We report the discovery of a bright, R = 19.5, arc-like feature associated with a rich cluster of galaxies at a redshift of z = 0.56, found in the course of a programme of optical identification of powerful ultra-steep spectrum radio sources at high redshifts. The redshift of this nearly straight arc, z = 1 .116, implies that the feature is the gravitationally lensed image of a background galaxy. The morphology of the arc, its emission line spectrum and blue colour, and its extremely high surface brightness indicate that the lensed galaxy is likely to be a luminous starburst galaxy, probably a merger of two late type systems. The new arc is the brightest and one of the most distant giant arcs discovered to date, and the only spectroscopical...
The most massive galaxies and the richest clusters are believed to have emerged from regions with th...
Faint straight arcs extending over ten to twenty arcseconds have been observed behind rich clusters ...
We present images and long-slit spectra obtained with FORS1 at UT1 of the VLT centered on the grav...
The cluster CL 1358+62 displays a prominent red arc in WFPC2 images obtained with the Hubble Space T...
Submitted to: Astrophys. J. Abstract: The cluster CL1358+62 displays a prominent red arc in WFPC2 im...
International audienceAs part of an all-sky follow-up of the Planck catalogue of Sunyaev-Zeldovich (...
As part of an all-sky follow-up of the Planck catalogue of Sunyaev-Zeldovich (SZ) cluster candidates...
We present the spatially resolved emission line ratio properties of a ∼ 1010 M⊙ star-forming galaxy ...
We present the first three galaxy clusters of a larger sample of the most X-ray luminous galaxy clus...
International audienceUsing Hubble Space Telescope imaging and Keck spectroscopy, we report the disc...
We report the discovery of two bright arcs in what turns out to be the brightest X-ray cluster in th...
6 pages, accepted for publication in A&AThe center of the galaxy cluster RX J0054.0-2823 at z = 0.29...
We present images and long-slit spectra obtained with FORS1 at UT1 of the VLT centered on the gravit...
We identify a strong lensing galaxy in the cluster IRC 0218 (also known as XMM-LSS J02182-05102) tha...
We measure the bulk photometric properties of a sample of 105 giant arcs that were identified in sys...
The most massive galaxies and the richest clusters are believed to have emerged from regions with th...
Faint straight arcs extending over ten to twenty arcseconds have been observed behind rich clusters ...
We present images and long-slit spectra obtained with FORS1 at UT1 of the VLT centered on the grav...
The cluster CL 1358+62 displays a prominent red arc in WFPC2 images obtained with the Hubble Space T...
Submitted to: Astrophys. J. Abstract: The cluster CL1358+62 displays a prominent red arc in WFPC2 im...
International audienceAs part of an all-sky follow-up of the Planck catalogue of Sunyaev-Zeldovich (...
As part of an all-sky follow-up of the Planck catalogue of Sunyaev-Zeldovich (SZ) cluster candidates...
We present the spatially resolved emission line ratio properties of a ∼ 1010 M⊙ star-forming galaxy ...
We present the first three galaxy clusters of a larger sample of the most X-ray luminous galaxy clus...
International audienceUsing Hubble Space Telescope imaging and Keck spectroscopy, we report the disc...
We report the discovery of two bright arcs in what turns out to be the brightest X-ray cluster in th...
6 pages, accepted for publication in A&AThe center of the galaxy cluster RX J0054.0-2823 at z = 0.29...
We present images and long-slit spectra obtained with FORS1 at UT1 of the VLT centered on the gravit...
We identify a strong lensing galaxy in the cluster IRC 0218 (also known as XMM-LSS J02182-05102) tha...
We measure the bulk photometric properties of a sample of 105 giant arcs that were identified in sys...
The most massive galaxies and the richest clusters are believed to have emerged from regions with th...
Faint straight arcs extending over ten to twenty arcseconds have been observed behind rich clusters ...
We present images and long-slit spectra obtained with FORS1 at UT1 of the VLT centered on the grav...