Gregor@night: The future high‐resolution stellar spectrograph for the GREGOR solar telescope
Identifieur interne : 000589 ( Main/Exploration ); précédent : 000588; suivant : 000590Gregor@night: The future high‐resolution stellar spectrograph for the GREGOR solar telescope
Auteurs : K. G. Strassmeier [Allemagne] ; I. V. Ilyin [Allemagne] ; M. Woche [Allemagne] ; T. Granzer [Allemagne] ; M. Weber [Allemagne] ; J. Weingrill [Allemagne] ; S. Bauer [Allemagne] ; E. Popow [Allemagne] ; C. Denker [Allemagne] ; W. Schmidt [Allemagne] ; O. Von Der Lühe [Allemagne] ; S. Berdyugina [Allemagne] ; M. Collados [Espagne] ; P. Koubsky [République tchèque] ; T. Hackman [Finlande] ; M. J. Mantere [Finlande]Source :
- Astronomische Nachrichten [ 0004-6337 ] ; 2012-11.
English descriptors
- KwdEn :
Abstract
We describe the future night‐time spectrograph for the GREGOR solar telescope and present its science core projects. The spectrograph provides a 3‐pixel resolution of up to R = 87 000 in 45 échelle orders covering the wavelength range 390‐900 nm with three grating settings. An iodine cell can be used for high‐precision radial velocity work in the 500‐630 nm range. The operation of the spectrograph and the telescope will be fully automated without the presence of humans during night‐time and will be based on the successful STELLA control system. Future upgrades include a second optical camera for even higher spectral resolution, a Stokes‐V polarimeter and a link to the laser‐frequency comb at the Vacuum Tower Telescope. The night‐time core projects are a study of the angular‐momentum evolution of “The Sun in Time” and a continuation of our long‐term Doppler imaging of active stars (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
Url:
DOI: 10.1002/asna.201211727
Affiliations:
- Allemagne, Espagne, Finlande, République tchèque
- Bade-Wurtemberg, Canaries, District de Fribourg-en-Brisgau, Finlande occidentale, Uusimaa
- Fribourg-en-Brisgau, Helsinki, Turku
- Université d'Helsinki, Université de Turku
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Berdyugina</name><affiliation wicri:level="3"><country xml:lang="fr">Allemagne</country><wicri:regionArea>Kiepenheuer‐Institut für Sonnenphysik (KIS), Schöneckstr. 6, D‐79104 Freiburg</wicri:regionArea><placeName><region type="land" nuts="1">Bade-Wurtemberg</region><region type="district" nuts="2">District de Fribourg-en-Brisgau</region><settlement type="city">Fribourg-en-Brisgau</settlement></placeName></affiliation></author><author><name sortKey="Collados, M" sort="Collados, M" uniqKey="Collados M" first="M." last="Collados">M. Collados</name><affiliation wicri:level="2"><country xml:lang="fr">Espagne</country><wicri:regionArea>Instituto de Astrofisica de Canarias (IAC), E‐38200 La Laguna</wicri:regionArea><placeName><region nuts="2" type="communauté">Canaries</region></placeName></affiliation></author><author><name sortKey="Koubsky, P" sort="Koubsky, P" uniqKey="Koubsky P" first="P." last="Koubsky">P. Koubsky</name><affiliation wicri:level="1"><country xml:lang="fr">République tchèque</country><wicri:regionArea>Astronomical Institute, Academy of Sciences, Fričova 298, CR‐25165 Ondřejov</wicri:regionArea><wicri:noRegion>CR‐25165 Ondřejov</wicri:noRegion></affiliation></author><author><name sortKey="Hackman, T" sort="Hackman, T" uniqKey="Hackman T" first="T." last="Hackman">T. Hackman</name><affiliation wicri:level="4"><country xml:lang="fr">Finlande</country><wicri:regionArea>Finnish Centre for Astronomy with ESO (FINCA), University of Turku, Väisäläntie 20, FI‐21500 Piikkiö</wicri:regionArea><orgName type="university">Université de Turku</orgName><placeName><settlement type="city">Turku</settlement><region type="région" nuts="2">Finlande occidentale</region></placeName></affiliation></author><author><name sortKey="Mantere, M J" sort="Mantere, M J" uniqKey="Mantere M" first="M. J." last="Mantere">M. J. Mantere</name><affiliation wicri:level="4"><country xml:lang="fr">Finlande</country><wicri:regionArea>University of Helsinki, Dept. of Physics, Gustaf Hällströminkatu 21, FI‐00014 Helsinki</wicri:regionArea><orgName type="university">Université d'Helsinki</orgName><placeName><settlement type="city">Helsinki</settlement><region type="région" nuts="2">Uusimaa</region></placeName></affiliation></author></analytic><monogr></monogr><series><title level="j">Astronomische Nachrichten</title><title level="j" type="abbrev">Astron. Nachr.</title><idno type="ISSN">0004-6337</idno><idno type="eISSN">1521-3994</idno><imprint><publisher>WILEY‐VCH Verlag</publisher><pubPlace>Berlin</pubPlace><date type="published" when="2012-11">2012-11</date><biblScope unit="volume">333</biblScope><biblScope unit="issue">9</biblScope><biblScope unit="page" from="901">901</biblScope><biblScope unit="page" to="910">910</biblScope></imprint><idno type="ISSN">0004-6337</idno></series><idno type="istex">17400FD90DBD0C3F55740B5EFC4314F6F2648E4B</idno><idno type="DOI">10.1002/asna.201211727</idno><idno type="ArticleID">ASNA201211727</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0004-6337</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>instrumentation: spectrographs</term><term>stars: activity</term><term>stars: rotation</term><term>techniques: spectroscopic</term><term>telescopes</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We describe the future night‐time spectrograph for the GREGOR solar telescope and present its science core projects. The spectrograph provides a 3‐pixel resolution of up to R = 87 000 in 45 échelle orders covering the wavelength range 390‐900 nm with three grating settings. An iodine cell can be used for high‐precision radial velocity work in the 500‐630 nm range. The operation of the spectrograph and the telescope will be fully automated without the presence of humans during night‐time and will be based on the successful STELLA control system. Future upgrades include a second optical camera for even higher spectral resolution, a Stokes‐V polarimeter and a link to the laser‐frequency comb at the Vacuum Tower Telescope. The night‐time core projects are a study of the angular‐momentum evolution of “The Sun in Time” and a continuation of our long‐term Doppler imaging of active stars (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)</div></front></TEI><affiliations><list><country><li>Allemagne</li><li>Espagne</li><li>Finlande</li><li>République tchèque</li></country><region><li>Bade-Wurtemberg</li><li>Canaries</li><li>District de Fribourg-en-Brisgau</li><li>Finlande occidentale</li><li>Uusimaa</li></region><settlement><li>Fribourg-en-Brisgau</li><li>Helsinki</li><li>Turku</li></settlement><orgName><li>Université d'Helsinki</li><li>Université de Turku</li></orgName></list><tree><country name="Allemagne"><noRegion><name sortKey="Strassmeier, K G" sort="Strassmeier, K G" uniqKey="Strassmeier K" first="K. G." last="Strassmeier">K. G. Strassmeier</name></noRegion><name sortKey="Bauer, S" sort="Bauer, S" uniqKey="Bauer S" first="S." last="Bauer">S. Bauer</name><name sortKey="Berdyugina, S" sort="Berdyugina, S" uniqKey="Berdyugina S" first="S." last="Berdyugina">S. Berdyugina</name><name sortKey="Denker, C" sort="Denker, C" uniqKey="Denker C" first="C." last="Denker">C. Denker</name><name sortKey="Granzer, T" sort="Granzer, T" uniqKey="Granzer T" first="T." last="Granzer">T. Granzer</name><name sortKey="Ilyin, I V" sort="Ilyin, I V" uniqKey="Ilyin I" first="I. V." last="Ilyin">I. V. Ilyin</name><name sortKey="Popow, E" sort="Popow, E" uniqKey="Popow E" first="E." last="Popow">E. Popow</name><name sortKey="Schmidt, W" sort="Schmidt, W" uniqKey="Schmidt W" first="W." last="Schmidt">W. Schmidt</name><name sortKey="Von Der Luhe, O" sort="Von Der Luhe, O" uniqKey="Von Der Luhe O" first="O." last="Von Der Lühe">O. Von Der Lühe</name><name sortKey="Weber, M" sort="Weber, M" uniqKey="Weber M" first="M." last="Weber">M. Weber</name><name sortKey="Weingrill, J" sort="Weingrill, J" uniqKey="Weingrill J" first="J." last="Weingrill">J. Weingrill</name><name sortKey="Woche, M" sort="Woche, M" uniqKey="Woche M" first="M." last="Woche">M. Woche</name></country><country name="Espagne"><region name="Canaries"><name sortKey="Collados, M" sort="Collados, M" uniqKey="Collados M" first="M." last="Collados">M. Collados</name></region></country><country name="République tchèque"><noRegion><name sortKey="Koubsky, P" sort="Koubsky, P" uniqKey="Koubsky P" first="P." last="Koubsky">P. Koubsky</name></noRegion></country><country name="Finlande"><region name="Finlande occidentale"><name sortKey="Hackman, T" sort="Hackman, T" uniqKey="Hackman T" first="T." last="Hackman">T. Hackman</name></region><name sortKey="Mantere, M J" sort="Mantere, M J" uniqKey="Mantere M" first="M. J." last="Mantere">M. J. Mantere</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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