Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Van Cuyck, M."'
Autor:
Hu, W., Beelen, A., Lagache, G., Fasano, A., Lundgren, A., Ade, P., Aravena, M., Barria, E., Benoit, A., Bethermin, M., Bounmy, J., Bourrion, O., Bres, G., De Breuck, C., Calvo, M., Catalano, A., Desert, F. -X., Dubois, C., Duran, C. A, Fenouillet, T., Garcia, J., Garde, G., Goupy, J., Hoarau, C., Lambert, J. -C., Lellouch, E., Levy-Bertrand, F., Macias-Perez, J., Marpaud, J., Monfardini, A., Pisano, G., Ponthieu, N., Prieur, L., Quinatoa, D., Roni, S., Roudier, S., Tourres, D., Tucker, C., Van Cuyck, M.
Publikováno v:
A&A 689, A20 (2024)
We present the data-processing algorithms and the performance of CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn epoch) in continuum by analysing the data from the commissioning and scientific observations. The beam pattern is charact
Externí odkaz:
http://arxiv.org/abs/2406.15572
Autor:
Van Cuyck, M., Ponthieu, N., Lagache, G., Beelen, A., Béthermin, M., Gkogkou, A., Aravena, M., Benoit, A., Bounmy, J., Calvo, M., Catalano, A., Désert, F. X., Dupé, F. -X., Fasano, A., Ferrara, A., Goupy, J., Hoarau, C., Hu, W., Lambert, J. -C, Macías-Pérez, J. F., Marpaud, J., Mellema, G., Monfardini, A., Pallottini, A.
CONCERTO is the first experiment to perform a [CII] line intensity mapping survey to target $z>5.2$. Measuring the [CII] power spectrum allows us to study the role of dusty star-forming galaxies in the star formation history during the Reionization a
Externí odkaz:
http://arxiv.org/abs/2306.01568
Autor:
Gkogkou, A., Béthermin, M., Lagache, G., Van Cuyck, M., Jullo, E., Aravena, M., Beelen, A., Benoit, A., Bounmy, J., Calvo, M., Catalano, A., Cora, S., Croton, D., de la Torre, S., Fasano, A., Ferrara, A., Goupy, J., Hoarau, C., Hu, W., Ishiyama, T., Knudsen, K. K., Lambert, J. -C., Macías-Pérez, J. F., Marpaud, J., Mellema, G., Monfardini, A., Pallottini, A., Ponthieu, N., Prada, F., Roehlly, Y., Vallini, L., Walter, F.
In the submm regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time. However, both of these two measurements suffer from field-to-field var
Externí odkaz:
http://arxiv.org/abs/2212.02235
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
Akademický článek
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Conference
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Autor:
M. Béthermin, A. Gkogkou, M. Van Cuyck, G. Lagache, A. Beelen, M. Aravena, A. Benoit, J. Bounmy, M. Calvo, A. Catalano, B. de Batz de Trenquelleon, C. De Breuck, A. Fasano, A. Ferrara, J. Goupy, C. Hoarau, C. Horellou, W. Hu, A. Julia, K. Knudsen, J.-C. Lambert, J. Macias-Perez, J. Marpaud, A. Monfardini, A. Pallottini, N. Ponthieu, Y. Roehlly, L. Vallini, F. Walter, A. Weiss
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 667, pp.A156. ⟨10.1051/0004-6361/202243888⟩
Astron.Astrophys.
Astron.Astrophys., 2022, 667, pp.A156. ⟨10.1051/0004-6361/202243888⟩
Astronomy and Astrophysics-A&A, 2022, 667, pp.A156. ⟨10.1051/0004-6361/202243888⟩
Astron.Astrophys.
Astron.Astrophys., 2022, 667, pp.A156. ⟨10.1051/0004-6361/202243888⟩
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc6451f01df425b7ceb38c859a7c6ada
https://doi.org/10.1051/0004-6361/202243888
https://doi.org/10.1051/0004-6361/202243888
