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pro vyhledávání: '"Grutzbauch, Ruth"'
Autor:
Simmons, B. D., Melvin, Thomas, Lintott, Chris, Masters, Karen L., Willett, Kyle W., Keel, William C., Smethurst, R. J., Cheung, Edmond, Nichol, Robert C., Schawinski, Kevin, Rutkowski, Michael, Kartaltepe, Jeyhan S., Bell, Eric F., Casteels, Kevin R. V., Conselice, Christopher J., Almaini, Omar, Ferguson, Henry C., Fortson, Lucy, Hartley, William, Kocevski, Dale, Koekemoer, Anton M., McIntosh, Daniel H., Mortlock, Alice, Newman, Jeffrey A., Ownsworth, Jamie, Bamford, Steven, Dahlen, Tomas, Faber, Sandra M., Finkelstein, Steven L., Fontana, Adriano, Galametz, Audrey, Grogin, N. A., Grutzbauch, Ruth, Guo, Yicheng, Haussler, Boris, Jek, Kian J., Kaviraj, Sugata, Lucas, Ray A., Peth, Michael, Salvato, Mara, Wiklind, Tommy, Wuyts, Stijn
The formation of bars in disk galaxies is a tracer of the dynamical maturity of the population. Previous studies have found that the incidence of bars in disks decreases from the local Universe to z ~ 1, and by z > 1 simulations predict that bar feat
Externí odkaz:
http://arxiv.org/abs/1409.1214
Autor:
Jorgensen, Inger, Chiboucas, Kristin, Toft, Sune, Bergmann, Marcel, Zirm, Andrew, Schiavon, Ricardo P., Grutzbauch, Ruth
RXJ0848.6+4453 (Lynx W) at redshift 1.27 is part of the Lynx Supercluster of galaxies. Our analysis of stellar populations and star formation history in the cluster covers 24 members and is based on deep optical spectroscopy from Gemini North and ima
Externí odkaz:
http://arxiv.org/abs/1408.2906
Autor:
Lani, Caterina, Almaini, Omar, Hartley, William G., Mortlock, Alice, Haeussler, Boris, Chuter, Robert W., Simpson, Chris, van der Wel, Arjen, Grutzbauch, Ruth, Conselice, Christopher J., Bradshaw, Emma J., Cooper, Michael C., Faber, Sandra M., Grogin, Norman A., Kocevski, Dale D., Koekemoer, Anton M., Lai, Kamson
We present evidence for a strong relationship between galaxy size and environment for the quiescent population in the redshift range 1 < z < 2. Environments were measured using projected galaxy overdensities on a scale of 400 kpc, as determined from
Externí odkaz:
http://arxiv.org/abs/1307.3247
Autor:
Buitrago, Fernando, Conselice, Christopher J., Epinat, Benoit, Bedregal, Alejandro G., Grutzbauch, Ruth, Weiner, Benjamin J.
There is cumulative evidence showing that, for the most massive galaxies, the fraction of disk-like objects compared to those with spheroidal properties increases with redshift. However, this evolution is thus far based on the surface brightness stud
Externí odkaz:
http://arxiv.org/abs/1305.0268
We present the results of an extended narrow-band H{\alpha} study of the massive galaxy cluster XMMU J2235.3-2557 at z = 1.39. This paper represents a follow up study to our previous investigation of star-formation in the cluster centre, extending ou
Externí odkaz:
http://arxiv.org/abs/1204.4417
Autor:
Bauer, Amanda E., Conselice, Christopher J., Perez-Gonzalez, Pablo G., Grutzbauch, Ruth, Bluck, Asa F. L., Buitrago, Fernando, Mortlock, Alice
We present a study of the star-forming properties of a stellar mass-selected sample of galaxies in the GOODS NICMOS Survey (GNS), based on deep Hubble Space Telescope imaging of the GOODS North and South fields. Using a stellar mass selected sample,
Externí odkaz:
http://arxiv.org/abs/1106.2656
We present the first results of a narrow-band photometric study of the massive galaxy cluster XMMU J2235.3-2557 at z=1.39. We obtained deep $H$ narrow-band imaging with NIRI on Gemini North, corresponding to H-alpha emission at the cluster's redshift
Externí odkaz:
http://arxiv.org/abs/1010.1238
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