We present first results of a spectroscopic survey targeting K-selected galaxies at z=2.0-2.7 using the Gemini near-infrared spectrograph (GNIRS). We obtained near-infrared spectra with a wavelength coverage of 1.0-2.5 mum for 26 K-bright galaxies (K<19.7) selected from the Multi-wavelength Survey by Yale-Chile (MUSYC) using photometric redshifts. We successfully derived spectroscopic redshifts for all 26 galaxies using rest-frame optical emission lines or the redshifted Balmer/4000 Å break. Twenty galaxies have spectroscopic redshifts in the range 2.0<z<2.7, for which bright emission lines like Halpha and [O III] fall in atmospheric windows. Surprisingly, we detected no emission lines for nine of these 20 galaxies. The median 2 sigma upper...
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn fro...
International audienceWe present the results of new near-IR spectroscopic observations of passive ga...
We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 < z ...
We present first results of a spectroscopic survey targeting K-selected galaxies at using the Gemini...
Using the Gemini Near-Infrared Spectrograph (GNIRS), we have completed a near-infrared spectroscopic...
Using the Gemini Near-Infrared Spectrograph (GNIRS), we have completed a near-infrared spectroscopic...
We present the results of deep near-infrared spectroscopy of seven submillimetre-selected galaxies f...
Spectroscopic redshifts have been measured for nine K-band luminous galaxies at 1.7<z<2.3, selected ...
A key issue in astronomy today is understanding the star-formation and assembly history of massive g...
Near infrared slitless spectroscopy with the Wide Field Camera 3, on board the Hubble Space Telescop...
We present spectroscopic evidence from the Gemini Deep Deep Survey for a significant population of c...
The WFC3 Infrared Spectroscopic Parallel Survey uses the Hubble Space Telescope (HST) infrared grism...
We report the likely identification of a substantial population of massive M similar to 10(11) M-cir...
We report the likely identification of a substantial population of massive M ~ 10¹¹ M⊙ galaxies at z...
We perform the first spatially-resolved stellar population study of galaxies in the early universe z...
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn fro...
International audienceWe present the results of new near-IR spectroscopic observations of passive ga...
We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 < z ...
We present first results of a spectroscopic survey targeting K-selected galaxies at using the Gemini...
Using the Gemini Near-Infrared Spectrograph (GNIRS), we have completed a near-infrared spectroscopic...
Using the Gemini Near-Infrared Spectrograph (GNIRS), we have completed a near-infrared spectroscopic...
We present the results of deep near-infrared spectroscopy of seven submillimetre-selected galaxies f...
Spectroscopic redshifts have been measured for nine K-band luminous galaxies at 1.7<z<2.3, selected ...
A key issue in astronomy today is understanding the star-formation and assembly history of massive g...
Near infrared slitless spectroscopy with the Wide Field Camera 3, on board the Hubble Space Telescop...
We present spectroscopic evidence from the Gemini Deep Deep Survey for a significant population of c...
The WFC3 Infrared Spectroscopic Parallel Survey uses the Hubble Space Telescope (HST) infrared grism...
We report the likely identification of a substantial population of massive M similar to 10(11) M-cir...
We report the likely identification of a substantial population of massive M ~ 10¹¹ M⊙ galaxies at z...
We perform the first spatially-resolved stellar population study of galaxies in the early universe z...
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn fro...
International audienceWe present the results of new near-IR spectroscopic observations of passive ga...
We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies at 3 < z ...