Zobrazeno 1 - 10
of 3 239
pro vyhledávání: '"Hanser, A."'
Autor:
Hanser, Kelsey, Mayers, Nicholas
Lascoux polynomials are a class of nonhomogeneous polynomials which form a basis of the full polynomial ring. Recently, Pan and Yu showed that Lascoux polynomials can be defined as generating polynomials for certain collections of diagrams consisting
Externí odkaz:
http://arxiv.org/abs/2410.03916
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:
Paliwal, A., Cui, W., de Andrés, D., De Petris, M., Ferragamo, A., Hanser, C., Macías-Pérez, J. -F., Mayet, F., Moyer-Anin, A., Muñoz-Echeverría, M., Perotto, L., Rasia, E., Yepes, G.
The abundance of galaxy clusters with mass and redshift is a well-known cosmological probe. The cluster mass is a key parameter for studies that aim to constrain cosmological parameters using galaxy clusters, making it critical to understand and prop
Externí odkaz:
http://arxiv.org/abs/2404.03376
Extended-connectivity fingerprints (ECFPs) are a ubiquitous tool in current cheminformatics and molecular machine learning, and one of the most prevalent molecular feature extraction techniques used for chemical prediction. Atom features learned by g
Externí odkaz:
http://arxiv.org/abs/2403.17954
Autor:
Muñoz-Echeverría, M., Macías-Pérez, J. F., Pratt, G. W., Pointecouteau, E., Bartalucci, I., De Petris, M., Ferragamo, A., Hanser, C., Kéruzoré, F., Mayet, F., Moyer-Anin, A., Paliwal, A., Perotto, L., Yepes, G.
Publikováno v:
Astronomy & Astrophysics, Volume 682, id.A147, 27 pp., February 2024
An accurate reconstruction of galaxy cluster masses is key to use this population of objects as a cosmological probe. In this work we present a study on the hydrostatic-to-lensing mass scaling relation for a sample of 53 clusters whose masses were re
Externí odkaz:
http://arxiv.org/abs/2312.01154
Autor:
Nguyen-Luong, Q., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., 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., Monfardini, A., Moyer-Anin, A., Muñoz-Echeverría, M., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Tucker, C., Zylka, R., Bacmann, A., Duong-Tuan, A., Peretto, N., Rigby, A.
To understand the evolution of dust properties in molecular clouds in the course of the star formation process, we constrain the changes in the dust emissivity index from star-forming filaments to prestellar and protostellar cores to T Tauri stars. U
Externí odkaz:
http://arxiv.org/abs/2310.16526
Weak gravitational lensing is an important tool to estimate the masses of galaxy clusters, as it allows us to directly access their projected surface mass density along the line-of-sight (LOS) in a manner largely independent of their dynamical state.
Externí odkaz:
http://arxiv.org/abs/2310.08175
Autor:
Hanser, C., 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 Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., Ferragamo, A., Gomez, A., Goupy, J., 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., Paliwal, A., Payerne, C., 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.
High-resolution mapping of the hot gas in galaxy clusters is a key tool for cluster-based cosmological analyses. Taking advantage of the NIKA2 millimeter camera operated at the IRAM 30-m telescope, the NIKA2 SZ Large Program seeks to get a high-resol
Externí odkaz:
http://arxiv.org/abs/2310.07400
Autor:
Pantoni, L., 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 Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., 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., Paradis, D., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Smith, M. W. S. L., Tabatabaei, F. S., Tedros, J., Tucker, C., Xilouris, E. M., Zylka, R.
Publikováno v:
EPJ Web of Conferences 293 (2024) 00038
We present the first preliminary results of the project \textit{ICED}, focusing on the face-on galaxy NGC4254. We use the millimetre maps observed with NIKA2 at IRAM-30m, as part of the IMEGIN Guaranteed Time Large Program, and of a wide collection o
Externí odkaz:
http://arxiv.org/abs/2310.06463
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