Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Wilman, Dave"'
Autor:
Mendel, J. Trevor, Beifiori, Alessandra, Saglia, Roberto, Bender, Ralf, Brammer, Gabe, Chan, Jeffrey, Schreiber, Natascha Forster, Fossati, Matteo, Galametz, Audrey, Momcheva, Iva, Nelson, Erica, Wilman, Dave, Wuyts, Stijn
We study the dynamical properties of massive quiescent galaxies at $1.4 < z < 2.1$ using deep Hubble Space Telescope WFC3/F160W imaging and a combination of literature stellar velocity dispersion measurements and new near-infrared spectra obtained us
Externí odkaz:
http://arxiv.org/abs/2006.13949
Autor:
Tadaki, Ken-ichi, Genzel, Reinhard, Kodama, Tadayuki, Wuyts, Stijn, Wisnioski, Emily, Schreiber, Natascha M. Förster, Burkert, Andreas, Lang, Philipp, Tacconi, Linda J., Lutz, Dieter, Belli, Sirio, Davies, Richard I., Hatsukade, Bunyo, Hayashi, Masao, Herrera-Camus, Rodrigo, Ikarashi, Soh, Inoue, Shigeki, Kohno, Kotaro, Koyama, Yusei, Mendel, J. Trevor, Nakanishi, Kouichiro, Shimakawa, Rhythm, Suzuki, Tomoko L., Tamura, Yoichi, Tanaka, Ichi, Übler, Hannah, Wilman, Dave J.
We present 0".2-resolution Atacama Large Millimeter/submillimeter Array observations at 870 um for 25 Halpha-seleced star-forming galaxies (SFGs) around the main-sequence at z=2.2-2.5. We detect significant 870 um continuum emission in 16 (64%) of th
Externí odkaz:
http://arxiv.org/abs/1608.05412
Autor:
Fontanot, Fabio, Maccio', Andrea V., Hirschmann, Michaela, De Lucia, Gabriella, Kannan, Rahul, Somerville, Rachel S., Wilman, Dave
The distribution of galaxy morphological types is a key test for models of galaxy formation and evolution, providing strong constraints on the relative contribution of different physical processes responsible for the growth of the spheroidal componen
Externí odkaz:
http://arxiv.org/abs/1507.04748
Autor:
Hirschmann, Michaela, De Lucia, Gabriella, Wilman, Dave, Weinmann, Simone, Iovino, Angela, Cucciati, Olga, Zibetti, Stefano, Villalobos, Álvaro
We present a detailed analysis of the influence of the environment and of the environmental history on quenching star formation in central and satellite galaxies in the local Universe. We take advantage of publicly available galaxy catalogues obtaine
Externí odkaz:
http://arxiv.org/abs/1407.5621
Autor:
Ziparo, Felicia, Popesso, Paola, Biviano, Andrea, Finoguenov, Alexis, Wuyts, Stijn, Wilman, Dave, Salvato, Mara, Tanaka, Masayuki, Ilbert, Olivier, Nandra, Kirpal, Lutz, Dieter, Elbaz, David, Dickinson, Mark, Altieri, Bruno, Aussel, Herve', Berta, Stefano, Cimatti, Andrea, Fadda, Dario, Genzel, Reinhard, Flo'ch, Emeric Le, Magnelli, Benjamin, Nordon, R., Poglitsch, Albrecht, Pozzi, Francesca, Sanchez-Portal, Miguel, Tacconi, Linda, Bauer, Franz, Brandt, W. Niel, Cappelluti, Nico, Cooper, M., Mulchaey, John
In the local Universe, galaxy properties show a strong dependence on environment. In cluster cores, early type galaxies dominate, whereas star-forming galaxies are more and more common in the outskirts. At higher redshifts and in somewhat less dense
Externí odkaz:
http://arxiv.org/abs/1307.0833
We study the correlation between the morphological mix of cluster galaxies and the assembly history of the parent cluster by taking advantage of two independently developed semi-analytic models for galaxy formation and evolution. In our models, both
Externí odkaz:
http://arxiv.org/abs/1109.2599
Autor:
Balogh, Michael L., McGee, Sean L., Wilman, Dave, Bower, Richard G., Hau, George, Morris, Simon L., Mulchaey, J. S., Oemler Jr., A., Parker, Laura, Gwyn, Stephen
(Abridged) We present new optical and near-infrared imaging for a sample of 98 spectroscopically-selected galaxy groups at 0.25
Externí odkaz:
http://arxiv.org/abs/0905.3401
Autor:
Balogh, Michael L., Wilman, Dave, Henderson, Robert D. E., Bower, Richard G., Gilbank, David, Whitaker, Richard, Morris, Simon L., Hau, George, Mulchaey, John S., Oemler Jr, A., Carlberg, R. G.
We have obtained near-infrared imaging of 58 galaxy groups, in the redshift range 0.1
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610839
Autor:
Tadaki, Ken-ichi, Genzel, Reinhard, Kodama, Tadayuki, Wuyts, Stijn, Wisnioski, Emily, Förster Schreiber, Natascha M., Burkert, Andreas, Lang, Philipp, Tacconi, Linda J., Lutz, Dieter, Belli, Sirio, Davies, Richard I., Hatsukade, Bunyo, Hayashi, Masao, Herrera-Camus, Rodrigo, Ikarashi, Soh, Inoue, Shigeki, Kohno, Kotaro, Koyama, Yusei, Mendel, J. Trevor, Nakanishi, Kouichiro, Shimakawa, Rhythm, Suzuki, Tomoko L., Tamura, Yoichi, Tanaka, Ichi, Übler, Hannah, Wilman, Dave J.
Publikováno v:
The Astrophysical Journal, 834(2):135. IOP PUBLISHING LTD
We present 0.″2-resolution Atacama Large Millimeter/submillimeter Array observations at 870 μm for 25 Hα-seleced star-forming galaxies around the main sequence at z = 2.2-2.5. We detect significant 870 μm continuum emission in 16 (64%) of these
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::25b75384e99e638c3d4f9d7be5478d4c
https://research.rug.nl/en/publications/e9d300e2-1ef0-40ca-85b8-0b47a0990dba
https://research.rug.nl/en/publications/e9d300e2-1ef0-40ca-85b8-0b47a0990dba
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We study the correlation between the morphological mix of cluster galaxies and the assembly history of the parent cluster by taking advantage of two independently developed semi-analytic models for galaxy formation and evolution. In our models, both