activity
20042009
most citedAge Determination of Six Intermediate-age SMC Star Clusters with HST/ACS

225 citations · 485 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2009★ 53 cited

Structural Parameters of Seven SMC Intermediate-Age and Old Star Clusters

Katharina Glatt, Eva K. Grebel, John S. Gallagher III. +9

We present structural parameters for the seven intermediate-age and old star clusters NGC121, Lindsay 1, Kron 3, NGC339, NGC416, Lindsay 38, and NGC419 in the Small Magellanic Clou…

astro-ph2008★ 225 cited

Age Determination of Six Intermediate-age SMC Star Clusters with HST/ACS

Katharina Glatt, Eva K. Grebel, Elena Sabbi +9

We present a photometric analysis of the star clusters Lindsay 1, Kron 3, NGC339, NGC416, Lindsay 38, and NGC419 in the Small Magellanic Cloud (SMC), observed with the Hubble Space…

astro-ph2008★ 82 cited

Comparing CN and CH Line Strengths in a Homogeneous Spectroscopic Sample of 8 Galactic Globular Clusters

Andrea Kayser, Michael Hilker, Eva K. Grebel +1

Our work focuses on the understanding of the origin of CNO-anomalies, which have been detected in several Galactic globular clusters (GCs). This study is based on a homogeneous dat…

astro-ph2006★ 29 cited

Medium resolution spectroscopy in Omega Centauri: abundances of 400 subgiant and turn-off region

Andrea Kayser, Michael Hilker, Tom Richtler +1

Medium resolution spectra of more than 400 subgiant and turn-off region stars in Omega Centauri were analysed. The observations were performed at the VLT/Paranal with FORS2/MXU. In…

astro-ph2006★ 1 cited

The Age-Metallicity Relation of the SMC

A. Kayser, E. K. Grebel, D. R. Harbeck +4

The Small Magellanic Cloud (SMC) is the only dwarf galaxy in the Local Group known to have formed and preserved populous star clusters continuously over the past 12 Gyr. These clus…

astro-ph2005★ 28 cited

Analysis of medium resolution spectra by automated methods - application to M55 and omega Centauri

P. G. Willemsen, M. Hilker, A. Kayser +1

We have employed feedforward neural networks trained on synthetic spectra in the range 3800 to 5600 AA with resolutions of 2-3 AA to determine metallicities from spectra of about 1…