Results 151 to 160 of about 15,230 (253)

Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at $1.4\lesssim z\lesssim1.7$

, 2018
V. Strazzullo, M. Pannella, J. J. Mohr, A. Saro, M. L. N. Ashby, Matthew Bayliss, S. Bocquet, Esra Bülbül, Gourav Khullar, A. Mantz, S. A. Stanford, B. A. Benson, L. E. Bleem, M. Brodwin, R. E. A. Canning, R. Capasso, I-Non Chiu, Anthony H. Gonzalez, N. Gupta, Julie Hlavacek-Larrondo, Matthias Klein, M. McDonald, Emil Noordeh, David Rapetti, C. L. Reichardt, T. Schrabback, Keren Sharon, B. Stalder   +27 more
openalex   +2 more sources

Testing Galaxy Formation Models with the Stellar Mass–Halo Mass Relations for Star-forming and Quiescent Galaxies

The Astrophysical Journal
The tight relationship between the stellar mass and halo mass of galaxies is one of the most fundamental scaling relations in galaxy formation and evolution. It has become a critical constraint for galaxy formation models.
Kai Wang, Yingjie Peng
doaj   +1 more source

Evidence for a change in the dominant satellite galaxy quenching mechanism atz = 1 [PDF]

, 2016
Michael L. Balogh, Sean McGee, Angus Mok, Adam Muzzin, R. F. J. van der Burg, R. G. Bower, A. Finoguenov, Henk Hoekstra, C. Lidman, John S. Mulchaey, Allison Noble, Laura C. Parker, Masayuki Tanaka, David J. Wilman, Tracy Webb, Gillian Wilson, H. K. C. Yee   +16 more
openalex   +1 more source

To High Redshift and Low Mass: Exploring the Emergence of Quenched Galaxies and Their Environments at 3 < z < 6 in the Ultra-deep JADES MIRI F770W Parallel [PDF]

Stacey Alberts, Christina C. Williams, Jakob M. Helton, Katherine A. Suess, Zhiyuan Ji, Irene Shivaei, Jianwei Lyu, G. H. Rieke, William Baker, Nina Bonaventura, Andrew J. Bunker, Stefano Carniani, S. Charlot, Emma Curtis-Lake, Francesco D’Eugenio, Daniel J. Eisenstein, Anna de Graaff, Kevin Hainline, Ryan Hausen, Benjamin D. Johnson, R. Maiolino, Eleonora Parlanti, Marcia Rieke, Brant Robertson, Yang Sun, Sandro Tacchella, Christopher N. A. Willmer, Chris J. Willott   +27 more
openalex   +1 more source

Active Galactic Nuclei in the Green Valley at z ∼ 0.7

The Astrophysical Journal
We present near-infrared (NIR) spectroscopy using the MMT and Magellan infrared spectrograph for a sample of 29 massive galaxies ( $\mathrm{log}\ {M}_{* }/{M}_{\odot }\gtrsim 10$ ) at z ∼ 0.7 with optical spectroscopy from the Large Early Galaxy ...
Charity Woodrum, Christina C. Williams, Marcia Rieke, Kevin N. Hainline, Raphael E. Hviding, Zhiyuan Ji, Robert Kennicutt, Christopher N. A. Willmer   +7 more
doaj   +1 more source

The ages, metallicities and element abundance ratios of massive quenched galaxies at z~1.6 [PDF]

, 2014
Masato Onodera, C. M. Carollo, A. Renzini, Michele Cappellari, C. Mancini, N. Arimoto, E. Daddi, R. Gobat, V. Strazzullo, Sandro Tacchella, Y. Yamada   +10 more
openalex   +1 more source

Improved SED-fitting Assumptions Result in Inside-out Quenching at z ~ 0.5 and Quenching at All Radii Simultaneously at z ~ 1

The Astrophysical Journal
Many studies conclude that galaxies quench from the inside-out by examining profiles of specific star formation rate (sSFR). These are usually measured by fitting spectral energy distributions (SEDs) assuming a fixed dust law and uniform priors on all ...
Alexander de la Vega, Susan A. Kassin, Camilla Pacifici, Stéphane Charlot, Emma Curtis-Lake, Jacopo Chevallard, Timothy M. Heckman, Anton M. Koekemoer, Weichen Wang   +8 more
doaj   +1 more source

THE QUENCHED MASS PORTION OF STAR-FORMING GALAXIES AND THE ORIGIN OF THE STAR FORMATION SEQUENCE SLOPE [PDF]

, 2016
Zhizheng Pan, Xianzhong Zheng, Xu Kong
openalex   +1 more source

Spatially Resolving Galaxy Environmental Quenching in the SAMI Galaxy Survey

, 2019
In order to identify how spatially resolved star formation depends on environment, we use the unitless scale-radius ratio (r50,Hα/r50,cont) (building on earlier work of Schaefer et al. 2017). We will use this metric to investigate quenching across a much enlarged dynamic range of environment (from clusters to the field), and with the full SAMI Galaxy ...
openaire   +1 more source

The Cosmic Web's Fingerprint on Galaxy Quenching: Direct Evidence from High-Redshift Filaments

Revista, Zen, ASTRO, 10
openalex   +2 more sources