Zobrazeno 1 - 10
of 409
pro vyhledávání: '"Mroczkowski, T."'
Autor:
Marini, I., Popesso, P., Lamer, G., Dolag, K., Biffi, V., Vladutescu-Zopp, S., Dev, A., Toptun, V., Bulbul, E., Comparat, J., Malavasi, N., Merloni, A., Mroczkowski, T., Ponti, G., Seppi, R., Shreeram, S., Zhang, Y.
The eROSITA will deliver an unprecedented volume of X-ray survey observations, 20-30 times more sensitive than ROSAT in the soft band (0.5-2 keV) and for the first time imaging in the hard band (2-10 keV) including galaxy clusters and groups along wi
Externí odkaz:
http://arxiv.org/abs/2404.12719
Autor:
Sikhosana, S. P., Hilton, M., Bernardi, G., Kesebonye, K., Klutse, D. Y., Knowles, K., Moodley, K., Mroczkowski, T., Partridge, B., Sifón, C., Vargas, C., Wollack, E.
In the current paradigm, high redshift radio halos are expected to be scarce due to inverse Compton energy losses and redshift dimming, which cause them to be intrinsically faint. This low occurrence fraction is predicted by cosmic ray electron turbu
Externí odkaz:
http://arxiv.org/abs/2404.03944
Autor:
van Marrewijk, J., Morris, T. W., Mroczkowski, T., Cicone, C., Dicker, S., Di Mascolo, L., Haridas, S. K., Orlowski-Scherer, J., Rasia, E., Romero, C.
Submillimeter single-dish telescopes offer two key advantages compared to interferometers: they can efficiently map larger portions of the sky and recover larger spatial scales. Nonetheless, fluctuations in the atmosphere limit the accurate retrieval
Externí odkaz:
http://arxiv.org/abs/2402.10731
Autor:
Lepore, M., Di Mascolo, L., Tozzi, P., Churazov, E., Mroczkowski, T., Borgani, S., Carilli, C., Gaspari, M., Ginolfi, M., Liu, A., Pentericci, L., Rasia, E., Rosati, P., Röttgering, H. J. A., Anderson, C. S., Dannerbauer, H., Miley, G., Norman, C.
We present the detailed analysis of the thermal, diffuse emission of the proto-intracluster medium (ICM) detected in the halo of the Spiderweb Galaxy at z=2.16, within a radius of $\sim$ 150 kpc. We combined deep X-ray data from Chandra and millimete
Externí odkaz:
http://arxiv.org/abs/2312.06392
Autor:
van Marrewijk, J., Di Mascolo, L., Gill, A. S., Battaglia, N., Battistelli, E. S., Bond, J. R., Devlin, M. J., Doze, P., Dunkley, J., Knowles, K., Hincks, A., Hughes, J. P., Hilton, M., Moodley, K., Mroczkowski, T., Naess, S., Partridge, B., Popping, G., Sifón, C., Staggs, S. T., Wollack, E. J.
How protoclusters evolved from sparse galaxy overdensities to mature galaxy clusters is still not well understood. In this context, detecting and characterizing the hot ICM at high redshifts (z~2) is key to understanding how the continuous accretion
Externí odkaz:
http://arxiv.org/abs/2310.06120
Autor:
Anbajagane, D., Chang, C., Baxter, E. J., Charney, S., Lokken, M., Aguena, M., Allam, S., Alves, O., Amon, A., An, R., Andrade-Oliveira, F., Bacon, D., Battaglia, N., Bechtol, K., Becker, M. R., Benson, B. A., Bernstein, G. M., Bleem, L., Bocquet, S., Bond, J. R., Brooks, D., Rosell, A. Carnero, Kind, M. Carrasco, Chen, R., Choi, A., Costanzi, M., Crawford, T. M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Davis, T. M., De Vicente, J., Desai, S., Devlin, M. J., Diehl, H. T., Doel, P., Doux, C., Drlica-Wagner, A., Elvin-Poole, J., Ferrero, I., Ferte, A., Flaugher, B., Fosalba, P., Friedel, D., Frieman, J., Garcia-Bellido, J., Gatti, M., Giannini, G., Grandis, S., Gruen, D., Gruendl, R. A., Gutierrez, G., Harrison, I., Hill, J. C., Hilton, M., Hinton, S. R., Hollowood, D. L., Honscheid, K., Jain, B., James, D. J., Jarvis, M., Kuehn, K., Lin, M., MacCrann, N., Marshall, J. L., McCullough, J., McMahon, J. J., Mena-Fernandez, J., Menanteau, F., Miquel, R., Moodley, K., Mroczkowski, T., Myles, J., Naess, S., Navarro-Alsina, A., Ogando, R. L. C., Page, L. A., Palmese, A., Pandey, S., Patridge, B., Pieres, A., Malagon, A. A. Plazas, Porredon, A., Prat, J., Reichardt, C., Reil, K., Rodriguez-Monroy, M., Rollins, R. P., Romer, A. K., Rykoff, E. S., Sanchez, E., Sanchez, C., Cid, D. Sanchez, Schaan, E., Schubnell, M., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Sifon, C., Smith, M., Staggs, S. T., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Troxel, M. A., Tutusaus, I., Vavagiakis, E. M., Weaverdyck, N., Weller, J., Wiseman, P., Wollack, E. J., Yanny, B.
We search for signatures of cosmological shocks in gas pressure profiles of galaxy clusters using the cluster catalogs from three surveys: the Dark Energy Survey (DES) Year 3, the South Pole Telescope (SPT) SZ survey, and the Atacama Cosmology Telesc
Externí odkaz:
http://arxiv.org/abs/2310.00059
Autor:
Mallaby-Kay, M., Amodeo, S., Hill, J. C., Aguena, M., Allam, S., Alves, O., Annis, J., Battaglia, N., Battistelli, E. S., Baxter, E. J., Bechtol, K., Becker, M. R., Bertin, E., Bond, J. R., Brooks, D., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Choi, A., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Doux, C., Drlica-Wagner, A., Dunkley, J., Elvin-Poole, J., Everett, S., Ferraro, S., Ferrero, I., Frieman, J., Gallardo, P. A., García-Bellido, J., Giannini, G., Gruen, D., Gruendl, R. A., Gutierrez, G., Hinton, S. R., Hollowood, D. L., James, D. J., Kosowsky, A., Kuehn, K., Lokken, M., Louis, T., Marshall, J. L., McMahon, J., Mena-Fernández, J., Menanteau, F., Miquel, R., Moodley, K., Mroczkowski, T., Naess, S., Niemack, M. D., Ogando, R. L. C., Page, L., Pandey, S., Pieres, A., Malagón, A. A. Plazas, Raveri, M., Rodriguez-Monroy, M., Rykoff, E. S., Samuroff, S., Sanchez, E., Schaan, E., Sevilla-Noarbe, I., Sheldon, E., Sifón, C., Smith, M., Soares-Santos, M., Sobreira, F., Suchyta, E., Tarle, G., To, C., Vargas, C., Vavagiakis, E. M., Weaverdyck, N., Weller, J., Wiseman, P., Yanny, B.
Publikováno v:
Phys. Rev. D 108, 023516 - Published 18 July 2023
The kinematic and thermal Sunyaev-Zel'dovich (kSZ and tSZ) effects probe the abundance and thermodynamics of ionized gas in galaxies and clusters. We present a new hybrid estimator to measure the kSZ effect by combining cosmic microwave background te
Externí odkaz:
http://arxiv.org/abs/2305.06792
Autor:
Andreon, S., Romero, C., Aussel, H., Bhandarkar, T., Devlin, M., Dicker, S., Ladjelate, B., Lowe, I., Mason, B., Mroczkowski, T., Raichoor, A., Sarazin, C., Trinchieri, G.
In this work we study the intracluster medium of a galaxy cluster at the cosmic noon: JKCS041 at z=1.803. A 28h long Sunyaev-Zel'dovich (SZ) observation using MUSTANG-2 allows us to detect JKCS041, even if intrinsically extremely faint compared to ot
Externí odkaz:
http://arxiv.org/abs/2305.02353
Autor:
Adam, R., Bartalucci, I., Pratt, G. W., Ade, P., André, P., Arnaud, M., Beelen, A., Benoît, A., Bideaud, A., Billot, N., Bourdin, H., Bourrion, O., Calvo, M., Catalano, A., Coiffard, G., Comis, B., D’Addabbo, A., De Petris, M., Démoclès, J., Désert, F.-X., Doyle, S., Egami, E., Ferrari, C., Goupy, J., Kramer, C., Lagache, G., Leclercq, S., Macías-Pérez, J.-F., Maurogordato, S., Mauskopf, P., Mayet, F., Monfardini, A., Mroczkowski, T., Pajot, F., Pascale, E., Perotto, L., Pisano, G., Pointecouteau, E., Ponthieu, N., Revéret, V., Ritacco, A., Rodriguez, L., Romero, C., Ruppin, F., Schuster, K., Sievers, A., Triqueneaux, S., Tucker, C., Zemcov, M., Zylka, R.
Measurement of the gas velocity distribution in galaxy clusters provides insight into the physics of mergers, through which large scale structures form in the Universe. Velocity estimates within the intracluster medium (ICM) can be obtained via the S
Externí odkaz:
http://hdl.handle.net/10150/623249
http://arizona.openrepository.com/arizona/handle/10150/623249
http://arizona.openrepository.com/arizona/handle/10150/623249
Autor:
Navarro-Almaida, D., Bop, C. T., Lique, F., Esplugues, G., Rodríguez-Baras, M., Kramer, C., Romero, C. E., Fuente, A., Caselli, P., Riviére-Marichalar, P., Kirk, J. M., Chacón-Tanarro, A., Roueff, E., Mroczkowski, T., Bhandarkar, T., Devlin, M., Dicker, S., Lowe, I., Mason, B., Sarazin, C. L., Sievers, J.
Publikováno v:
A&A 670, A110 (2023)
HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as chemical thermometers and evolutionary tracers to characterize star-forming regions. Despite their importance in carrying information that is vital to studies of the chemist
Externí odkaz:
http://arxiv.org/abs/2212.07675