Zobrazeno 1 - 10
of 640
pro vyhledávání: '"Yannick M"'
Autor:
Brown, Harley J., Martin, Garreth, Pearce, Frazer R., Hatch, Nina A., Bahé, Yannick M., Dubois, Yohan
The diffuse stellar component of galaxy clusters made up of intergalactic stars is termed the intracluster light (ICL). Though there is a developing understanding of the mechanisms by which the ICL is formed, no strong consensus has yet been reached
Externí odkaz:
http://arxiv.org/abs/2409.10607
Autor:
Xie, Lizhi, De Lucia, Gabriella, Fontanot, Fabio, Hirschmann, Michaela, Bahé, Yannick M, Balogh, Michael L., Muzzin, Adam, Vulcani, Benedetta, Baxter, Devontae C., Forrest, Ben, Wilson, Gillian, Rudnick, Gregory H., Cooper, M. C., Rescigno, Umberto
Many quiescent galaxies discovered in the early Universe by \textit{JWST} raise fundamental questions on when and how these galaxies became and stayed quenched. Making use of the latest version of the semi-analytic model GAEA that provides good agree
Externí odkaz:
http://arxiv.org/abs/2402.01314
Autor:
Edward, Adit H., Balogh, Michael L., Bahe, Yannick M., Cooper, Michael C., Hatch, Nina A., Marchioni, Justin, Muzzin, Adam, Noble, Allison, Rednick, Gregory H., Vulcani, Benedetta, Wilson, Gillian, De Lucia, Gabriella, Demarco, Ricardo, Forrest, Ben, Hirschmann, Michaela, Castignani, Gianluca, Cerulo, Pierluigi, Finn, Rose A., Hewitt, Guillaume, Jablonka, Pascale, Kodama, Yadayuki, Maurogordato, Sophie, Nantais, Julie, Xie, Lizhi
We present an analysis of the galaxy stellar mass function (SMF) of 14 known protoclusters between $2.0 < z < 2.5$ in the COSMOS field, down to a mass limit of $10^{9.5}$ M$_{\odot}$. We use existing photometric redshifts with a statistical backgroun
Externí odkaz:
http://arxiv.org/abs/2312.12380
Autor:
Štofanová, Lýdia, Simionescu, Aurora, Wijers, Nastasha A., Schaye, Joop, Kaastra, Jelle S., Bahé, Yannick M., Arámburo-García, Andrés
The warm-hot plasma in cosmic web filaments is thought to comprise a large fraction of the gas in the local Universe. So far, the search for this gas has focused on mapping its emission, or detecting its absorption signatures against bright, point-li
Externí odkaz:
http://arxiv.org/abs/2311.10062
Autor:
Stevens, Adam R. H., Brown, Toby, Diemer, Benedikt, Pillepich, Annalisa, Hernquist, Lars, Nelson, Dylan, Bahé, Yannick M., Boselli, Alessandro, Davis, Timothy A., Elahi, Pascal J., Ellison, Sara L., Jiménez-Donaire, María J., Roberts, Ian D., Spekkens, Kristine, Villanueva, Vicente, Watts, Adam B., Wilson, Christine D., Zabel, Nikki
It has been shown in previous publications that the TNG100 simulation quantitatively reproduces the observed reduction in each of the total atomic and total molecular hydrogen gas for galaxies within massive halos, i.e.~dense environments. In this Le
Externí odkaz:
http://arxiv.org/abs/2310.08023
Autor:
Brown, Toby, Roberts, Ian D., Thorp, Mallory, Ellison, Sara L., Zabel, Nikki, Wilson, Christine D., Bahé, Yannick M., Bisaria, Dhruv, Bolatto, Alberto D., Boselli, Alessandro, Chung, Aeree, Cortese, Luca, Catinella, Barbara, Davis, Timothy A., Jiménez-Donaire, María J., Lagos, Claudia D. P., Lee, Bumhyun, Parker, Laura C., Smith, Rory, Spekkens, Kristine, Stevens, Adam R. H., Villanueva, Vicente, Watts, Adam B.
We study how environment regulates the star formation cycle of 33 Virgo Cluster satellite galaxies on 720 parsec scales. We present the first resolved star-forming main sequence for cluster galaxies, dividing the sample based on their global HI prope
Externí odkaz:
http://arxiv.org/abs/2308.10943
Many $z=1.5$ galaxies with a stellar mass ($M_{\star}$) $\geq 10^{10}\,\mathrm{M}_\odot$ are already quenched in both galaxy clusters ($>50$ per cent) and the field ($>20$ per cent), with clusters having a higher quenched fraction at all stellar mass
Externí odkaz:
http://arxiv.org/abs/2307.01147
Autor:
Kugel, Roi, Schaye, Joop, Schaller, Matthieu, Helly, John C., Braspenning, Joey, Elbers, Willem, Frenk, Carlos S., McCarthy, Ian G., Kwan, Juliana, Salcido, Jaime, van Daalen, Marcel P., Vandenbroucke, Bert, Bahé, Yannick M., Borrow, Josh, Chaikin, Evgenii, Huško, Filip, Jenkins, Adrian, Lacey, Cedric G., Nobels, Folkert S. J., Vernon, Ian
To fully take advantage of the data provided by large-scale structure surveys, we need to quantify the potential impact of baryonic effects, such as feedback from active galactic nuclei (AGN) and star formation, on cosmological observables. In simula
Externí odkaz:
http://arxiv.org/abs/2306.05492
Autor:
Schaye, Joop, Kugel, Roi, Schaller, Matthieu, Helly, John C., Braspenning, Joey, Elbers, Willem, McCarthy, Ian G., van Daalen, Marcel P., Vandenbroucke, Bert, Frenk, Carlos S., Kwan, Juliana, Salcido, Jaime, Bahé, Yannick M., Borrow, Josh, Chaikin, Evgenii, Hahn, Oliver, Huško, Filip, Jenkins, Adrian, Lacey, Cedric G., Nobels, Folkert S. J.
Publikováno v:
2023, MNRAS, 526, 4978
We introduce the Virgo Consortium's FLAMINGO suite of hydrodynamical simulations for cosmology and galaxy cluster physics. To ensure the simulations are sufficiently realistic for studies of large-scale structure, the subgrid prescriptions for stella
Externí odkaz:
http://arxiv.org/abs/2306.04024
Autor:
Watts, Adam B., Cortese, Luca, Catinella, Barbara, Brown, Toby, Wilson, Christine D., Zabel, Nikki, Roberts, Ian D., Davis, Timothy A., Thorp, Mallory, Chung, Aeree, Stevens, Adam R. H., Ellison, Sara L., Spekkens, Kristine, Parker, Laura C., Bahé, Yannick M., Villanueva, Vicente, Jiménez-Donaire, María, Bisaria, Dhruv, Boselli, Alessandro, Bolatto, Alberto D., Lee, Bumhyun
The quenching of cluster satellite galaxies is inextricably linked to the suppression of their cold interstellar medium (ISM) by environmental mechanisms. While the removal of neutral atomic hydrogen (HI) at large radii is well studied, how the envir
Externí odkaz:
http://arxiv.org/abs/2303.07549