Zobrazeno 1 - 10
of 455
pro vyhledávání: '"Faccioli, L"'
Autor:
Adam, R., Ricci, M., Eckert, D., Ade, P., Ajeddig, H., Altieri, B., André, P., Artis, E., Aussel, H., Beelen, A., Benoist, C., Benoît, A., Berta, S., Bing, L., Birkinshaw, M., Bourrion, O., Boutigny, D., Bremer, M., Calvo, M., Cappi, A., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Faccioli, L., Ferrari, C., Gastaldello, F., Giles, P., Gomez, A., Goupy, J., Hahn, O., Hanser, C., Horellou, C., Kéruzoré, F., Koulouridis, E., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S., Maughan, B., Maurogordato, S., Maury, A., Mauskopf, P., Monfardini, A., Muñoz-Echeverría, M., Pacaud, F., Perotto, L., Pierre, M., Pisano, G., Pompei, E., Ponthieu, N., Revéret, V., Rigby, A., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Sereno, M., Schuster, K., Sievers, A., TintoréVidal, G., Tucker, C., Zylka, R.
Three galaxy clusters selected from the XXL X-ray survey at high redshift and low mass ($z\sim1$ and $M_{500} \sim 1-2 \times 10^{14}$ M$_{\odot}$) were observed with NIKA2 to image their Sunyaev-Zel'dovich effect (SZ) signal. They all present an SZ
Externí odkaz:
http://arxiv.org/abs/2310.06373
Autor:
Adam, R., Ricci, M., Eckert, D., Ade, P., Ajeddig, H., Altieri, B., André, P., Artis, E., Aussel, H., Beelen, A., Benoist, C., Benoît, A., Berta, S., Bing, L., Birkinshaw, M., Bourrion, O., Boutigny, D., Bremer, M., Calvo, M., Cappi, A., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Faccioli, L., Ferrari, C., Gastaldello, F., Giles, P., Gomez, A., Goupy, J., Hahn, O., Hanser, C., Horellou, C., Kéruzoré, F., Koulouridis, E., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S., Maughan, B., Maurogordato, S., Maury, A., Mauskopf, P., Monfardini, A., Muñoz-Echeverría, M., Pacaud, F., Perotto, L., Pierre, M., Pisano, G., Pompei, E., Ponthieu, N., Revéret, V., Rigby, A., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Sereno, M., Schuster, K., Sievers, A., Vidal, G. Tintoré, Tucker, C., Zylka, R.
Publikováno v:
A&A 684, A18 (2024)
The thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in galaxy clusters. At low masses ($\sim 10^{14}$ M$_{\odot}$) and high re
Externí odkaz:
http://arxiv.org/abs/2310.05819
Autor:
Koulouridis, E., Clerc, N., Sadibekova, T., Chira, M., Drigga, E., Faccioli, L., Fèvre, J. P. Le, Garrel, C., Gaynullina, E., Gkini, A., Kosiba, M., Pacaud, F., Pierre, M., Ridl, J., Tazhenova, K., Adami, C., Altieri, B., Baguley, J. -C., Cabanac, R., Cucchetti, E., Khalikova, A., Lieu, M., Melin, J. -B., Molham, M., Ramos-Ceja, M. E., Soucail, G., Takey, A., Valtchanov, I.
Cosmological probes based on galaxy clusters rely on cluster number counts and large-scale structure information. X-ray cluster surveys are well suited for this purpose, since they are far less affected than optical surveys by projection effects, and
Externí odkaz:
http://arxiv.org/abs/2104.06617
Autor:
Willis, J. P., Oguri, M., Ramos-Ceja, M. E., Gastaldello, F., Sereno, M., Adami, C., Alis, S., Altieri, B., Chiappetti, L., Corasaniti, P. S., Eckert, D., Ettori, S., Garrel, C., Giles, P., Lefevre, J., Faccioli, L., Fotopoulou, S., Hamabata, A., Koulouridis, E., Lieu, M., Lin, Y. -T., Maughan, B., Nishizawa, A. J., Okabe, T., Okabe, N., Pacaud, F., Paltani, S., Pierre, M., Plionis, M., Poggianti, B., Pompei, E., Sadibekova, T., Umetsu, K., Valageas, P.
Large samples of galaxy clusters provide knowledge of both astrophysics in the most massive virialised environments and the properties of the cosmological model that defines our Universe. However, an important issue that affects the interpretation of
Externí odkaz:
http://arxiv.org/abs/2103.13434
Autor:
Trudeau, A., Garrel, C., Willis, J., Pierre, M., Gastaldello, F., Chiappetti, L., Ettori, S., Umetsu, K., Adami, C., Adams, N., Bowler, R. A. A., Faccioli, L., Häußler, B., Jarvis, M., Koulouridis, E., Fevre, J. P. Le, Pacaud, F., Poggianti, B., Sadibekova, T.
Publikováno v:
A&A 642, A124 (2020)
Context. Distant galaxy clusters provide an effective laboratory in which to study galaxy evolution in dense environments and at early cosmic times. Aims. We aim to identify distant galaxy clusters as extended X-ray sources coincident with overdensit
Externí odkaz:
http://arxiv.org/abs/2009.04049
Autor:
Ricci, M., Adam, R., Eckert, D., Ade, P., André, P., Andrianasolo, A., Altieri, B., Aussel, H., Beelen, A., Benoist, C., Benoît, A., Berta, S., Bideaud, A., Birkinshaw, M., Bourrion, O., Boutigny, D., Bremer, M., Calvo, M., Cappi, A., Chiappetti, L., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Faccioli, L., Ferrari, C., Fotopoulou, S., Gastaldello, F., Giles, P., Gomez, A., Goupy, J., Hahn, O., Horellou, C., Kéruzoré, F., Koulouridis, E., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Mantz, A., Maughan, B., Maurogordato, S., Mauskopf, P., Monfardini, A., Pacaud, F., Perotto, L., Pierre, M., Pisano, G., Pompei, E., Ponthieu, N., Revéret, V., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Portal, M. Sánchez, Schuster, K., Sereno, M., Shu, S., Sievers, A., Tucker, C., Umetsu, K.
Publikováno v:
A&A 642, A126 (2020)
In this paper, we present resolved observations of the Sunyaev-Zel'dovich (SZ) effect, obtained with the NIKA2 camera, towards the cluster of galaxies XLSSC102, a relatively low-mass system ($M_{500} \sim 2 \times 10^{14}$ M$_{\odot}$) at $z = 0.97$
Externí odkaz:
http://arxiv.org/abs/2004.07866
Autor:
Adam R., Ricci M., Eckert D., Ade P., Ajeddig H., Altieri B., André P., Artis E., Aussel H., Beelen A., Benoist C., Benoît A., Berta S., Bing L., Birkinshaw M., Bourrion O., Boutigny D., Bremer M., Calvo M., Cappi A., Catalano A., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Faccioli L., Ferrari C., Gastaldello F., Giles P., Gomez A., Goupy J., Hahn O., Hanser C., Horellou C., Kéruzoré F., Koulouridis E., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Madden S., Maughan B., Maurogordato S., Maury A., Mauskopf P., Monfardini A., Muñoz-Echeverría M., Pacaud F., Perotto L., Pierre M., Pisano G., Pompei E., Ponthieu N., Revéret V., Rigby A., Ritacco A., Romero C., Roussel H., Ruppin F., Sereno M., Schuster K., Sievers A., Vidal G. Tintoré, Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 293, p 00002 (2024)
Three galaxy clusters selected from the XXL X-ray survey at high redshift and low mass (z ~ 1 and M500 ~ 1 – 2 × 1014 M⊙) were observed with NIKA2 to image their Sunyaev-Zel'dovich effect (SZ) signal. They all present an SZ morphology, together
Externí odkaz:
https://doaj.org/article/7cd96fa3f3224506bd8ec88961fc51ff
Autor:
Chiappetti, L., Fotopoulou, S., Lidman, C., Faccioli, L., Pacaud, F., Elyiv, A., Paltani, S., Pierre, M., Plionis, M., Adami, C., Alis, S., Altieri, B., Baldry, I., Bolzonella, M., Bongiorno, A., Brown, M., Driver, S., Elmer, E., Franzetti, P., Grootes, M., Guglielmo, V., Iovino, A., Koulouridis, E., Lefevre, J. P., Liske, J., Maurogordato, S., Melnyk, O., Owers, M., Poggianti, B., Polletta, M., Pompei, E., Ponman, T., Robotham, A., Sadibekova, T., Tuffs, R., Valtchanov, I., Vignali, C., Wagner, G.
We present the version of the point source catalogue of the XXL Survey that was used, in part, in the first series of XXL papers. In this paper we release, in our database in Milan and at CDS: (i) the X-ray source catalogue with 26056 objects in two
Externí odkaz:
http://arxiv.org/abs/1810.03929
Autor:
Adami, C., Giles, P., Koulouridis, E., Pacaud, F., Caretta, C. A., Pierre, M., Eckert, D., Ramos-Ceja, M. E., Gastaldello, F., Fotopoulou, S., Guglielmo, V., Lidman, C., Sadibekova, T., Iovino, A., Maughan, B., Chiappetti, L., Alis, S., Altieri, B., Baldry, I., Bottini, D., Birkinshaw, M., Bremer, M., Brown, M., Cucciati, O., Driver, S., Elmer, E., Ettori, S., Evrard, A. E., Faccioli, L., Granett, B., Grootes, M., Guzzo, L., Hopkins, A., Horellou, C., Lef, J. P., Liske, J., Malek, K., Marulli, F., Maurogordato, S., Owers, M., Paltani, S., Poggianti, B., Polletta, M., Plionis, M., Pollo, A., Pompei, E., Ponman, T., Rapetti, D., Ricci, M., Robotham, A., Tuffs, R., Tasca, L., Valtchanov, I., Vergani, D., Wagner, G., Willis, J., consortium, the XXL
In the currently debated context of using clusters of galaxies as cosmological probes, the need for well-defined cluster samples is critical. The XXL Survey has been specifically designed to provide a well characterised sample of some 500 X-ray detec
Externí odkaz:
http://arxiv.org/abs/1810.03849
Autor:
Pacaud, F., Pierre, M., Melin, J. -B., Adami, C., Evrard, A. E., Galli, S., Gastaldello, F., Maughan, B. J., Sereno, M., Alis, S., Altieri, B., Birkinshaw, M., Chiappetti, L., Faccioli, L., Giles, P. A., Horellou, C., Iovino, A., Koulouridis, E., Fèvre, J. -P. Le, Lidman, C., Lieu, M., Maurogordato, S., Moscardini, L., Poggianti, B. M., Pompei, E., Sadibekova, T., Valtchanov, I., Willis, J. P.
Context. We present an estimation of cosmological parameters with clusters of galaxies. Aims. We constrain the $\Omega_m$, $\sigma_8$, and $w$ parameters from a stand-alone sample of X-ray clusters detected in the 50 deg$^2$ XMM-XXL survey with a wel
Externí odkaz:
http://arxiv.org/abs/1810.01624