Following our previous spectroscopic observations of z > 7 galaxies with Gemini/Gemini Near Infra-Red Spectrograph (GNIRS) and Very Large Telescope (VLT)/XSHOOTER, which targeted a total of eight objects,we present here our results froma deeper and largerVLT/FOcal Reducer and Spectrograph (FORS2) spectroscopic sample of Wide Field Camera 3 selected z>7 candidate galaxies.With our FORS2 setup we cover the 737-1070 nm wavelength range, enabling a search for Lyman α in the redshift range spanning 5.06-7.80. We target 22 z-band dropouts and nd no evidence of Lyman α emission, with the exception of a tentative detection (<5σ, which is our adopted criterion for a secure detection) for one object. The upper limits on Lyman α ux and the broad-band ...
We use the spatially-resolved, multi-band photometry in the GOODS South field acquired by the CANDEL...
We present three bright z(+)-dropout candidates selected from deep near-infrared (NIR) imaging of th...
The definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright the Royal Astronom...
Following our previous spectroscopic observations of z > 7 galaxies with Gemini/Gemini Near Infra-Re...
Following our previous spectroscopic observations of z > 7 galaxies with Gemini/Gemini Near Infra-Re...
This thesis presents spectroscopic observations of z ≥ 7 galaxy candidates in the Hubble Ultra Deep ...
International audienceWe study the extent to which very bright (-23.0 \textless M-UV \textless -21.7...
We report the spectroscopic confirmation of two Lyman break galaxies at redshift \u3e 7. The galaxie...
We present ultradeep optical spectroscopy obtained with FORS2 on VLT of seven Lyman-break galaxy (LB...
International audienceWe present three bright z(+)-dropout candidates selected from deep near-infrar...
The recent Hubble Space Telescope near-infrared imaging with the Wide-Field Camera #3 (WFC 3) of the...
We present the results of rest-frame, UV slitless spectroscopic observations of a sample of 32 z ~ 0...
We present the results of rest-frame, UV slitless spectroscopic observations of a sample of 32 z~0.7...
The observed deficit of strongly Lyman-α emitting galaxies at z \u3e 6.5 is attributed to either inc...
International audienceWe present the results of a systematic search for gravitationally lensed conti...
We use the spatially-resolved, multi-band photometry in the GOODS South field acquired by the CANDEL...
We present three bright z(+)-dropout candidates selected from deep near-infrared (NIR) imaging of th...
The definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright the Royal Astronom...
Following our previous spectroscopic observations of z > 7 galaxies with Gemini/Gemini Near Infra-Re...
Following our previous spectroscopic observations of z > 7 galaxies with Gemini/Gemini Near Infra-Re...
This thesis presents spectroscopic observations of z ≥ 7 galaxy candidates in the Hubble Ultra Deep ...
International audienceWe study the extent to which very bright (-23.0 \textless M-UV \textless -21.7...
We report the spectroscopic confirmation of two Lyman break galaxies at redshift \u3e 7. The galaxie...
We present ultradeep optical spectroscopy obtained with FORS2 on VLT of seven Lyman-break galaxy (LB...
International audienceWe present three bright z(+)-dropout candidates selected from deep near-infrar...
The recent Hubble Space Telescope near-infrared imaging with the Wide-Field Camera #3 (WFC 3) of the...
We present the results of rest-frame, UV slitless spectroscopic observations of a sample of 32 z ~ 0...
We present the results of rest-frame, UV slitless spectroscopic observations of a sample of 32 z~0.7...
The observed deficit of strongly Lyman-α emitting galaxies at z \u3e 6.5 is attributed to either inc...
International audienceWe present the results of a systematic search for gravitationally lensed conti...
We use the spatially-resolved, multi-band photometry in the GOODS South field acquired by the CANDEL...
We present three bright z(+)-dropout candidates selected from deep near-infrared (NIR) imaging of th...
The definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright the Royal Astronom...