Zobrazeno 1 - 10
of 894
pro vyhledávání: '"Balogh, Michael"'
Autor:
Sazonova, Elizaveta, Morgan, Cameron R, Balogh, Michael, Alatalo, Katherine, Benavides, Jose A., Bluck, Asa, Brough, Sarah, Busa, Innocenza, Demarco, Ricardo, Donevski, Darko, Figueira, Miguel, Martin, Garreth, Mullaney, James R, Rodriguez-Gomez, Vicente, Román, Javier, Rowlands, Kate
Structural disturbances, such as galaxy mergers or instabilities, are key candidates for driving galaxy evolution, so it is important to detect and quantify galaxies hosting these disturbances spanning a range of masses, environments, and cosmic time
Externí odkaz:
http://arxiv.org/abs/2404.05792
Autor:
Marshall, Madeline A., Amen, Laurie, Woods, Tyrone E., Cote, Patrick J., Yung, L. Y. Aaron, Amenouche, Melissa, Pass, Emily K., Balogh, Michael, Salim, Samir, Moutard, Thibaud
The Cosmological Advanced Survey Telescope for Optical and UV Research (CASTOR) is a planned flagship space telescope, covering the blue-optical and UV part of the spectrum. Here we introduce the CASTOR image simulator, a Python GalSim package-based
Externí odkaz:
http://arxiv.org/abs/2402.17163
Autor:
Cheng, Isaac, Woods, Tyrone E., Côté, Patrick, Glover, Jennifer, Bansal, Dhananjhay, Amenouche, Melissa, Marshall, Madeline A., Amen, Laurie, Hutchings, John, Ferrarese, Laura, Venn, Kim A., Balogh, Michael, Blouin, Simon, Cloutier, Ryan, Dickson, Nolan, Gallagher, Sarah, Hellmich, Martin, Hénault-Brunet, Vincent, Khatu, Viraja, Lawlor-Forsyth, Cameron, Morgan, Cameron, Richer, Harvey, Sawicki, Marcin, Sorba, Robert
The Cosmological Advanced Survey Telescope for Optical and ultraviolet Research (CASTOR) is a proposed Canadian-led 1m-class space telescope that will carry out ultraviolet and blue-optical wide-field imaging, spectroscopy, and photometry. CASTOR wil
Externí odkaz:
http://arxiv.org/abs/2402.08137
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:
Cheng, Chloe M., Villaume, Alexa, Balogh, Michael L., Brodie, Jean P., Martín-Navarro, Ignacio, Romanowsky, Aaron J., van Dokkum, Pieter G.
We present a uniform analysis of the stellar initial mass function (IMF) from integrated light spectroscopy of 15 compact stellar systems (11 globular clusters in M31 and 4 ultra compact dwarfs in the Virgo cluster, UCDs) and two brightest Coma clust
Externí odkaz:
http://arxiv.org/abs/2309.14415
Autor:
Rudnick, Gregory, Bahé, Yannick, Balogh, Michael, Cooper, Mike, Hatch, Nina, Vulcani, Benedetta, Wilson, Gillian, Castignani, Gianluca, Cerulo, Pierluigi, De Lucia, Gabriella, DeMarco, Ricardo, Forrest, Benjamin, Jablonka, Pascale
Protoclusters are the densest regions in the distant universe ($z>2$) and are the progenitors of massive galaxy clusters ($M_{halo}>10^{14}{\rm M}_\odot$) in the local universe. They undoubtedly play a key role in early massive galaxy evolution and t
Externí odkaz:
http://arxiv.org/abs/2306.15735
Autor:
Baxter, Devontae C., Cooper, Michael C., Balogh, Michael L., Rudnick, Gregory H., De Lucia, Gabriella, Demarco, Ricardo, Finoguenov, Alexis, Forrest, Ben, Muzzin, Adam, Reeves, Andrew, Sarron, Florian, Vulcani, Benedetta, Wilson, Gillian, Zaritsky, Dennis
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 526, Issue 3, December 2023
We explore models of massive ($\gt 10^{10}~{\rm M}_{\odot}$) satellite quenching in massive clusters at $z\gtrsim1$ using an MCMC framework, focusing on two primary parameters: $R_{\rm quench}$ (the host-centric radius at which quenching begins) and
Externí odkaz:
http://arxiv.org/abs/2306.09404
Autor:
Balogh, Michael L., Gilbank, David G., Muzzin, Adam, Rudnick, Gregory, Cooper, Michael C., Lidman, Chris, Biviano, Andrea, Demarco, Ricardo, McGee, Sean L., Nantais, Julie B., Noble, Allison, Old, Lyndsay, Wilson, Gillian, Yee, Howard K. C., Bellhouse, Callum, Cerulo, Pierluigi, Chan, Jeffrey, Pintos-Castro, Irene, Simpson, Rane, van der Burg, Remco F. J., Zaritsky, Dennis, Ziparo, Felicia, Alonso, María Victoria, Bower, Richard G., De Lucia, Gabriella, Finoguenov, Alexis, Lambas, Diego Garcia, Muriel, Hernan, Parker, Laura C., Rettura, Alessandro, Valotto, Carlos, Wetzel, Andrew
We describe a new Large Program in progress on the Gemini North and South telescopes: Gemini Observations of Galaxies in Rich Early Environments (GOGREEN). This is an imaging and deep spectroscopic survey of 21 galaxy systems at 1 < z < 1.5, selected
Externí odkaz:
http://hdl.handle.net/10150/625732
http://arizona.openrepository.com/arizona/handle/10150/625732
http://arizona.openrepository.com/arizona/handle/10150/625732