWARF STARS</subject><issn>0004-6256</issn><issn>1538-3881</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqN0E1Lw0AQgOFFFKzVP-Ap4MVLzOxnd_HU1rQJhBTS9KCXJdlsMdI2NZse9NebUPHsaQ7zMAMvQvcYnjBIGQAA8wXhIsCMBiyQ4gKNMKfSp1LiSzT6A9foxrkPAIwlsBF6jl_CNI8Xr3G69GbJJvSiVRa_rdJ8mnizbJrOI2-dT7O1t1kPJI9C79tbxEkeZrfoalvsnL37nWO0WYT5PPKT1TKeTxPfUIY7n0hsylJsK2UVB05o_7hUhFSU9KtJyQWWlsoJlJxzi5lllZgAFEVVKKYko2P0cL7buK7WztSdNe-mORys6TQhQJkQslePZ3Vsm8-TdZ3e187Y3a442ObkNBZCScWYov-hwEAyAT0lZ2raxrnWbvWxrfdF-6Ux6CG9Hsrqoazu02umpaA_ee5tlQ</recordid><startdate>20120401</startdate><enddate>20120401</enddate><creator>Vickers, John J</creator><creator>Grebel, Eva K</creator><creator>HUXOR, AVON P</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20120401</creationdate><title>IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER</title><author>Vickers, John J ; Grebel, Eva K ; HUXOR, AVON P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c341t-281cbb6fd9e950523804b922d322817b5618e3870b555e14e4d6700aada949843</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>ACCURACY</topic><topic>ASTRONOMY</topic><topic>ASTROPHYSICS</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Bands</topic><topic>COLOR</topic><topic>FILTERS</topic><topic>Galactic structure</topic><topic>GRAVITATION</topic><topic>Horizontal branch stars</topic><topic>MAIN SEQUENCE STARS</topic><topic>MILKY WAY</topic><topic>PHOTOMETRY</topic><topic>PROBES</topic><topic>QUASARS</topic><topic>Sky surveys (astronomy)</topic><topic>Stars</topic><topic>WHITE DWARF STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Vickers, John J</creatorcontrib><creatorcontrib>Grebel, Eva K</creatorcontrib><creatorcontrib>HUXOR, AVON P</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Vickers, John J</au><au>Grebel, Eva K</au><au>HUXOR, AVON P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER</atitle><jtitle>The Astronomical journal</jtitle><date>2012-04-01</date><risdate>2012</risdate><volume>143</volume><issue>4</issue><spage>1</spage><epage>9</epage><pages>1-9</pages><issn>0004-6256</issn><issn>1538-3881</issn><eissn>1538-3881</eissn><abstract>In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-type stars. Using the g, r, i, and ; bands, we demonstrate that extraction accuracies on a par with more traditional u, g, and r photometric selection methods may be achieved. We also show that the completeness necessary to probe major Galactic structure may be maintained. Our new method allows us to efficiently select BHB stars from photometric sky surveys that do not include a u-band filter such as the Panoramic Survey Telescope and Rapid Response System.</abstract><cop>United States</cop><doi>10.1088/0004-6256/143/4/86</doi><tpages>9</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6256 |
ispartof | The Astronomical journal, 2012-04, Vol.143 (4), p.1-9 |
issn | 0004-6256 1538-3881 1538-3881 |
language | eng |
recordid | cdi_osti_scitechconnect_22034668 |
source | Institute of Physics Open Access Journal Titles; EZB-FREE-00999 freely available EZB journals; IOPscience extra; Alma/SFX Local Collection |
subjects | ACCURACY ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Bands COLOR FILTERS Galactic structure GRAVITATION Horizontal branch stars MAIN SEQUENCE STARS MILKY WAY PHOTOMETRY PROBES QUASARS Sky surveys (astronomy) Stars WHITE DWARF STARS |
title | IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-30T10%3A38%3A36IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=IDENTIFYING%20BLUE%20HORIZONTAL%20BRANCH%20STARS%20USING%20THE%20z%20FILTER&rft.jtitle=The%20Astronomical%20journal&rft.au=Vickers,%20John%20J&rft.date=2012-04-01&rft.volume=143&rft.issue=4&rft.spage=1&rft.epage=9&rft.pages=1-9&rft.issn=0004-6256&rft.eissn=1538-3881&rft_id=info:doi/10.1088/0004-6256/143/4/86&rft_dat=%3Cproquest_osti_%3E1660408460%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1660408460&rft_id=info:pmid/&rfr_iscdi=true |