LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW

We present observational details and first results of a near-infrared (JHKs) synoptic survey of the central region of the Large Magellanic Cloud (LMC) using the CPAPIR camera at the CTIO 1.5 m telescope. We covered 18 square degrees to a depth of K sub(s)~16.5 mag and obtained an average of 16 epoch...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astronomical journal 2015-04, Vol.149 (4), p.1-17
Hauptverfasser: Macri, Lucas M, Ngeow, Chow-Choong, Kanbur, Shashi M, Mahzooni, Salma, Smitka, Michael T
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 17
container_issue 4
container_start_page 1
container_title The Astronomical journal
container_volume 149
creator Macri, Lucas M
Ngeow, Chow-Choong
Kanbur, Shashi M
Mahzooni, Salma
Smitka, Michael T
description We present observational details and first results of a near-infrared (JHKs) synoptic survey of the central region of the Large Magellanic Cloud (LMC) using the CPAPIR camera at the CTIO 1.5 m telescope. We covered 18 square degrees to a depth of K sub(s)~16.5 mag and obtained an average of 16 epochs in each band at any given location. Our catalog contains more than 3.5 x 10 super(6) sources, including 1417 Cepheid variables previously studied at optical wavelengths by the OGLE survey. Our sample of fundamental-mode pulsators represents a nine-fold increase in the number of these variables with time-resolved, multi-band near-infrared photometry. We combine our large Cepheid sample and a recent precise determination of the distance to the LMC to derive a robust absolute calibration of the near-infrared Leavitt Law for fundamental-mode and first-overtone Cepheids with 10x better constraints on the slopes relative to previous work. We also obtain calibrations for the tip of the red giant branch and the red clump based on our ensemble photometry which are in good agreement with previous determinations.
doi_str_mv 10.1088/0004-6256/149/4/117
format Article
fullrecord <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22879397</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1770356515</sourcerecordid><originalsourceid>FETCH-LOGICAL-c409t-ce3ff4a76c55c2bcfc55a8d527de713daf976237f368a6fc1f5a8056f9389eb83</originalsourceid><addsrcrecordid>eNqFkT1PwzAQhiMEEp-_gMUSC0taO45jZzSp21oyCUrTIiYruLYoKg3EYeDf41IGNqY73fvcDfdE0TWCIwQZG0MI0zhLSDZGaT5OxwjRo-gMEcxizBg6_tOfRufev0KIEIPpWfSheD0T4J7PhFK8lAUoVLWcgFLwOpbltOa1mIDFU1k9NCFcLOuVeBoBOQKFeJgLOQErXkt-p8QC8HICmrkABVfyruaNrEpQTX9GSvCVbBqg-ONldOLarbdXv_UiWk5FU8xjVc1kWI1NCvMhNhY7l7Y0M4SY5Nm4UFu2JgldW4rwunU5zRJMHc5YmzmDXIghyVyOWW6fGb6Ibg53Oz9stDebwZoX0-121gw6SRjNcU4DdXug3vvu49P6Qb9tvLHbbbuz3afXiFKISUbC__5HccISSnAeUHxATd9531un3_vNW9t_aQT13pjeG9N7YzoY06kOxvA3wLR93w</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1732827539</pqid></control><display><type>article</type><title>LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW</title><source>IOP Publishing Free Content</source><source>EZB-FREE-00999 freely available EZB journals</source><source>IOPscience extra</source><source>Alma/SFX Local Collection</source><creator>Macri, Lucas M ; Ngeow, Chow-Choong ; Kanbur, Shashi M ; Mahzooni, Salma ; Smitka, Michael T</creator><creatorcontrib>Macri, Lucas M ; Ngeow, Chow-Choong ; Kanbur, Shashi M ; Mahzooni, Salma ; Smitka, Michael T</creatorcontrib><description>We present observational details and first results of a near-infrared (JHKs) synoptic survey of the central region of the Large Magellanic Cloud (LMC) using the CPAPIR camera at the CTIO 1.5 m telescope. We covered 18 square degrees to a depth of K sub(s)~16.5 mag and obtained an average of 16 epochs in each band at any given location. Our catalog contains more than 3.5 x 10 super(6) sources, including 1417 Cepheid variables previously studied at optical wavelengths by the OGLE survey. Our sample of fundamental-mode pulsators represents a nine-fold increase in the number of these variables with time-resolved, multi-band near-infrared photometry. We combine our large Cepheid sample and a recent precise determination of the distance to the LMC to derive a robust absolute calibration of the near-infrared Leavitt Law for fundamental-mode and first-overtone Cepheids with 10x better constraints on the slopes relative to previous work. We also obtain calibrations for the tip of the red giant branch and the red clump based on our ensemble photometry which are in good agreement with previous determinations.</description><identifier>ISSN: 1538-3881</identifier><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.1088/0004-6256/149/4/117</identifier><language>eng</language><publisher>United States</publisher><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; CALIBRATION ; CAMERAS ; Cepheid variables ; CEPHEIDS ; Clumps ; INFRARED SURVEYS ; LIMITING VALUES ; MAGELLANIC CLOUDS ; NEAR INFRARED RADIATION ; PHOTOMETRY ; Slopes ; TELESCOPES ; TIME RESOLUTION ; WAVELENGTHS</subject><ispartof>The Astronomical journal, 2015-04, Vol.149 (4), p.1-17</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c409t-ce3ff4a76c55c2bcfc55a8d527de713daf976237f368a6fc1f5a8056f9389eb83</citedby><cites>FETCH-LOGICAL-c409t-ce3ff4a76c55c2bcfc55a8d527de713daf976237f368a6fc1f5a8056f9389eb83</cites><orcidid>0000-0001-8771-7554</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27903,27904</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22879397$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Macri, Lucas M</creatorcontrib><creatorcontrib>Ngeow, Chow-Choong</creatorcontrib><creatorcontrib>Kanbur, Shashi M</creatorcontrib><creatorcontrib>Mahzooni, Salma</creatorcontrib><creatorcontrib>Smitka, Michael T</creatorcontrib><title>LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW</title><title>The Astronomical journal</title><description>We present observational details and first results of a near-infrared (JHKs) synoptic survey of the central region of the Large Magellanic Cloud (LMC) using the CPAPIR camera at the CTIO 1.5 m telescope. We covered 18 square degrees to a depth of K sub(s)~16.5 mag and obtained an average of 16 epochs in each band at any given location. Our catalog contains more than 3.5 x 10 super(6) sources, including 1417 Cepheid variables previously studied at optical wavelengths by the OGLE survey. Our sample of fundamental-mode pulsators represents a nine-fold increase in the number of these variables with time-resolved, multi-band near-infrared photometry. We combine our large Cepheid sample and a recent precise determination of the distance to the LMC to derive a robust absolute calibration of the near-infrared Leavitt Law for fundamental-mode and first-overtone Cepheids with 10x better constraints on the slopes relative to previous work. We also obtain calibrations for the tip of the red giant branch and the red clump based on our ensemble photometry which are in good agreement with previous determinations.</description><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>CALIBRATION</subject><subject>CAMERAS</subject><subject>Cepheid variables</subject><subject>CEPHEIDS</subject><subject>Clumps</subject><subject>INFRARED SURVEYS</subject><subject>LIMITING VALUES</subject><subject>MAGELLANIC CLOUDS</subject><subject>NEAR INFRARED RADIATION</subject><subject>PHOTOMETRY</subject><subject>Slopes</subject><subject>TELESCOPES</subject><subject>TIME RESOLUTION</subject><subject>WAVELENGTHS</subject><issn>1538-3881</issn><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqFkT1PwzAQhiMEEp-_gMUSC0taO45jZzSp21oyCUrTIiYruLYoKg3EYeDf41IGNqY73fvcDfdE0TWCIwQZG0MI0zhLSDZGaT5OxwjRo-gMEcxizBg6_tOfRufev0KIEIPpWfSheD0T4J7PhFK8lAUoVLWcgFLwOpbltOa1mIDFU1k9NCFcLOuVeBoBOQKFeJgLOQErXkt-p8QC8HICmrkABVfyruaNrEpQTX9GSvCVbBqg-ONldOLarbdXv_UiWk5FU8xjVc1kWI1NCvMhNhY7l7Y0M4SY5Nm4UFu2JgldW4rwunU5zRJMHc5YmzmDXIghyVyOWW6fGb6Ibg53Oz9stDebwZoX0-121gw6SRjNcU4DdXug3vvu49P6Qb9tvLHbbbuz3afXiFKISUbC__5HccISSnAeUHxATd9531un3_vNW9t_aQT13pjeG9N7YzoY06kOxvA3wLR93w</recordid><startdate>20150401</startdate><enddate>20150401</enddate><creator>Macri, Lucas M</creator><creator>Ngeow, Chow-Choong</creator><creator>Kanbur, Shashi M</creator><creator>Mahzooni, Salma</creator><creator>Smitka, Michael T</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><orcidid>https://orcid.org/0000-0001-8771-7554</orcidid></search><sort><creationdate>20150401</creationdate><title>LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW</title><author>Macri, Lucas M ; Ngeow, Chow-Choong ; Kanbur, Shashi M ; Mahzooni, Salma ; Smitka, Michael T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c409t-ce3ff4a76c55c2bcfc55a8d527de713daf976237f368a6fc1f5a8056f9389eb83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>CALIBRATION</topic><topic>CAMERAS</topic><topic>Cepheid variables</topic><topic>CEPHEIDS</topic><topic>Clumps</topic><topic>INFRARED SURVEYS</topic><topic>LIMITING VALUES</topic><topic>MAGELLANIC CLOUDS</topic><topic>NEAR INFRARED RADIATION</topic><topic>PHOTOMETRY</topic><topic>Slopes</topic><topic>TELESCOPES</topic><topic>TIME RESOLUTION</topic><topic>WAVELENGTHS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Macri, Lucas M</creatorcontrib><creatorcontrib>Ngeow, Chow-Choong</creatorcontrib><creatorcontrib>Kanbur, Shashi M</creatorcontrib><creatorcontrib>Mahzooni, Salma</creatorcontrib><creatorcontrib>Smitka, Michael T</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; 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>Macri, Lucas M</au><au>Ngeow, Chow-Choong</au><au>Kanbur, Shashi M</au><au>Mahzooni, Salma</au><au>Smitka, Michael T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW</atitle><jtitle>The Astronomical journal</jtitle><date>2015-04-01</date><risdate>2015</risdate><volume>149</volume><issue>4</issue><spage>1</spage><epage>17</epage><pages>1-17</pages><issn>1538-3881</issn><issn>0004-6256</issn><eissn>1538-3881</eissn><abstract>We present observational details and first results of a near-infrared (JHKs) synoptic survey of the central region of the Large Magellanic Cloud (LMC) using the CPAPIR camera at the CTIO 1.5 m telescope. We covered 18 square degrees to a depth of K sub(s)~16.5 mag and obtained an average of 16 epochs in each band at any given location. Our catalog contains more than 3.5 x 10 super(6) sources, including 1417 Cepheid variables previously studied at optical wavelengths by the OGLE survey. Our sample of fundamental-mode pulsators represents a nine-fold increase in the number of these variables with time-resolved, multi-band near-infrared photometry. We combine our large Cepheid sample and a recent precise determination of the distance to the LMC to derive a robust absolute calibration of the near-infrared Leavitt Law for fundamental-mode and first-overtone Cepheids with 10x better constraints on the slopes relative to previous work. We also obtain calibrations for the tip of the red giant branch and the red clump based on our ensemble photometry which are in good agreement with previous determinations.</abstract><cop>United States</cop><doi>10.1088/0004-6256/149/4/117</doi><tpages>17</tpages><orcidid>https://orcid.org/0000-0001-8771-7554</orcidid></addata></record>
fulltext fulltext
identifier ISSN: 1538-3881
ispartof The Astronomical journal, 2015-04, Vol.149 (4), p.1-17
issn 1538-3881
0004-6256
1538-3881
language eng
recordid cdi_osti_scitechconnect_22879397
source IOP Publishing Free Content; EZB-FREE-00999 freely available EZB journals; IOPscience extra; Alma/SFX Local Collection
subjects ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
CALIBRATION
CAMERAS
Cepheid variables
CEPHEIDS
Clumps
INFRARED SURVEYS
LIMITING VALUES
MAGELLANIC CLOUDS
NEAR INFRARED RADIATION
PHOTOMETRY
Slopes
TELESCOPES
TIME RESOLUTION
WAVELENGTHS
title LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. I. CEPHEID VARIABLES AND THE CALIBRATION OF THE LEAVITT LAW
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-27T10%3A54%3A20IST&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=LARGE%20MAGELLANIC%20CLOUD%20NEAR-INFRARED%20SYNOPTIC%20SURVEY.%20I.%20CEPHEID%20VARIABLES%20AND%20THE%20CALIBRATION%20OF%20THE%20LEAVITT%20LAW&rft.jtitle=The%20Astronomical%20journal&rft.au=Macri,%20Lucas%20M&rft.date=2015-04-01&rft.volume=149&rft.issue=4&rft.spage=1&rft.epage=17&rft.pages=1-17&rft.issn=1538-3881&rft.eissn=1538-3881&rft_id=info:doi/10.1088/0004-6256/149/4/117&rft_dat=%3Cproquest_osti_%3E1770356515%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=1732827539&rft_id=info:pmid/&rfr_iscdi=true