activity
19962008
most citedThe SAURON project -- IX. A kinematic classification for early-type galaxies

786 citations · 786 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph2008

Stellar Velocity Profiles and Line-Strengths out to Four Effective Radii in the Early-Type Galaxy NGC 3379

A. Weijmans, M. Cappellari, P. T. de Zeeuw +6

We describe a new technique to measure stellar kinematics and line-strengths at large radii in nearby galaxies. Using the integral-field spectrograph SAURON as a 'photon-collector'…

astro-ph2007786 cited

The SAURON project -- IX. A kinematic classification for early-type galaxies

Eric Emsellem, Michele Cappellari, Davor Krajnovic +10

2D stellar kinematics of 48 representative E and S0 galaxies obtained with the SAURON IFS reveal that early-type galaxies appear in two broad flavours, depending on whether they ex…

astro-ph2003

An XMM and Chandra view of massive clusters of galaxies to z=1

L. R. Jones, B. J. Maughan, H. Ebeling +7

The X-ray properties of a sample of high redshift (z>0.6), massive clusters observed with XMM-Newton and Chandra are described, including two exceptional systems. One, at z=0.89, h…

astro-ph2002

Timing with the EPIC pn Camera of XMM-Newton

Markus Kuster, Eckhard Kendziorra, Sara Benlloch +4

The EPIC pn CCD camera on board of XMM-Newton is designed to perform high throughput imaging and spectroscopy as well as high resolution timing observations in the energy range of…

astro-ph2002

XMM-Newton GT and AO-1 observations of SHARC galaxy clusters : RX J1120.1+4318 and RX J0256.5+0006

Sebastien Majerowicz, Monique Arnaud, David Lumb +1

We present the follow-up of two galaxy clusters from the Bright and Southern SHARC surveys observed with the XMM-Newton satellite. We studied the galaxy cluster RX J1120.1+4318 whi…

astro-ph2002

Strongly absorbed quiescent X-ray emission from the X-ray transient XTE J0421+56

L. Boirin, A. N. Parmar, D. Lumb +2

We have observed the soft X-ray transient XTE J0421+56 in quiescence with XMM-Newton. The observed spectrum is highly unusual being dominated by a broad feature at 6.5 keV and can…