127 citations
- Max Planck SocietyDE61 papers
- CEA Paris-SaclayFR5 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR5 papers
- OpticaUS5 papers
- Thüringer Landessternwarte TautenburgDE4 papers
- University of ÉvoraPT4 papers
- Clemson UniversityUS3 papers
- European Southern ObservatoryCL3 papers
- Goddard Space Flight CenterUS3 papers
- Max Planck Institute for AstrophysicsDE3 papers
- Pacific States UniversityUS3 papers
- Ruhr University BochumDE3 papers
12 papers · 1 filter
Evolution of local Ultraluminous mergers from NIR spectroscopy
K. M. Dasyra, L. J. Tacconi, R. I. Davies +4
We present results from our VLT Large Program to study the dynamical evolution of Ultraluminous Infrared Galaxies (ULIRGs). We have so far obtained near-infrared high-resolution IS…
Multi-Wavelength Studies of the Optically Dark Gamma-Ray Burst 001025A
K. Pedersen, K. Hurley, J. Hjorth +18
We identify the fading X-ray afterglow of GRB 001025A from XMM-Newton observations obtained 1.9-2.3 days, 2 years, and 2.5 years after the burst. The non-detection of an optical co…
Gamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI
A. W. Strong, R. Diehl, H. Halloin +5
The diffuse continuum emission from the Galactic plane in the energy range 18-1000 keV has been studied using 16 Ms of data from the SPI instrument on INTEGRAL. With such an exposu…
Toward a Census of Variable Stars in Northern Local Group Dwarf Irregular Galaxies
J. Snigula, C. A. Goessl, U. Hopp
Dwarf galaxies in the local group provide a unique astrophysical laboratory. In particular, they allow us to probe pulsating (and other) variable stars in low-metallicity environme…
Dust properties of UV bright galaxies at z ~ 2
S. Noll, D. Pierini
We investigate the properties of the extinction curve in the rest-frame UV for a sample of 34 UV-luminous galaxies at 2 < z < 2.5, selected from the FORS Deep Field (FDF) spectrosc…
The XMM-Newton Slew Survey
A. M. Read, R. D. Saxton, M. P. Esquej +2
XMM-Newton, with the huge collecting area of its mirrors and the high quantum efficiency of its EPIC detectors, is the most sensitive X-ray observatory ever flown. This is striking…