Zobrazeno 1 - 10
of 557
pro vyhledávání: '"Ponthieu P"'
Autor:
Paliwal, A., De Petris, M., Ferragamo, A., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Luca, F., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., Gomez, A., Goupy, J., Hanser, C., Katsioli, S., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Melin, J. -B., Monfardini, A., Moyer-Anin, A., Muñoz-Echeverría, M., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G. W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Tucker, C., Wicker, R., Zylka, R.
Having a detailed knowledge of the intracluster medium (ICM) to infer the exact cluster physics such as the cluster dynamical state is crucial for cluster-based cosmological studies. This knowledge limits the accuracy and precision of mass estimation
Externí odkaz:
http://arxiv.org/abs/2410.11668
Autor:
Ejlali, G., Tabatabaei, F. S., Roussel, H., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Baes, M., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Looze, I., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Galliano, F., Gomez, A., Goupy, J., Jones, A. P., Hanser, C., Hughes, A., Katsioli, S., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Moyer-Anin, A., Muñoz-Echeverría, M., Nersesian, A., Pantoni, L., Paradis, D., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Ruppin, F., Schuster, K., Sievers, A., Smith, M. W. L., Tedros, J., Tucker, C., Xilouris, E. M., Ysard, N., Zylka, R.
The millimeter continuum emission from galaxies provides important information about cold dust, its distribution, heating, and role in their InterStellar Medium (ISM). This emission also carries an unknown portion of the free-free and synchrotron rad
Externí odkaz:
http://arxiv.org/abs/2410.09827
Autor:
Macías-Pérez, J. F., Fernández-Torreiro, M., Catalano, A., Fasano, A., Aguiar, M., Beelen, A., Benoit, A., Bideaud, A., Bounmy, J., Bourrion, O., Calvo, M., Castro-Almazán, J. A., de Bernardis, P., de Petris, M., de Taoro, A. P., Garde, G., Génova-Santos, R. T., Gomez, A., Gómez-Renasco, M. F., Goupy, J., Hoarau, C., Hoyland, R., Lagache, G., Marpaud, J., Marton, M., Masi, S., Monfardini, A., Peel, M. W., Pisano, G., Ponthieu, N., Rebolo, R., Roni, S., Roudier, S., Rubiño-Martín, J. A., Tourres, D., Tucker, C., Viera-Curvelo, T., Vescovi, C.
Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimetre range. Their compact size enables to optimally fill the focal plane, thus boosting sensitivity. The KISS (KIDs Inter
Externí odkaz:
http://arxiv.org/abs/2409.20272
Autor:
Moyer-Anin, A., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Bartalucci, I., Beelen, A., Benoît, A., Berta, S., Bing, L., Bolliet, B., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., Ferragamo, A., Gomez, A., Goupy, J., Hanser, C., Katsioli, S., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Melin, J. -B., Monfardini, A., Muñoz-EcheverrÍa, M., Paliwal, A., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Pratt, G. W., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Tucker, C., Yepes, G.
In Sunyaev-Zeldovich (SZ) cluster cosmology, two tools are needed to be able to exploit data from large scale surveys in the millimeter-wave domain. An accurate description of the IntraCluster Medium (ICM) pressure profile is needed along with the sc
Externí odkaz:
http://arxiv.org/abs/2409.00977
Autor:
Fasano, Alessandro, Ade, Peter, Aravena, Manuel, Barria, Emilio, Beelen, Alexandre, Benoit, Alain, Béthermin, Matthieu, Bounmy, Julien, Bourrion, Olivier, Bres, Guillaume, Calvo, Martino, Catalano, Andrea, De Breuck, Carlos, Désert, François-Xavier, Dubois, Cédric, Durán, Carlos, Fenouillet, Thomas, Garcia, Jose, Garde, Gregory, Goupy, Johannes, Hoarau, Christophe, Hu, Wenkai, Lagache, Guilaine, Lambert, Jean-Charles, Levy-Bertrand, Florence, Lundgren, Andreas, Macías-Pérez, Juan-Francisco, Marpaud, Julien, Monfardini, Alessandro, Pisano, Giampaolo, Ponthieu, Nicolas, Prieur, Leo, Roni, Samuel, Roudier, Sebastien, Tourres, Damien, Tucker, Carol, Van Cuyck, Mathilde
Modern astrophysics relies on intricate instrument setups to meet the demands of sensitivity, sky coverage, and multi-channel observations. An example is the CONCERTO project, employing advanced technology like kinetic inductance detectors and a Mart
Externí odkaz:
http://arxiv.org/abs/2406.16334
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:
Ritacco, A., Bizzarri, L., Savorgnano, S., Boulanger, F., Pérault, M., Treuttel, J., Morfin, P., Catalano, A., Darson, D., Ponthieu, N., Feret, A., Maffei, B., Chahadih, A., Pisano, G., Zannoni, M., Nati, F., Macías-Pérez, J. F., Monfardini, A., Calvo, M., Murgia, M., Ortu, P., Pisanu, T., Aumont, J., Errard, J., Leclercq, S., Migliaccio, M.
The cosmic microwave background (CMB), a remnant of the Big Bang, provides unparalleled insights into the primordial universe, its energy content, and the origin of cosmic structures. The success of forthcoming terrestrial and space experiments hinge
Externí odkaz:
http://arxiv.org/abs/2405.12135
Autor:
Bing, L. -J., Beelen, A., Lagache, G., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Benoît, A., Berta, S., Béthermin, M., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Gomez, A., Goupy, J., Kéruzoré, F., Kramer, C., Ladjelate, B., Leclercq, S., Liu, D. -Z., Lestrade, J. -F., Macías-Pérez, J. F., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Muñoz-Echeverría, M., Neri, R., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Shu, S., Sievers, A., Tucker, C., Xiao, M. -Y., Zylka, R.
We develop a new framework to constrain the source redshift. The method jointly accounts for the detection/non-detection of spectral lines and the prior information from the photometric redshift and total infrared luminosity from spectral energy dist
Externí odkaz:
http://arxiv.org/abs/2403.00911
Autor:
Désert, François-Xavier, Calvo, Martino, Catalano, Andrea, Leclercq, Samuel, Macias-Perez, Juan, Mayet, Frédéric, Monfardini, Alessandro, Perotto, Laurence, Ponthieu, Nicolas
Publikováno v:
EPJ Web Conf. 293 00014 (2024)
There are several new projects to survey the sky with millimetre eyes, the biggest being Simons Observatory and CMB-S4, in the Southern Hemisphere. The NIKA2 collaboration has acquired sufficient knowledge to build a large focal plane KID camera for
Externí odkaz:
http://arxiv.org/abs/2402.00520
Autor:
Ritacco, A., Bizzarri, L., Boulanger, F., Pérault, M., Aumont, J., Bouchet, F., Calvo, M., Catalano, A., Darson, D., Désert, F. X., Errard, J., Feret, A., Macías-Pérez, J. F., Maffei, B., Monfardini, A., Montier, L., Murgia, M., Morfin, P., Nati, F., Pisano, G., Ponthieu, N., Puget, J. L., Savorgnano, S., Segret, B., Schuster, K., Treuttel, J., Zannoni, M.
The Cosmic Microwave Background (CMB) radiation offers a unique window into the early Universe, facilitating precise examinations of fundamental cosmological theories. However, the quest for detecting B-modes in the CMB, predicted by theoretical mode
Externí odkaz:
http://arxiv.org/abs/2311.08307