CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

Autor: Bethermin, M., Gkogkou, A., Van Cuyck, M., Lagache, G., Beelen, A., Aravena, M., Benoit, A., Bounmy, J., Calvo, M., Catalano, A., de Trenquelleon, B. de Batz, De Breuck, C., Fasano, A., Ferrara, A., Goupy, J., Hoarau, C., Horellou, C., Hu, W., Julia, A., Knudsen, K., Lambert, J. -C., Macias-Perez, J., Marpaud, J., Monfardini, A., Pallottini, A., Ponthieu, N., Roehlly, Y., Vallini, L., Walter, F., Weiss, A.

Publikováno v: A&A 667, A156 (2022)

The intensity mapping of the [CII] 158um line redshifted to the sub-mm window is a promising probe of the z>4 star formation and its spatial distribution into the large-scale structure. To prepare the first-generation experiments (e.g., CONCERTO), we

Externí odkaz: http://arxiv.org/abs/2204.12827

The MiMeS survey of magnetism in massive stars

Autor: Torsten Böhm, Alex C. Carciofi, Raman K. Prinja, Colin P. Folsom, Rodolfo H. Barbá, Lex Kaper, B. de Batz, Jean-François Donati, J. C. Bouret, Werner W. Weiss, J. Braithwaite, David A. Bohlender, John D. Landstreet, Fabrice Martins, A. F. J. Moffat, W. L. F. Marcolino, Mary E. Oksala, Richard Ignace, Coralie Neiner, J. O. Sundqvist, C. Catala, N. St. Louis, I. Yakunin, A. Blazère, Yaël Nazé, B. Leroy, Lilia Ferrario, Alexander W. Fullerton, Evelyne Alecian, Stanley P. Owocki, Richard H. D. Townsend, Stefano Bagnulo, J. D. Bailey, David H. Cohen, Stéphane Mathis, Theresa Lüftinger, Alexandre David-Uraz, Gregg A. Wade, Th. Rivinius, Jason Grunhut, Nadine Manset, D. Harrington, Matt Shultz, Jorick S. Vink, Michel Aurière, Oleg Kochukhov, Véronique Petit, Maryline Briquet, Asif ud-Doula, Huib F. Henrichs, I. D. Howarth

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2015, 456 (1), pp.2-22. ⟨10.1093/mnras/stv2568⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 456 (1), pp.2-22. ⟨10.1093/mnras/stv2568⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Monthly Notices of the Royal Astronomical Society, 456(1), 2-22. Oxford University Press

The MiMeS project is a large-scale, high resolution, sensitive spectropolarimetric investigation of the magnetic properties of O and early B type stars. Initiated in 2008 and completed in 2013, the project was supported by 3 Large Program allocations

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9c10efa217e78bb2b2e26914ea8d0f9
https://ui.adsabs.harvard.edu/abs/2016MNRAS.456....2W/abstract

An investigation of the magnetic properties of the classical Be star ω Ori by the MiMeS Collaboration

Autor: John D. Landstreet, Véronique Petit, Juan Gutiérrez-Soto, Gregg A. Wade, B. de Batz, Asif ud-Doula, A. L. Huat, F. Cochard, Jason Grunhut, Coralie Neiner

Publikováno v: Monthly Notices of the Royal Astronomical Society. 426:2738-2750

One hundred and twenty-five new high-precision spectropolarimetric observations have been obtained with ESPaDOnS (Eschelle Spectro-Polarimetric Device for the Observation of Stars) at the Canada–France–Hawaii Telescope and Narval at Telescope Ber

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::99d2b17ded4c3c4d1efe84c992c5e58d
https://doi.org/10.1111/j.1365-2966.2012.21833.x

Low-amplitude variations detected by CoRoT in the B8IIIe star HD 175869

Autor: M. Auvergne, A. L. Huat, B. de Batz, O. Thizy L. Andrade, Y. Frémat, J. Suso, Eduardo Janot-Pacheco, T. Semaan, Juan Gutiérrez-Soto, R. Garrido, Michele Floquet, R. Samadi, Marcelo Emilio, Coralie Neiner, Juan Fabregat, F. Espinosa Lara, B. Leroy, Anne-Marie Hubert, P. D. Diago, Christophe Martayan, S. Chaintreuil, C. Catala, Eric Michel

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2009, 506, pp.133-141. ⟨10.1051/0004-6361/200911915⟩

International audience; Context: The origin of the short-term variability in Be stars remains a matter of controversy. Pulsations and rotational modulation are the components of the favored hypothesis. Aims: We present our analysis of CoRoT data of t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b1114c1664ad157759626154142fc5e
https://doi.org/10.1051/0004-6361/200911915

Erratum: An investigation of the magnetic properties of the classical Be star ω Ori by the MiMeS Collaboration

Autor: Juan Gutiérrez-Soto, F. Cochard, Véronique Petit, Jason Grunhut, A. L. Huat, Gregg A. Wade, C. Neiner, John D. Landstreet, Asif ud-Doula, B. de Batz

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 436 (1), pp.943-943. ⟨10.1093/mnras/stt1554⟩
Monthly Notices of the Royal Astronomical Society, 2013, 436 (1), pp.943-943. ⟨10.1093/mnras/stt1554⟩

International audience

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::150109c910643dd5937759ae5ad5c894
https://hal.archives-ouvertes.fr/hal-02539933