THE ASTEROSEISMIC POTENTIAL OF TESS: EXOPLANET-HOST STARS

ABSTRACT New insights on stellar evolution and stellar interior physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host stars and their planetary systems. The upcomi...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2016-10, Vol.830 (2), p.138
Hauptverfasser: Campante, T. L., Schofield, M., Kuszlewicz, J. S., Bouma, L., Chaplin, W. J., Huber, D., Christensen-Dalsgaard, J., Kjeldsen, H., Bossini, D., North, T. S. H., Appourchaux, T., Latham, D. W., Pepper, J., Ricker, G. R., Stassun, K. G., Vanderspek, R., Winn, J. N.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 2
container_start_page 138
container_title The Astrophysical journal
container_volume 830
creator Campante, T. L.
Schofield, M.
Kuszlewicz, J. S.
Bouma, L.
Chaplin, W. J.
Huber, D.
Christensen-Dalsgaard, J.
Kjeldsen, H.
Bossini, D.
North, T. S. H.
Appourchaux, T.
Latham, D. W.
Pepper, J.
Ricker, G. R.
Stassun, K. G.
Vanderspek, R.
Winn, J. N.
description ABSTRACT New insights on stellar evolution and stellar interior physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host stars and their planetary systems. The upcoming NASA Transiting Exoplanet Survey Satellite (TESS) will be performing a near all-sky survey for planets that transit bright nearby stars. In addition, its excellent photometric precision, combined with its fine time sampling and long intervals of uninterrupted observations, will enable asteroseismology of solar-type and red-giant stars. Here we develop a simple test to estimate the detectability of solar-like oscillations in TESS photometry of any given star. Based on an all-sky stellar and planetary synthetic population, we go on to predict the asteroseismic yield of the TESS mission, placing emphasis on the yield of exoplanet-host stars for which we expect to detect solar-like oscillations. This is done for both the target stars (observed at a 2-minute cadence) and the full-frame-image stars (observed at a 30-minute cadence). A similar exercise is also conducted based on a compilation of known host stars. We predict that TESS will detect solar-like oscillations in a few dozen target hosts (mainly subgiant stars but also in a smaller number of F dwarfs), in up to 200 low-luminosity red-giant hosts, and in over 100 solar-type and red-giant known hosts, thereby leading to a threefold improvement in the asteroseismic yield of exoplanet-host stars when compared to Kepler's.
doi_str_mv 10.3847/0004-637X/830/2/138
format Article
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_journals_2365897579</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365897579</sourcerecordid><originalsourceid>FETCH-LOGICAL-c498t-143472b98ee45eded655c92471e177bf9575d9e58569f9d2dabd739fff3d8d4a3</originalsourceid><addsrcrecordid>eNp9kE1Lw0AQhhdRsFZ_gZeA55jsV3bHWyhbE4hN6a7Q25J2d6FFTU3ag__ehIrePA0D7_MO8yB0j9NHKplI0jRlcUbFOpE0TUiCqbxAE8ypjBnl4hJNfhPX6Kbv9-NKACYITKGiXBu1qrUq9Us5i5a1UQtT5lVUzyOjtH6K1LpeVvlCmbiotYm0yVf6Fl2F5q33dz9zil7nysyKuKqfy1lexVsG8hhjRpkgG5DeM-6ddxnnWyBMYI-F2ATggjvwXPIMAjjimo0TFEII1EnHGjpFD-feQ9d-nnx_tPv21H0MJy2hGZcguIAhRc-pbdf2feeDPXS796b7sji1oyM7vmxHA3ZwZIkdHA1UcqZ27eGv9j_iG5dvYgk</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365897579</pqid></control><display><type>article</type><title>THE ASTEROSEISMIC POTENTIAL OF TESS: EXOPLANET-HOST STARS</title><source>IOP_英国物理学会OA刊</source><creator>Campante, T. L. ; Schofield, M. ; Kuszlewicz, J. S. ; Bouma, L. ; Chaplin, W. J. ; Huber, D. ; Christensen-Dalsgaard, J. ; Kjeldsen, H. ; Bossini, D. ; North, T. S. H. ; Appourchaux, T. ; Latham, D. W. ; Pepper, J. ; Ricker, G. R. ; Stassun, K. G. ; Vanderspek, R. ; Winn, J. N.</creator><creatorcontrib>Campante, T. L. ; Schofield, M. ; Kuszlewicz, J. S. ; Bouma, L. ; Chaplin, W. J. ; Huber, D. ; Christensen-Dalsgaard, J. ; Kjeldsen, H. ; Bossini, D. ; North, T. S. H. ; Appourchaux, T. ; Latham, D. W. ; Pepper, J. ; Ricker, G. R. ; Stassun, K. G. ; Vanderspek, R. ; Winn, J. N.</creatorcontrib><description>ABSTRACT New insights on stellar evolution and stellar interior physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host stars and their planetary systems. The upcoming NASA Transiting Exoplanet Survey Satellite (TESS) will be performing a near all-sky survey for planets that transit bright nearby stars. In addition, its excellent photometric precision, combined with its fine time sampling and long intervals of uninterrupted observations, will enable asteroseismology of solar-type and red-giant stars. Here we develop a simple test to estimate the detectability of solar-like oscillations in TESS photometry of any given star. Based on an all-sky stellar and planetary synthetic population, we go on to predict the asteroseismic yield of the TESS mission, placing emphasis on the yield of exoplanet-host stars for which we expect to detect solar-like oscillations. This is done for both the target stars (observed at a 2-minute cadence) and the full-frame-image stars (observed at a 30-minute cadence). A similar exercise is also conducted based on a compilation of known host stars. We predict that TESS will detect solar-like oscillations in a few dozen target hosts (mainly subgiant stars but also in a smaller number of F dwarfs), in up to 200 low-luminosity red-giant hosts, and in over 100 solar-type and red-giant known hosts, thereby leading to a threefold improvement in the asteroseismic yield of exoplanet-host stars when compared to Kepler's.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/0004-637X/830/2/138</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>asteroseismology ; Astrophysics ; Extrasolar planets ; Giant stars ; Kepler mission (NASA) ; Luminosity ; Oscillations ; Photometry ; Planet detection ; Planetary systems ; planets and satellites: detection ; Red giant stars ; Sky surveys (astronomy) ; Solar oscillations ; space vehicles: instruments ; Stellar evolution ; Stellar seismology ; Subgiant stars ; surveys ; techniques: photometric ; Transit ; Yield</subject><ispartof>The Astrophysical journal, 2016-10, Vol.830 (2), p.138</ispartof><rights>2016. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Oct 20, 2016</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c498t-143472b98ee45eded655c92471e177bf9575d9e58569f9d2dabd739fff3d8d4a3</citedby><cites>FETCH-LOGICAL-c498t-143472b98ee45eded655c92471e177bf9575d9e58569f9d2dabd739fff3d8d4a3</cites><orcidid>0000-0002-4265-047X ; 0000-0002-5714-8618 ; 0000-0003-4894-9779 ; 0000-0001-9911-7388 ; 0000-0002-1790-1951 ; 0000-0002-3827-8417 ; 0000-0002-3481-9052 ; 0000-0002-4588-5389 ; 0000-0001-5137-0966</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/0004-637X/830/2/138/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,776,780,27901,27902,38867,53842</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/0004-637X/830/2/138$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc></links><search><creatorcontrib>Campante, T. L.</creatorcontrib><creatorcontrib>Schofield, M.</creatorcontrib><creatorcontrib>Kuszlewicz, J. S.</creatorcontrib><creatorcontrib>Bouma, L.</creatorcontrib><creatorcontrib>Chaplin, W. J.</creatorcontrib><creatorcontrib>Huber, D.</creatorcontrib><creatorcontrib>Christensen-Dalsgaard, J.</creatorcontrib><creatorcontrib>Kjeldsen, H.</creatorcontrib><creatorcontrib>Bossini, D.</creatorcontrib><creatorcontrib>North, T. S. H.</creatorcontrib><creatorcontrib>Appourchaux, T.</creatorcontrib><creatorcontrib>Latham, D. W.</creatorcontrib><creatorcontrib>Pepper, J.</creatorcontrib><creatorcontrib>Ricker, G. R.</creatorcontrib><creatorcontrib>Stassun, K. G.</creatorcontrib><creatorcontrib>Vanderspek, R.</creatorcontrib><creatorcontrib>Winn, J. N.</creatorcontrib><title>THE ASTEROSEISMIC POTENTIAL OF TESS: EXOPLANET-HOST STARS</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>ABSTRACT New insights on stellar evolution and stellar interior physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host stars and their planetary systems. The upcoming NASA Transiting Exoplanet Survey Satellite (TESS) will be performing a near all-sky survey for planets that transit bright nearby stars. In addition, its excellent photometric precision, combined with its fine time sampling and long intervals of uninterrupted observations, will enable asteroseismology of solar-type and red-giant stars. Here we develop a simple test to estimate the detectability of solar-like oscillations in TESS photometry of any given star. Based on an all-sky stellar and planetary synthetic population, we go on to predict the asteroseismic yield of the TESS mission, placing emphasis on the yield of exoplanet-host stars for which we expect to detect solar-like oscillations. This is done for both the target stars (observed at a 2-minute cadence) and the full-frame-image stars (observed at a 30-minute cadence). A similar exercise is also conducted based on a compilation of known host stars. We predict that TESS will detect solar-like oscillations in a few dozen target hosts (mainly subgiant stars but also in a smaller number of F dwarfs), in up to 200 low-luminosity red-giant hosts, and in over 100 solar-type and red-giant known hosts, thereby leading to a threefold improvement in the asteroseismic yield of exoplanet-host stars when compared to Kepler's.</description><subject>asteroseismology</subject><subject>Astrophysics</subject><subject>Extrasolar planets</subject><subject>Giant stars</subject><subject>Kepler mission (NASA)</subject><subject>Luminosity</subject><subject>Oscillations</subject><subject>Photometry</subject><subject>Planet detection</subject><subject>Planetary systems</subject><subject>planets and satellites: detection</subject><subject>Red giant stars</subject><subject>Sky surveys (astronomy)</subject><subject>Solar oscillations</subject><subject>space vehicles: instruments</subject><subject>Stellar evolution</subject><subject>Stellar seismology</subject><subject>Subgiant stars</subject><subject>surveys</subject><subject>techniques: photometric</subject><subject>Transit</subject><subject>Yield</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNp9kE1Lw0AQhhdRsFZ_gZeA55jsV3bHWyhbE4hN6a7Q25J2d6FFTU3ag__ehIrePA0D7_MO8yB0j9NHKplI0jRlcUbFOpE0TUiCqbxAE8ypjBnl4hJNfhPX6Kbv9-NKACYITKGiXBu1qrUq9Us5i5a1UQtT5lVUzyOjtH6K1LpeVvlCmbiotYm0yVf6Fl2F5q33dz9zil7nysyKuKqfy1lexVsG8hhjRpkgG5DeM-6ddxnnWyBMYI-F2ATggjvwXPIMAjjimo0TFEII1EnHGjpFD-feQ9d-nnx_tPv21H0MJy2hGZcguIAhRc-pbdf2feeDPXS796b7sji1oyM7vmxHA3ZwZIkdHA1UcqZ27eGv9j_iG5dvYgk</recordid><startdate>20161020</startdate><enddate>20161020</enddate><creator>Campante, T. L.</creator><creator>Schofield, M.</creator><creator>Kuszlewicz, J. S.</creator><creator>Bouma, L.</creator><creator>Chaplin, W. J.</creator><creator>Huber, D.</creator><creator>Christensen-Dalsgaard, J.</creator><creator>Kjeldsen, H.</creator><creator>Bossini, D.</creator><creator>North, T. S. H.</creator><creator>Appourchaux, T.</creator><creator>Latham, D. W.</creator><creator>Pepper, J.</creator><creator>Ricker, G. R.</creator><creator>Stassun, K. G.</creator><creator>Vanderspek, R.</creator><creator>Winn, J. N.</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-4265-047X</orcidid><orcidid>https://orcid.org/0000-0002-5714-8618</orcidid><orcidid>https://orcid.org/0000-0003-4894-9779</orcidid><orcidid>https://orcid.org/0000-0001-9911-7388</orcidid><orcidid>https://orcid.org/0000-0002-1790-1951</orcidid><orcidid>https://orcid.org/0000-0002-3827-8417</orcidid><orcidid>https://orcid.org/0000-0002-3481-9052</orcidid><orcidid>https://orcid.org/0000-0002-4588-5389</orcidid><orcidid>https://orcid.org/0000-0001-5137-0966</orcidid></search><sort><creationdate>20161020</creationdate><title>THE ASTEROSEISMIC POTENTIAL OF TESS: EXOPLANET-HOST STARS</title><author>Campante, T. L. ; Schofield, M. ; Kuszlewicz, J. S. ; Bouma, L. ; Chaplin, W. J. ; Huber, D. ; Christensen-Dalsgaard, J. ; Kjeldsen, H. ; Bossini, D. ; North, T. S. H. ; Appourchaux, T. ; Latham, D. W. ; Pepper, J. ; Ricker, G. R. ; Stassun, K. G. ; Vanderspek, R. ; Winn, J. N.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c498t-143472b98ee45eded655c92471e177bf9575d9e58569f9d2dabd739fff3d8d4a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>asteroseismology</topic><topic>Astrophysics</topic><topic>Extrasolar planets</topic><topic>Giant stars</topic><topic>Kepler mission (NASA)</topic><topic>Luminosity</topic><topic>Oscillations</topic><topic>Photometry</topic><topic>Planet detection</topic><topic>Planetary systems</topic><topic>planets and satellites: detection</topic><topic>Red giant stars</topic><topic>Sky surveys (astronomy)</topic><topic>Solar oscillations</topic><topic>space vehicles: instruments</topic><topic>Stellar evolution</topic><topic>Stellar seismology</topic><topic>Subgiant stars</topic><topic>surveys</topic><topic>techniques: photometric</topic><topic>Transit</topic><topic>Yield</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Campante, T. L.</creatorcontrib><creatorcontrib>Schofield, M.</creatorcontrib><creatorcontrib>Kuszlewicz, J. S.</creatorcontrib><creatorcontrib>Bouma, L.</creatorcontrib><creatorcontrib>Chaplin, W. J.</creatorcontrib><creatorcontrib>Huber, D.</creatorcontrib><creatorcontrib>Christensen-Dalsgaard, J.</creatorcontrib><creatorcontrib>Kjeldsen, H.</creatorcontrib><creatorcontrib>Bossini, D.</creatorcontrib><creatorcontrib>North, T. S. H.</creatorcontrib><creatorcontrib>Appourchaux, T.</creatorcontrib><creatorcontrib>Latham, D. W.</creatorcontrib><creatorcontrib>Pepper, J.</creatorcontrib><creatorcontrib>Ricker, G. R.</creatorcontrib><creatorcontrib>Stassun, K. G.</creatorcontrib><creatorcontrib>Vanderspek, R.</creatorcontrib><creatorcontrib>Winn, J. N.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Campante, T. L.</au><au>Schofield, M.</au><au>Kuszlewicz, J. S.</au><au>Bouma, L.</au><au>Chaplin, W. J.</au><au>Huber, D.</au><au>Christensen-Dalsgaard, J.</au><au>Kjeldsen, H.</au><au>Bossini, D.</au><au>North, T. S. H.</au><au>Appourchaux, T.</au><au>Latham, D. W.</au><au>Pepper, J.</au><au>Ricker, G. R.</au><au>Stassun, K. G.</au><au>Vanderspek, R.</au><au>Winn, J. N.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE ASTEROSEISMIC POTENTIAL OF TESS: EXOPLANET-HOST STARS</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2016-10-20</date><risdate>2016</risdate><volume>830</volume><issue>2</issue><spage>138</spage><pages>138-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>ABSTRACT New insights on stellar evolution and stellar interior physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host stars and their planetary systems. The upcoming NASA Transiting Exoplanet Survey Satellite (TESS) will be performing a near all-sky survey for planets that transit bright nearby stars. In addition, its excellent photometric precision, combined with its fine time sampling and long intervals of uninterrupted observations, will enable asteroseismology of solar-type and red-giant stars. Here we develop a simple test to estimate the detectability of solar-like oscillations in TESS photometry of any given star. Based on an all-sky stellar and planetary synthetic population, we go on to predict the asteroseismic yield of the TESS mission, placing emphasis on the yield of exoplanet-host stars for which we expect to detect solar-like oscillations. This is done for both the target stars (observed at a 2-minute cadence) and the full-frame-image stars (observed at a 30-minute cadence). A similar exercise is also conducted based on a compilation of known host stars. We predict that TESS will detect solar-like oscillations in a few dozen target hosts (mainly subgiant stars but also in a smaller number of F dwarfs), in up to 200 low-luminosity red-giant hosts, and in over 100 solar-type and red-giant known hosts, thereby leading to a threefold improvement in the asteroseismic yield of exoplanet-host stars when compared to Kepler's.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/0004-637X/830/2/138</doi><tpages>15</tpages><orcidid>https://orcid.org/0000-0002-4265-047X</orcidid><orcidid>https://orcid.org/0000-0002-5714-8618</orcidid><orcidid>https://orcid.org/0000-0003-4894-9779</orcidid><orcidid>https://orcid.org/0000-0001-9911-7388</orcidid><orcidid>https://orcid.org/0000-0002-1790-1951</orcidid><orcidid>https://orcid.org/0000-0002-3827-8417</orcidid><orcidid>https://orcid.org/0000-0002-3481-9052</orcidid><orcidid>https://orcid.org/0000-0002-4588-5389</orcidid><orcidid>https://orcid.org/0000-0001-5137-0966</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2016-10, Vol.830 (2), p.138
issn 0004-637X
1538-4357
language eng
recordid cdi_proquest_journals_2365897579
source IOP_英国物理学会OA刊
subjects asteroseismology
Astrophysics
Extrasolar planets
Giant stars
Kepler mission (NASA)
Luminosity
Oscillations
Photometry
Planet detection
Planetary systems
planets and satellites: detection
Red giant stars
Sky surveys (astronomy)
Solar oscillations
space vehicles: instruments
Stellar evolution
Stellar seismology
Subgiant stars
surveys
techniques: photometric
Transit
Yield
title THE ASTEROSEISMIC POTENTIAL OF TESS: EXOPLANET-HOST STARS
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-01T10%3A07%3A22IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=THE%20ASTEROSEISMIC%20POTENTIAL%20OF%20TESS:%20EXOPLANET-HOST%20STARS&rft.jtitle=The%20Astrophysical%20journal&rft.au=Campante,%20T.%20L.&rft.date=2016-10-20&rft.volume=830&rft.issue=2&rft.spage=138&rft.pages=138-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/0004-637X/830/2/138&rft_dat=%3Cproquest_O3W%3E2365897579%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2365897579&rft_id=info:pmid/&rfr_iscdi=true