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...
Ausführliche Beschreibung
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] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2021 |
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Schlagwörter: |
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Übergeordnetes Werk: |
In: Universe - MDPI AG, 2015, 7(2021), 6, p 199 |
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Übergeordnetes Werk: |
volume:7 ; year:2021 ; number:6, p 199 |
Links: |
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DOI / URN: |
10.3390/universe7060199 |
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Katalog-ID: |
DOAJ031442781 |
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10.3390/universe7060199 doi (DE-627)DOAJ031442781 (DE-599)DOAJea1eaae50a7a49ed95580ffc7e659ca9 DE-627 ger DE-627 rakwb eng QC793-793.5 Werner W. Weiss verfasserin aut Space Photometry with Brite-Constellation 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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. space photometry stellar structure stellar evolution stellar environment nanosatellites Elementary particle physics Konstanze Zwintz verfasserin aut Rainer Kuschnig verfasserin aut Gerald Handler verfasserin aut Anthony F. J. Moffat verfasserin aut Dietrich Baade verfasserin aut Dominic M. Bowman verfasserin aut Thomas Granzer verfasserin aut Thomas Kallinger verfasserin aut Otto F. Koudelka verfasserin aut Catherine C. Lovekin verfasserin aut Coralie Neiner verfasserin aut Herbert Pablo verfasserin aut Andrzej Pigulski verfasserin aut Adam Popowicz verfasserin aut Tahina Ramiaramanantsoa verfasserin aut Slavek M. Rucinski verfasserin aut Klaus G. Strassmeier verfasserin aut Gregg A. Wade verfasserin aut In Universe MDPI AG, 2015 7(2021), 6, p 199 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:7 year:2021 number:6, p 199 https://doi.org/10.3390/universe7060199 kostenfrei https://doaj.org/article/ea1eaae50a7a49ed95580ffc7e659ca9 kostenfrei https://www.mdpi.com/2218-1997/7/6/199 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 7 2021 6, p 199 |
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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@@ |
publishDateDaySort_date |
2021-01-01T00:00:00Z |
hierarchy_top_id |
820684236 |
id |
DOAJ031442781 |
language_de |
englisch |
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Space Photometry with Brite-Constellation |
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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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Space Photometry with Brite-Constellation |
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