278 citations · 660 across the 10 of their papers we have counts for
10 papers
EROs found behind lensing clusters: II.Empirical properties, classification, and SED modelling based on multi-wavelength observations
A. Hempel, D. Schaerer, E. Egami +5
We study the properties and nature of extremely red galaxies (ERO, R-K>5.6) found behind two lensing clusters and compare them with other known galaxy populations. New HST/ACS obse…
EROs found behind lensing clusters. II. Stellar populations and dust properties of optical dropout EROs and comparison with related objects
D. Schaerer, A. Hempel, E. Egami +6
We determine the nature, redshift, stellar populations and dust properties of optically faint or non-detected extremely red objects (ERO) found from our survey of the lensing clust…
Resolved Spectroscopy of a Gravitationally Lensed L* Lyman-break Galaxy at z~5
A. M. Swinbank, R. G. Bower, G. P. Smith +6
By combining HST imaging with optical (VIMOS) and near-infrared (SINFONI) integral field spectroscopy we exploit the gravitational potential of a massive, rich cluster at z=0.9 to…
High resolution imaging of the anomalous flux-ratio gravitational lens system CLASS B2045+265: Dark or luminous satellites?
J. P. McKean, L. V. E. Koopmans, C. E. Flack +6
The existence of flux-ratio anomalies between fold and cusp images in galaxy-scale strong-lens systems has led to an interpretation based on the presence of a high mass-fraction of…
Searching for the first galaxies through gravitational lenses
D. Schaerer, R. Pello, J. Richard +7
Observing the first galaxies formed during the reionisation epoch, i.e. approximately within the first billion years after the Big Bang, remains one of the challenges of contempora…
The Link between Submillimetre Galaxies and Luminous Ellipticals: Near-Infrared IFU Spectroscopy of Submillimetre Galaxies
Mark Swinbank, ; Scott Chapman, Ian Smail +5
We present two-dimensional spectroscopy covering the rest-frame wavelengths of strong optical emission lines in six luminous submillimetre galaxies at z=1.3--2.5. Together with HST…