Our current understanding of galaxy evolution still has many uncertainties associated with the details of the accretion, processing, and removal of gas across cosmic time. The next generation of radio telescopes will image the neutral hydrogen (H i) in galaxies over large volumes at high redshifts, which will provide key insights into these processes. We are conducting the COSMOS H i Large Extragalactic Survey (CHILES) with the Karl G. Jansky Very Large Array, which is the first survey to simultaneously observe H i from z = 0 to z ˜ 0.5. Here, we report the highest redshift H i 21 cm detection in emission to date of the luminous infrared galaxy COSMOS J100054.83+023126.2 at z = 0.376 with the first 178 hr of CHILES data. The total H i mass ...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
The neutral atomic gas content of individual galaxies at large cosmological distances has until rece...
We present neutral hydrogen (H I) and ionized hydrogen (H a) observations of 10 galaxies out to a re...
Our current understanding of galaxy evolution still has many uncertainties associated with the detai...
Our current understanding of galaxy evolution still has many uncertainties associated with the detai...
Measurements of hydrogen are important in our understanding of the Universe. Following reionization ...
We measure the neutral atomic hydrogen (H i) gas content of field galaxies at intermediate redshifts...
High-resolution 21 cm H I deep fields provide spatially and kinematically resolved images of neutral...
We use observations made with the Giant Metrewave Radio Telescope (GMRT) to probe the neutral hydrog...
We present a study of 16 H I-detected galaxies found in 178 h of observations from Epoch 1 of the CO...
Using a spectral stacking technique, we measure the neutral hydrogen (H I) properties of a sample of...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
The neutral atomic gas content of individual galaxies at large cosmological distances has until rece...
We present neutral hydrogen (H I) and ionized hydrogen (H a) observations of 10 galaxies out to a re...
Our current understanding of galaxy evolution still has many uncertainties associated with the detai...
Our current understanding of galaxy evolution still has many uncertainties associated with the detai...
Measurements of hydrogen are important in our understanding of the Universe. Following reionization ...
We measure the neutral atomic hydrogen (H i) gas content of field galaxies at intermediate redshifts...
High-resolution 21 cm H I deep fields provide spatially and kinematically resolved images of neutral...
We use observations made with the Giant Metrewave Radio Telescope (GMRT) to probe the neutral hydrog...
We present a study of 16 H I-detected galaxies found in 178 h of observations from Epoch 1 of the CO...
Using a spectral stacking technique, we measure the neutral hydrogen (H I) properties of a sample of...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
The neutral atomic gas content of individual galaxies at large cosmological distances has until rece...
We present neutral hydrogen (H I) and ionized hydrogen (H a) observations of 10 galaxies out to a re...