Zobrazeno 1 - 10
of 2 221
pro vyhledávání: '"Comparat"'
Autor:
COMPARATO, Fábio Konder
Publikováno v:
Revista de Direito Sanitário, Vol 11, Iss 3, Pp 204-219 (2010)
Jurisprudência em perspectiva. Comentários.
Externí odkaz:
https://doaj.org/article/09d342620dc0441fa5bc6560a2360b15
Publikováno v:
Journal of Dental Medicine, Vol 18, Iss 2, Pp 29-34 (2005)
Statement of Problem: One of the greatest problems in metal –ceramic restorations is debonding of porcelain from dental alloys. Production of dental alloys by Iranian companies necessitates the evaluation of physical and handling properties of thes
Externí odkaz:
https://doaj.org/article/cd4046e6c1164c429743c761abab86cc
Publikováno v:
Comparative Cytogenetics, Vol 3, Iss 1, Pp 79-81 (2009)
On 6 December 2008 Egeny Kachvoryan, an eminent specialist in the field of entomology, taxonomy, cytogenetics and ecology of blackflies (Simulidae, Diptera) passed away. She had many ideas and plans for the future and until her last day she was strug
Externí odkaz:
https://doaj.org/article/bd9da5c988f5465083e03fbfbca191a8
The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
Autor:
Zhang, Yi, Comparat, Johan, Ponti, Gabriele, Merloni, Andrea, Nandra, Kirpal, Haberl, Frank, Truong, Nhut, Pillepich, Annalisa, Popesso, Paola, Locatelli, Nicola, Zhang, Xiaoyuan, Sanders, Jeremy, Zheng, Xueying, Liu, Ang, Liu, Teng, Predehl, Peter, Salvato, Mara, Bruggen, Marcus, Shreeram, Soumya, Yeung, Michael C. H.
The circumgalactic medium (CGM), as the gas repository for star formation, might contain the answer to the mysterious galaxy quenching and bimodal galaxy population origin. We measured the X-ray emission of the hot CGM around star-forming and quiesce
Externí odkaz:
http://arxiv.org/abs/2411.19945
Autor:
Popesso, P., Marini, I., Dolag, K., Lamer, G., Csizi, B., Biffi, V., Robothan, A., Bravo, M., Biviano, A., Vladutesku-Zopp, S., Lovisari, L., Ettori, S., Angelinelli, M., Driver, S., Toptun, V., Dev, A., Mazengo, D., Merloni, A., Zhang, Y., Comparat, J., Ponti, G., Bulbul, E.
This study examines the average X-ray properties of massive halos at z< 0.2, covering the largest halo mass range to date, from Milky Way-like halos to massive clusters. The analysis is based on stacking in the eFEDS area of the GAMA galaxy group sam
Externí odkaz:
http://arxiv.org/abs/2411.17120
Autor:
Popesso, P., Biviano, A., Marini, I., Dolag, K., Vladutescu-Zopp, S., Csizi, B., Biffi, V., Lamer, G., Robothan, A., Bravo, M., Lovisari, L., Ettori, S., Angelinelli, M., Driver, S., Toptun, V., Dev, A., Mazengo, D., Merloni, A., Comparat, J., Ponti, G., Bulbul, E., Grandis, S., Bahar, E.
By using eROSITA data in the eFEDS area, we provide a measure of the hot gas fraction vs. halo mass relation over the largest halo mass range, from Milky Way-sized halos to massive clusters, and to the largest radii ever probed so far in local system
Externí odkaz:
http://arxiv.org/abs/2411.16555
Autor:
Popesso, P., Marini, I., Dolag, K., Lamer, G., Csizi, B., Vladutescu-Zopp, S., Biffi, V., Robothan, A., Bravo, M., Tempel, E., Yang, X., Li, Q., Biviano, A., Lovisari, L., Ettori, S., Angelinelli, M., Driver, S., Toptun, V., Dev, A., Mazengo, D., Merloni, A., Comparat, J., Zhang, Y., Ponti, G., Bulbul, E.
Hydrodynamical simulation predictions are often compared with observational data without fully accounting for systematics and biases specific to observational techniques. Using the magnetohydrodynamical simulation Magneticum, we generate mock eROSITA
Externí odkaz:
http://arxiv.org/abs/2411.16546
Autor:
Sifón, Cristóbal, Finoguenov, Alexis, Haines, Christopher P., Jaffé, Yara, Amrutha, B. M., Demarco, Ricardo, Lima, E. V. R., Lima-Dias, Ciria, Méndez-Hernández, Hugo, Merluzzi, Paola, Monachesi, Antonela, Teixeira, Gabriel S. M., Tejos, Nicolas, Araya-Araya, Pablo, Argudo-Fernández, Maria, Baier-Soto, Raúl, Bilton, Lawrence E., Bom, C. R., Calderón, Juan Pablo, Cassarà, Letizia P., Comparat, Johan, Courtois, H. M., D'Ago, Giuseppe, Dupuy, Alexandra, Fritz, Alexander, Haack, Rodrigo F., Herpich, Fabio R., Ibar, E., Kuchner, Ulrike, Lopes, Amanda R., Lopez, Sebastian, Lösch, Elismar, McGee, Sean, de Oliveira, C. Mendes, Morelli, Lorenzo, Moretti, Alessia, Pallero, Diego, Piraino-Cerda, Franco, Pompei, Emanuela, Rescigno, U., Smith, Rory, Castelli, Analía V. Smith, Sodré Jr, Laerte, Tempel, Elmo
CHANCES, the CHileAN Cluster galaxy Evolution Survey, will study the evolution of galaxies in and around ${\sim}$150 massive galaxy clusters, from the local universe out to z=0.45. CHANCES will use the new 4MOST Spectroscopic Survey Facility on the V
Externí odkaz:
http://arxiv.org/abs/2411.13655
Autor:
Li, Pengfei, Liu, Ang, Kluge, Matthias, Comparat, Johan, Tian, Yong, Júlio, Mariana P., Pawlowski, Marcel S., Sanders, Jeremy, Bulbul, Esra, Schwope, Axel, Ghirardini, Vittorio, Zhang, Xiaoyuan, Bahar, Y. Emre, Ramos-Ceja, Miriam E., Balzer, Fabian, Garrel, Christian
The mass of galaxy clusters is a critical quantity for probing cluster cosmology and testing theories of gravity, but its measurement could be biased given assumptions are inevitable. In this paper, we employ and compare two mass proxies for galaxy c
Externí odkaz:
http://arxiv.org/abs/2411.09735
The baryon census and the mass-density of stars, neutral gas, and hot gas as a function of halo mass
Autor:
Dev, Ajay, Driver, Simon P., Meyer, Martin, Robotham, Aaron, Obreschkow, Danail, Popesso, Paola, Comparat, Johan
We study the stellar, neutral gas content within halos over a halo mass range $10^{10} \text{ to } 10^{15.5} \text{M}_\odot$ and hot X-ray gas content over a halo mass range $10^{12.8} \text{ to } 10^{15.5} \text{M}_\odot$ in the local universe. We c
Externí odkaz:
http://arxiv.org/abs/2411.00456