activity
20082018
most citedStudying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2

97 citations · 355 across the 9 of their papers we have counts for

collaborators

9 papers

physics.pop-ph2018★ 1 cited

Sitnikov in Westeros: How Celestial Mechanics finally explains why winter is coming in Game of Thrones

Florian Freistetter, Ruth Grützbauch

"Winter is coming". As far as meteorological predictions go, the words of House Stark are both trivial and not very helpful for a scientific analysis to explain the chaotic sequenc…

astro-ph.CO2013★ 39 cited

SINFONI/VLT 3D spectroscopy of massive galaxies: Evidence of rotational support at z~1.4

Fernando Buitrago, Christopher J. Conselice, Benoit Epinat +3

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. Ho…

astro-ph.CO2013★ 97 cited

Studying the emergence of the red sequence through galaxy clustering: host halo masses at z > 2

William G. Hartley, Omar Almaini, Alice Mortlock +10

We use the UKIDSS Ultra-Deep Survey, the deepest degree-scale near-infrared survey to date, to investigate the clustering of star-forming and passive galaxies to z ~ 3.5. Our new m…

astro-ph.CO2010

Galaxy properties in different environments at z > 1.5 in the GOODS-NICMOS Survey

Ruth Grützbauch, Robert W. Chuter, Christopher J. Conselice +4

We present a study of the relationship between galaxy colour, stellar mass, and local galaxy density in a deep near-infrared imaging survey up to a redshift of z~3 using the GOODS…

astro-ph.CO2010★ 17 cited

Nature vs. nurture in the low-density environment: structure and evolution of early-type dwarf galaxies in poor groups

F. Annibali, R. Grutzbauch, R. Rampazzo +2

We present the stellar population properties of 13 dwarf galaxies residing in poor groups (low-density environment, LDE) observed with VIMOS@VLT. Ages, metallicities, and [alpha/Fe…

astro-ph.CO2010★ 30 cited

Star Formation in the XMMU J2235.3-2557 Galaxy Cluster at z=1.39

Amanda E. Bauer, Ruth Grutzbauch, Inger Jorgensen +2

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 narrow-band imaging with NIRI on Gem…

astro-ph.CO2010★ 92 cited

The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3

C. J. Conselice, A. F. L. Bluck, F. Buitrago +27

We present the details and early results from a deep near-infrared survey utilising the NICMOS instrument on the Hubble Space Telescope centred around massive M_* > 10^11 M_0 galax…

astro-ph.CO2010★ 73 cited

How does galaxy environment matter? The relationship between galaxy environments, colour and stellar mass at 0.4 < z < 1 in the Palomar/DEEP2 survey

Ruth Grützbauch, Christopher J. Conselice, Jesús Varela +4

We present a study characterizing the environments of galaxies in the redshift range of 0.4 < z < 1 based on data from the POWIR near infrared imaging and DEEP2 spectroscopic redsh…

astro-ph2008★ 6 cited

XMM-Newton X-ray and Optical Monitor far UV observations of NGC 7070A and ESO 2400100 shell galaxies

G. Trinchieri, R. Rampazzo, C. Chiosi +3

We present XMM-Newton X-ray observations of two shell galaxies, NGC 7070A and ESO 2400100, and far UV observations obtained with the Optical Monitor for these and for an additional…