We present a search for the [C II] 158 μm fine structure line (a main cooling line of the interstellar medium) and the underlying far-infrared (FIR) continuum in three high-redshift (6.6 6 LAEs studied here is lower by a factor of a few than what has recently been found in some LAEs at lower redshift (2 6 LAE sample is consistent with recent rest-frame UV studies of z ~ 7 Lyman break galaxies
The definitive article is available at: http://www3.interscience.wiley.com/ Copyright Royal Astronom...
Using deep Keck spectroscopy of Lyman break galaxies selected from infrared imaging data taken with ...
Strong [O iii]λλ4959,5007 + Hβ emission appears to be typical in star-forming galaxies at z > 6.5...
We present deep HST near-IR and Spitzer mid-IR observations of a large sample of spectroscopically- ...
We report on deep spectroscopy, using LRIS on Keck I and FORS2 on the VLT, of a sample of 22 candida...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We present the results of a photometric redshift analysis designed to identify z≥ 6 galaxies from th...
We present and discuss the mean rest-frame ultraviolet spectrum for a sample of 81 Lyman break galax...
Using Hα spectra of 114 rest-frame UV-selected galaxies at z ~ 2, we compare inferred star formation...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
The fraction of Lyman-α emitters (LAEs) among the galaxy population has been found to increase from ...
Using the Very Large Array and ALMA, we have obtained CO(2–1), [C II], and [N II] line emission and ...
We present the results of ALMA spectroscopic follow-up of a z = 6.766 Lyα emitting galaxy behind the...
We have obtained deep ultraviolet imaging of the lensing cluster A1689 with the WFC3/UVIS camera onb...
We study the physical characteristics of galaxies at 6.3 \u3c z \u3c 8.6, selected from deep near-in...
The definitive article is available at: http://www3.interscience.wiley.com/ Copyright Royal Astronom...
Using deep Keck spectroscopy of Lyman break galaxies selected from infrared imaging data taken with ...
Strong [O iii]λλ4959,5007 + Hβ emission appears to be typical in star-forming galaxies at z > 6.5...
We present deep HST near-IR and Spitzer mid-IR observations of a large sample of spectroscopically- ...
We report on deep spectroscopy, using LRIS on Keck I and FORS2 on the VLT, of a sample of 22 candida...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
We present the results of a photometric redshift analysis designed to identify z≥ 6 galaxies from th...
We present and discuss the mean rest-frame ultraviolet spectrum for a sample of 81 Lyman break galax...
Using Hα spectra of 114 rest-frame UV-selected galaxies at z ~ 2, we compare inferred star formation...
We provide a systematic measurement of the rest-frame UV continuum slope β over a wide range in reds...
The fraction of Lyman-α emitters (LAEs) among the galaxy population has been found to increase from ...
Using the Very Large Array and ALMA, we have obtained CO(2–1), [C II], and [N II] line emission and ...
We present the results of ALMA spectroscopic follow-up of a z = 6.766 Lyα emitting galaxy behind the...
We have obtained deep ultraviolet imaging of the lensing cluster A1689 with the WFC3/UVIS camera onb...
We study the physical characteristics of galaxies at 6.3 \u3c z \u3c 8.6, selected from deep near-in...
The definitive article is available at: http://www3.interscience.wiley.com/ Copyright Royal Astronom...
Using deep Keck spectroscopy of Lyman break galaxies selected from infrared imaging data taken with ...
Strong [O iii]λλ4959,5007 + Hβ emission appears to be typical in star-forming galaxies at z > 6.5...