Zobrazeno 1 - 4
of 4
pro vyhledávání: '"de La Vernhe, Isaure González Rivera"'
Autor:
de La Vernhe, Isaure González Rivera, Hill, Vanessa, Kordopatis, Georges, Gran, Felipe, Fernández-Alvar, Emma, Ardern-Arentsen, Anke, Thomas, Guillaume F., Sestito, Federico, Navarrete, Camila, Martin, Nicolas F., Starkenburg, Else, Viswanathan, Akshara, Battaglia, Giuseppina, Venn, Kim A., Vitali, Sara
Through the chemodynamical characterisation of metal-poor stars, one can efficiently probe the early history of the Milky Way. We aim at decontaminating a sample of $\sim$ 3M giant stars with Gaia DR3 XP-based \textit{Pristine-Gaia} metallicities, to
Externí odkaz:
http://arxiv.org/abs/2406.05728
Autor:
Fernández-Alvar, Emma, Kordopatis, Georges, Hill, Vanessa, Battaglia, Giuseppina, Gallart, Carme, de la Vernhe, Isaure González Rivera, Thomas, Guillaume, Sestito, Federico, Ardern-Arentsen, Anke, Martin, Nicolas, Viswanathan, Akshara, Starkenburg, Else
Publikováno v:
A&A 685, A151 (2024)
The emergence of the disc in our Galaxy and the relation of the thick and thin disc formation and evolution is still a matter of debate. The chemo-dynamical characterization of disc stars is key to resolve this question, in particular at parameter re
Externí odkaz:
http://arxiv.org/abs/2402.02943
Autor:
Martin, Nicolas F., Starkenburg, Else, Yuan, Zhen, Fouesneau, Morgan, Ardern-Arentsen, Anke, De Angeli, Francesca, Gran, Felipe, Montelius, Martin, Rusterucci, Samuel, Andrae, René, Bellazzini, Michele, Montegriffo, Paolo, Esselink, Anna F., Zhang, Hanyuan, Venn, Kim A., Viswanathan, Akshara, Aguado, David S., Battaglia, Giuseppina, Bayer, Manuel, Bonifacio, Piercarlo, Caffau, Elisabetta, Côté, Patrick, Carlberg, Raymond, Fabbro, Sébastien, Alvar, Emma Fernández, Hernández, Jonay I. González, de La Vernhe, Isaure González Rivera, Hill, Vanessa, Ibata, Rodrigo A., Jablonka, Pascale, Kordopatis, Georges, Lardo, Carmela, McConnachie, Alan W., Navarrete, Camila, Navarro, Julio, Recio-Blanco, Alejandra, Janssen, Rubén Sánchez, Sestito, Federico, Thomas, Guillaume F., Vitali, Sara, Youakim, Kristopher
We used the spectro-photometric information of ~219 million stars from Gaia's DR3 to calculate synthetic, narrow-band, metallicity-sensitive CaHK magnitudes that mimic the observations of the Pristine survey, a survey of photometric metallicities of
Externí odkaz:
http://arxiv.org/abs/2308.01344
Akademický článek
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