Zobrazeno 1 - 10
of 824
pro vyhledávání: '"Lambert J. C."'
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:
Zavagno, A., Dupé, F. -X., Bensaid, S., Schisano, E., Causi, G. Li, Gray, M., Molinari, S., Elia, D., Lambert, J. -C., Brescia, M., Arzoumanian, D., Russeil, D., Riccio, G., Cavuoti, S.
Publikováno v:
A&A 669, A120 (2023)
Context. Filaments are ubiquitous in the Galaxy, and they host star formation. Detecting them in a reliable way is therefore key towards our understanding of the star formation process. Aims. We explore whether supervised machine learning can identif
Externí odkaz:
http://arxiv.org/abs/2212.00463
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
Autor:
Catalano, A., Ade, P., Aravena, M., Barria, E., Beelen, A., Benoit, A., Béthermin, M., Bounmy, J., Bourrion, O., Bres, G., De Breuck, C., Calvo, M., Désert, F. -X., Duràn, C. A, Duvauchelle, G., Eraud, L., Fasano, A., Fenouillet, T., Garcia, J., Garde, G., Goupy, J., Groppi, C., Hoarau, C., Hu, W., Lagache, G., Lambert, J. -C., Leggeri, J. -P., Levy-Bertrand, F., Macìas-Pérez, J., Mani, H., Marpaud, J., Marton, M., Mauskopf, P., Monfardini, A., Pisano, G., Ponthieu, N., Prieur, L., Raffin, G., Roni, S., Roudier, S., Tourres, D., Tucker, C., Vivargent, L.
CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn) is a large field-of-view (FoV) spectro-imager that has been installed on the Cassegrain Cabin of Atacama Pathfinder EXperiment (APEX) telescope in April 2021. CONCERTO hosts 2 focal pla
Externí odkaz:
http://arxiv.org/abs/2110.14984
Autor:
Monfardini, A., Beelen, A., Benoit, A., Bounmy, J., Calvo, M., Catalano, A., Goupy, J., Lagache, G., Ade, P., Barria, E., Bethermin, M., Bourrion, O., Bres, G., De Breuck, C., Desert, F. -X., Duvauchelle, G., Fasano, A., Fenouillet, T., Garcia, J., Garde, G., Hoarau, C., Hu, W., Lambert, J. -C., Levy-Bertrand, F., Lundgren, A., Macias-Perez, J., Marpaud, J., Pisano, G., Ponthieu, N., Prieur, L., Roni, S., Roudier, S., Tourres, D., Tucker, C., Cantzler, M., Caro, P., Diaz, M., Duran, C., Montenegro, F., Navarro, M., Olguin, R., Palma, F., Parra, R., Santana, J.
We describe the deployment and first tests on Sky of CONCERTO, a large field-of-view (18.6arc-min) spectral-imaging instrument. The instrument operates in the range 130-310GHz from the APEX 12-meters telescope located at 5100m a.s.l. on the Chajnanto
Externí odkaz:
http://arxiv.org/abs/2106.14028
Autor:
Tang, Z., Watkins, E. B., Clayton, S. M., Currie, S. A., Fellers, D. E., Hassan, Md. T., Hooks, D. E., Ito, T. M., Lawrence, S. K., MacDonald, S. W. T., Makela, M., Morris, C. L., Neukirch, L. P., Saunders, A., O'Shaughnessy, C. M., Cude-Woods, C., Choi, J. H., Young, A. R., Zeck, B. A., Gonzalez, F., Liu, C. Y., Floyd, N. C., Hickerson, K. P., Holley, A. T., Johnson, B. A., Lambert, J. C., Pattie, R. W.
In this paper we report studies of the Fermi potential and loss per bounce of ultracold neutron (UCN) on a deuterated scintillator (Eljen-299-02D). These UCN properties of the scintillator enables a wide variety of applications in fundamental neutron
Externí odkaz:
http://arxiv.org/abs/2009.13517
Autor:
The CONCERTO collaboration, Ade, P., Aravena, M., Barria, E., Beelen, A., Benoit, A., Béthermin, M., Bounmy, J., Bourrion, O., Bres, G., De Breuck, C., Calvo, M., Cao, Y., Catalano, A., Désert, F. -X., Durán, C. A, Fasano, A., Fenouillet, T., Garcia, J., Garde, G., Goupy, J., Groppi, C., Hoarau, C., Lagache, G., Lambert, J. -C., Leggeri, J. -P., Levy-Bertrand, F., Macias-Perez, J., Mani, H., Marpaud, J., Mauskopf, P., Monfardini, A., Pisano, G., Ponthieu, N., Prieur, L., Roni, S., Roudier, S., Tourres, D., Tucker, C.
Publikováno v:
A&A 642, A60 (2020)
Characterise the large-scale structure in the Universe from present times to the high redshift epoch of reionisation is essential to constraining the cosmology, the history of star formation and reionisation, measuring the gas content of the Universe
Externí odkaz:
http://arxiv.org/abs/2007.14246
Autor:
Coroller, H. Le, Nowak, M., Delorme, P., Chauvin, G., Gratton, R., Devinat, M., Bec-Canet, J., Schneeberger, A., Estevez, D., Arnold, L., Beust, H., Bonnefoy, M., Boccaletti, A., Desgrange, C., Desidera, S., Galicher, R., Lagrange, A. M., Langlois, M., Maire, A. L., Menard, F., Vernazza, P., Vigan, A., Zurlo, A., Fenouillet, T., Lambert, J. C., Bonavita, M., Cheetham, A., Dorazi, V., Feldt, M., Janson, M., Ligi, R., Mesa, D., Meyer, M., Samland, M., Sissa, E., Beuzit, J. L., Dohlen, K., Fusco, T., Mignant, D. Le, Mouillet, D., Ramos, J., Rochat, S., Sauvage, J. F.
Publikováno v:
A&A 639, A113 (2020)
Recent high-contrast imaging surveys, looking for planets in young, nearby systems showed evidence of a small number of giant planets at relatively large separation beyond typically 20 au where those surveys are the most sensitive. Access to smaller
Externí odkaz:
http://arxiv.org/abs/2004.12878