Zobrazeno 1 - 10
of 287
pro vyhledávání: '"P, Trcka"'
Autor:
Gebek, Andrea, Trčka, Ana, Baes, Maarten, Martorano, Marco, Pillepich, Annalisa, Kapoor, Anand Utsav, Nersesian, Angelos, van der Wel, Arjen
We apply the 3D dust radiative transfer code SKIRT to the low-redshift ($z\leq0.1$) galaxy population in the TNG100 cosmological simulation, the fiducial run of the IllustrisTNG project. We compute global fluxes and spectral energy distributions (SED
Externí odkaz:
http://arxiv.org/abs/2405.04925
Autor:
Baes, Maarten, Mosenkov, Aleksandr, Kelly, Raymond, Abdurro'uf, Andreadis, Nick, Tulu, Sena Bokona, Camps, Peter, Emana, Abdissa Tassama, Fritz, Jacopo, Gebek, Andrea, Kovacic, Inja, La Marca, Antonio, Martorano, Marco, Nersesian, Angelos, Rodriguez-Gomez, Vicente, Tortora, Crescenzo, Trcka, Ana, Meulen, Bert Vander, van der Wel, Arjen, Wang, Lingyu
Galaxy sizes correlate with many other important properties of galaxies, and the cosmic evolution of galaxy sizes is an important observational diagnostic for constraining galaxy evolution models. The effective radius is probably the most widely used
Externí odkaz:
http://arxiv.org/abs/2401.04225
Autor:
Baes, Maarten, Gebek, Andrea, Trcka, Ana, Camps, Peter, van der Wel, Arjen, Abdurro'uf, Andreadis, Nick, Tulu, Sena Bokona, Emana, Abdissa Tassama, Fritz, Jacopo, Kelly, Raymond, Kovacic, Inja, La Marca, Antonio, Martorano, Marco, Mosenkov, Aleksandr, Nersesian, Angelos, Rodriguez-Gomez, Vicente, Tortora, Crescenzo, Meulen, Bert Vander, Wang, Lingyu
Galaxy morphology is a powerful diagnostic to assess the realism of cosmological hydrodynamical simulations. Determining the morphology of simulated galaxies requires the generation of synthetic images through 3D radiative transfer post-processing th
Externí odkaz:
http://arxiv.org/abs/2401.04224
Autor:
Trcka, Ana, Baes, Maarten, Camps, Peter, Kapoor, Anand Utsav, Nelson, Dylan, Pillepich, Annalisa, Barrientos, Daniela, Hernquist, Lars, Marinacci, Federico, Vogelsberger, Mark
We apply the radiative transfer (RT) code SKIRT on a sample of ~14000 low-redshift (z<= 0.1) galaxies extracted from the TNG50 simulation to enable an apples-to-apples comparison with observations. The RT procedure is calibrated via comparison of a s
Externí odkaz:
http://arxiv.org/abs/2208.06424
Autor:
Camps, Peter, Kapoor, Anand Utsav, Trčka, Ana, Font, Andreea S., McCarthy, Ian G., Trayford, James, Baes, Maarten
We present redshift-zero synthetic dust-aware observations for the 45 Milky Way-mass simulated galaxies of the ARTEMIS project, calculated with the SKIRT radiative transfer code. The post-processing procedure includes components for star-forming regi
Externí odkaz:
http://arxiv.org/abs/2203.06078
Autor:
Kapoor, Anand Utsav, Camps, Peter, Baes, Maarten, Trcka, Ana, Grand, Robert J. J., van der Wel, Arjen, Cortese, Luca, De Looze, Ilse, Barrientos, Daniela
We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The post-processing procedure includes components f
Externí odkaz:
http://arxiv.org/abs/2107.06595
Autor:
Nersesian, Angelos, Dobbels, Wouter, Xilouris, Manolis E., Baes, Maarten, Bianchi, Simone, Casasola, Viviana, Clark, Christopher J. R., De Looze, Ilse, Galliano, Frédéric, Madden, Suzanne C., Mosenkov, Aleksandr V., Paspaliaris, Evangelos-D., Trčka, Ana
The objective of this paper is to understand the variance of the far-infrared (FIR) spectral energy distribution (SED) of the DustPedia galaxies, and its link with the stellar and dust properties. An interesting aspect of the dust emission is the inf
Externí odkaz:
http://arxiv.org/abs/2107.04383
Autor:
Oliver Simoncik, Vlastimil Tichy, Michal Durech, Lenka Hernychova, Filip Trcka, Lukas Uhrik, Miroslav Bardelcik, Philip J Coates, Borivoj Vojtesek, Petr Muller
Publikováno v:
PLoS ONE, Vol 19, Iss 11, p e0312524 (2024)
Stress responses play a vital role in cellular survival against environmental challenges, often exploited by cancer cells to proliferate, counteract genomic instability, and resist therapeutic stress. Heat shock factor protein 1 (HSF1), a central tra
Externí odkaz:
https://doaj.org/article/6dd347d083d24ae2a6d2adedd9e277ab
Autor:
Nersesian, Angelos, Viaene, Sebastien, De Looze, Ilse, Baes, Maarten, Xilouris, Emmanuel M., Smith, Matthew W. L., Bianchi, Simone, Casasola, Viviana, Cassara, Letizia P., Clark, Christopher J. R., Dobbels, Wouter, Fritz, Jacopo, Galliano, Frederic, Madden, Suzanne C., Mosenkov, Aleksandr V., Trcka, Ana
Publikováno v:
A&A 643, A90 (2020)
Investigating the dust heating mechanisms in galaxies provides a deeper understanding of how the internal energy balance drives their evolution. Over the last decade, radiative transfer simulations based on the Monte Carlo method have underlined the
Externí odkaz:
http://arxiv.org/abs/2009.07280
Autor:
Baes, Maarten, Nersesian, Angelos, Casasola, Viviana, Bianchi, Simone, Cassarà, Letizia P., Clark, Christopher J. R., De Looze, Ilse, Dobbels, Wouter, Fritz, Jacopo, Galametz, Maud, Galliano, Frédéric, Madden, Suzanne C., Mosenkov, Aleksandr V., Viaene, Sébastien, Trčka, Ana, Xilouris, Emmanuel M.
Publikováno v:
A&A 641, A119 (2020)
We present the first nonparametric morphological analysis of a set of spiral galaxies from UV to submm wavelengths. Our study is based on high-quality multi-wavelength imaging for nine well-resolved spiral galaxies from the DustPedia database, combin
Externí odkaz:
http://arxiv.org/abs/2007.02012