Space Photometry with Brite-Constellation

BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and allows for very long and continuous observing runs wi...
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Autor*in:	Werner W. Weiss [verfasserIn] Konstanze Zwintz [verfasserIn] Rainer Kuschnig [verfasserIn] Gerald Handler [verfasserIn] Anthony F. J. Moffat [verfasserIn] Dietrich Baade [verfasserIn] Dominic M. Bowman [verfasserIn] Thomas Granzer [verfasserIn] Thomas Kallinger [verfasserIn] Otto F. Koudelka [verfasserIn] Catherine C. Lovekin [verfasserIn] Coralie Neiner [verfasserIn] Herbert Pablo [verfasserIn] Andrzej Pigulski [verfasserIn] Adam Popowicz [verfasserIn] Tahina Ramiaramanantsoa [verfasserIn] Slavek M. Rucinski [verfasserIn] Klaus G. Strassmeier [verfasserIn] Gregg A. Wade [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2021

Schlagwörter:	space photometry stellar structure stellar evolution stellar environment nanosatellites

Übergeordnetes Werk:	In: Universe - MDPI AG, 2015, 7(2021), 6, p 199
Übergeordnetes Werk:	volume:7 ; year:2021 ; number:6, p 199

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/universe7060199

Katalog-ID:	DOAJ031442781

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authorswithroles_txt_mv	Werner W. Weiss @@aut@@ Konstanze Zwintz @@aut@@ Rainer Kuschnig @@aut@@ Gerald Handler @@aut@@ Anthony F. J. Moffat @@aut@@ Dietrich Baade @@aut@@ Dominic M. Bowman @@aut@@ Thomas Granzer @@aut@@ Thomas Kallinger @@aut@@ Otto F. Koudelka @@aut@@ Catherine C. Lovekin @@aut@@ Coralie Neiner @@aut@@ Herbert Pablo @@aut@@ Andrzej Pigulski @@aut@@ Adam Popowicz @@aut@@ Tahina Ramiaramanantsoa @@aut@@ Slavek M. Rucinski @@aut@@ Klaus G. Strassmeier @@aut@@ Gregg A. Wade @@aut@@
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callnumber-first	Q - Science
author	Werner W. Weiss
spellingShingle	Werner W. Weiss misc QC793-793.5 misc space photometry misc stellar structure misc stellar evolution misc stellar environment misc nanosatellites misc Elementary particle physics Space Photometry with Brite-Constellation
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topic_title	QC793-793.5 Space Photometry with Brite-Constellation space photometry stellar structure stellar evolution stellar environment nanosatellites
topic	misc QC793-793.5 misc space photometry misc stellar structure misc stellar evolution misc stellar environment misc nanosatellites misc Elementary particle physics
topic_unstemmed	misc QC793-793.5 misc space photometry misc stellar structure misc stellar evolution misc stellar environment misc nanosatellites misc Elementary particle physics
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title	Space Photometry with Brite-Constellation
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author_browse	Werner W. Weiss Konstanze Zwintz Rainer Kuschnig Gerald Handler Anthony F. J. Moffat Dietrich Baade Dominic M. Bowman Thomas Granzer Thomas Kallinger Otto F. Koudelka Catherine C. Lovekin Coralie Neiner Herbert Pablo Andrzej Pigulski Adam Popowicz Tahina Ramiaramanantsoa Slavek M. Rucinski Klaus G. Strassmeier Gregg A. Wade
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title_sort	space photometry with brite-constellation
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title_auth	Space Photometry with Brite-Constellation
abstract	BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and allows for very long and continuous observing runs with high time resolution and thus provides the data necessary for understanding various processes inside stars (e.g., asteroseismology) and in their immediate environment. While the first astronomical observations from space focused on the spectral regions not accessible from the ground it soon became obvious around 1970 that avoiding the turbulent terrestrial atmosphere significantly improved the accuracy of photometry and satellites explicitly dedicated to high-quality photometry were launched. A perfect example is BRITE-Constellation, which is the result of a very successful cooperation between Austria, Canada and Poland. Research highlights for targets distributed nearly over the entire HRD are presented, but focus primarily on massive and hot stars.
abstractGer	BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and allows for very long and continuous observing runs with high time resolution and thus provides the data necessary for understanding various processes inside stars (e.g., asteroseismology) and in their immediate environment. While the first astronomical observations from space focused on the spectral regions not accessible from the ground it soon became obvious around 1970 that avoiding the turbulent terrestrial atmosphere significantly improved the accuracy of photometry and satellites explicitly dedicated to high-quality photometry were launched. A perfect example is BRITE-Constellation, which is the result of a very successful cooperation between Austria, Canada and Poland. Research highlights for targets distributed nearly over the entire HRD are presented, but focus primarily on massive and hot stars.
abstract_unstemmed	BRITE-Constellation is devoted to high-precision optical photometric monitoring of bright stars, distributed all over the Milky Way, in red and/or blue passbands. Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and allows for very long and continuous observing runs with high time resolution and thus provides the data necessary for understanding various processes inside stars (e.g., asteroseismology) and in their immediate environment. While the first astronomical observations from space focused on the spectral regions not accessible from the ground it soon became obvious around 1970 that avoiding the turbulent terrestrial atmosphere significantly improved the accuracy of photometry and satellites explicitly dedicated to high-quality photometry were launched. A perfect example is BRITE-Constellation, which is the result of a very successful cooperation between Austria, Canada and Poland. Research highlights for targets distributed nearly over the entire HRD are presented, but focus primarily on massive and hot stars.
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container_issue	6, p 199
title_short	Space Photometry with Brite-Constellation
url	https://doi.org/10.3390/universe7060199 https://doaj.org/article/ea1eaae50a7a49ed95580ffc7e659ca9 https://www.mdpi.com/2218-1997/7/6/199 https://doaj.org/toc/2218-1997
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author2	Konstanze Zwintz Rainer Kuschnig Gerald Handler Anthony F. J. Moffat Dietrich Baade Dominic M. Bowman Thomas Granzer Thomas Kallinger Otto F. Koudelka Catherine C. Lovekin Coralie Neiner Herbert Pablo Andrzej Pigulski Adam Popowicz Tahina Ramiaramanantsoa Slavek M. Rucinski Klaus G. Strassmeier Gregg A. Wade
author2Str	Konstanze Zwintz Rainer Kuschnig Gerald Handler Anthony F. J. Moffat Dietrich Baade Dominic M. Bowman Thomas Granzer Thomas Kallinger Otto F. Koudelka Catherine C. Lovekin Coralie Neiner Herbert Pablo Andrzej Pigulski Adam Popowicz Tahina Ramiaramanantsoa Slavek M. Rucinski Klaus G. Strassmeier Gregg A. Wade
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up_date	2024-07-03T20:37:12.347Z
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Photometry from space avoids the turbulent and absorbing terrestrial atmosphere and allows for very long and continuous observing runs with high time resolution and thus provides the data necessary for understanding various processes inside stars (e.g., asteroseismology) and in their immediate environment. While the first astronomical observations from space focused on the spectral regions not accessible from the ground it soon became obvious around 1970 that avoiding the turbulent terrestrial atmosphere significantly improved the accuracy of photometry and satellites explicitly dedicated to high-quality photometry were launched. A perfect example is BRITE-Constellation, which is the result of a very successful cooperation between Austria, Canada and Poland. 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Koudelka</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Catherine C. 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