Zobrazeno 1 - 10
of 122
pro vyhledávání: '"Bahe, Yannick"'
Autor:
Morishita, Takahiro, Mason, Charlotte A., Kreilgaard, Kimi C., Trenti, Michele, Treu, Tommaso, Vulcani, Benedetta, Zhang, Yechi, Abdurro'uf, Alavi, Anahita, Atek, Hakim, Bahe, Yannick, Bradac, Marusa, Bradley, Larry D., Bunker, Andrew J., Coe, Dan, Colbert, James, Gelli, Viola, Hayes, Matthew J., Jones, Tucker, Kodama, Tadayuki, Leethochawalit, Nicha, Liu, Zhaoran, Malkan, Matthew A., Mehta, Vihang, Metha, Benjamin, Newman, Andrew B., Rafelski, Marc, Roberts-Borsani, Guido, Rutkowski, Michael J., Scarlata, Claudia, Stiavelli, Massimo, Sutanto, Ryo A., Takahashi, Kosuke, Teplitz, Harry I., Wang, Xin
We introduce the Bias-free Extragalactic Analysis for Cosmic Origins with NIRCam (BEACON) survey, a JWST Cycle2 program allocated up to 600 pure-parallel hours of observations. BEACON explores high-latitude areas of the sky with JWST/NIRCam over $\si
Externí odkaz:
http://arxiv.org/abs/2412.04211
Autor:
Conger, Kim, Rudnick, Gregory, Finn, Rose A., Castignani, Gianluca, Moustakas, John, Vulcani, Benedetta, Zakharova, Daria, Xie, Lizhi, Combes, Francoise, Jablonka, Pascale, Bahé, Yannick, De Lucia, Gabriella, Desai, Vandana, Koopmann, Rebecca A., Norman, Dara, Townsend, Melinda, Zaritsky, Dennis
Recent theoretical work and targeted observational studies suggest that filaments are sites of galaxy preprocessing. The aim of the WISESize project is to directly probe galaxies over the full range of environments to quantify and characterize extrin
Externí odkaz:
http://arxiv.org/abs/2411.02352
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:
Correa, Camila, Schaller, Matthieu, Schaye, Joop, Ploeckinger, Sylvia, Borrow, Josh, Bahe, Yannick
Self-interacting dark matter (SIDM) has the potential to significantly influence galaxy formation in comparison to the cold, collisionless dark matter paradigm (CDM), resulting in observable effects. This study aims to elucidate this influence and to
Externí odkaz:
http://arxiv.org/abs/2403.09186
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:
Gully, Harry, Hatch, Nina, Bahé, Yannick, Balogh, Michael, Bolzonella, Micol, Cooper, M. C., Muzzin, Adam, Pozzetti, Lucia, Rudnick, Gregory, Vulcani, Benedetta, Wilson, Gillian
Publikováno v:
MNRAS, Volume 527, Issue 4, February 2024, Pages 10680-10696
We have identified 189 candidate $z > 1.3$ protoclusters and clusters in the LSST Deep Drilling Fields. This sample will enable the measurement of the metal enrichment and star formation history of clusters during their early assembly period through
Externí odkaz:
http://arxiv.org/abs/2401.05504
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