Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Kurk, Jaron"'
Autor:
Shimakawa, Rhythm, Pérez-Martínez, José Manuel, Koyama, Yusei, Tanaka, Masayuki, Tanaka, Ichi, Kodama, Tadayuki, Hatch, Nina A., Röttgering, Huub J. A., Dannerbauer, Helmut, Kurk, Jaron D.
As a considerable investment of time from various telescope facilities were dedicated toward studying the Spiderweb protocluster at $z=2.2$, it so far remains one of the most extensively studied protocluster. We report here the latest results in this
Externí odkaz:
http://arxiv.org/abs/2306.06392
Autor:
Namiki, Shigeru V., Koyama, Yusei, Hayashi, Masao, Tadaki, Ken-ichi, Kashikawa, Nobunari, Onodera, Masato, Shimakawa, Rhythm, Kodama, Tadayuki, Tanaka, Ichi, Schreiber, N. M. Förster, Kurk, Jaron, Genzel, R.
We present the results of our near-infrared (NIR) spectroscopic observations of a rich cluster candidate around a radio galaxy at $z=1.52$ (4C65.22) with Subaru/MOIRCS and LBT/LUCI. We observed 71 galaxies mostly on the star-forming main sequence sel
Externí odkaz:
http://arxiv.org/abs/1904.12090
Autor:
Shimakawa, Rhythm, Koyama, Yusei, Rottgering, Huub J. A., Kodama, Tadayuki, Hayashi, Masao, Hatch, Nina A., Dannerbauer, Helmut, Tanaka, Ichi, Tadaki, Ken-ichi, Suzuki, Tomoko L., Fukagawa, Nao, Cai, Zheng, Kurk, Jaron D.
This paper is the second in a series presenting the results of our deep H$\alpha$-line survey towards protoclusters at $z>2$, based on narrow-band imaging with the Subaru Telescope. This work investigates massive galaxies in a protocluster region ass
Externí odkaz:
http://arxiv.org/abs/1809.08755
Akademický článek
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We report on a study of the 2300-2600\AA FeII/FeII* multiplets in the rest-UV spectra of star-forming galaxies at 1.0
Externí odkaz:
http://arxiv.org/abs/1407.0149
Autor:
Wuyts, Eva, Kurk, Jaron, Schreiber, Natascha M. Förster, Genzel, Reinhard, Wisnioski, Emily, Bandara, Kaushala, Wuyts, Stijn, Beifiori, Alessandra, Bender, Ralf, Brammer, Gabriel B., Burkert, Andreas, Buschkamp, Peter, Carollo, C. Marcella, Chan, Jeffrey, Davies, Ric, Eisenhauer, Frank, Fossati, Matteo, Kulkarni, Sandesh K., Lang, Philipp, Lilly, Simon J., Lutz, Dieter, Mancini, Chiara, Mendel, J. Trevor, Momcheva, Ivelina G., Naab, Thorsten, Nelson, Erica J., Renzini, Alvio, Rosario, David, Saglia, Roberto P., Seitz, Stella, Sharples, Ray M., Sternberg, Amiel, Tacchella, Sandro, Tacconi, Linda J., van Dokkum, Pieter, Wilman, David J.
We present the correlations between stellar mass, star formation rate (SFR) and [NII]/Ha flux ratio as indicator of gas-phase metallicity for a sample of 222 galaxies at 0.8 < z < 2.6 and log(M*/Msun)=9.0-11.5 from the LUCI, SINS/zC-SINF and KMOS3D s
Externí odkaz:
http://arxiv.org/abs/1405.6590
Autor:
Galametz, Audrey, Stern, Daniel, Pentericci, Laura, De Breuck, Carlos, Vernet, Joel, Wylezalek, Dominika, Fassbender, Rene, Hatch, Nina, Kurk, Jaron, Overzier, Roderik, Rettura, Alessandro, Seymour, Nick
We present the spectroscopic confirmation of a structure of galaxies surrounding the radio galaxy MRC0156-252 at z = 2.02. The structure was initially discovered as an overdensity of both near-infrared selected z > 1.6 and mid-infrared selected z > 1
Externí odkaz:
http://arxiv.org/abs/1309.6645
Autor:
Bañados, Eduardo, Venemans, Bram, Walter, Fabian, Kurk, Jaron, Overzier, Roderik, Ouchi, Masami
Publikováno v:
ApJ, 773, 178, 2013
High-redshift quasars are believed to reside in massive halos in the early universe and should therefore be located in fields with overdensities of galaxies, which are thought to evolve into galaxy clusters seen in the local universe. However, despit
Externí odkaz:
http://arxiv.org/abs/1306.6642
On the formation time scale of massive cluster ellipticals based on deep near-IR spectroscopy at z~2
Autor:
Tanaka, Masayuki, Toft, Sune, Marchesini, Danilo, Zirm, Andrew, De Breuck, Carlos, Kodama, Tadayuki, Koyama, Yusei, Kurk, Jaron, Tanaka, Ichi
We present improved constraints on the formation time scale of massive cluster galaxies based on rest-frame optical spectra of galaxies in a forming cluster located at z=2.16. The spectra are obtained with MOIRCS on the Subaru telescope with an integ
Externí odkaz:
http://arxiv.org/abs/1306.4406
Autor:
Koyama, Yusei, Smail, Ian, Kurk, Jaron, Geach, James E., Sobral, David, Kodama, Tadayuki, Nakata, Fumiaki, Swinbank, A. M., Best, Philip N., Hayashi, Masao, Tadaki, Ken-ichi
This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and stellar mass (M*) over the last ~10 Gyrs, particularly focusing on its environmental dependence. We first present the mid-infrared (MIR) properties o
Externí odkaz:
http://arxiv.org/abs/1302.5315