We report the detection of ADFS-27, a dusty, starbursting major merger at a redshift of z=5.655, using the Atacama Large Millimeter/submillimeter Array (ALMA). ADFS-27 was selected from Herschel/SPIRE and APEX/LABOCA data as an extremely red “870 m riser” (i.e., S250m<S350m<S500m<S870m), demonstrating the utility of this technique to identify some of the highest-redshift dusty galaxies. A scan of the 3mm atmospheric window with ALMA yields detections of CO(J=54) and CO(J=65) emission, and a tentative detection of H2O(211202) emission, which provides an unambiguous redshift measurement. The strength of the CO lines implies a large molecular gas reservoir with a mass of Mgas=2.51011 (CO=0:8) (0:39=r51)M, sufficient to maintain its 2400M yr1 s...
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society,...
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in...
We report the detection of ADFS-27, a dusty, starbursting major merger at a redshift of z = 5.655, u...
We report new observations toward the hyper-luminous dusty starbursting major merger ADFS-27 (z=5.65...
We present ultrahigh spatial resolution (˜20 mas or 150 pc) ALMA observations of the dust continuum ...
We report the detection of ADFS-27, a dusty, starbursting major merger at a redshift of z=5.655, usi...
Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Arra...
We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using Northern Extend...
Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Arra...
Using the Atacama Large Millimeter/submillimeter Array (ALMA), we report high angular-resolution obs...
We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using NOEMA and ALMA,...
We exploit the continuity equation approach and “main-sequence” star formation timescales to show th...
We report the serendipitous detection of two 3 mm continuum sources found in deep ALMA Band 3 observ...
We report interferometric imaging of [C II](^2 P_(3/2)→^2 P_(1/2)) and OH(^2Π_(1/2)J = 3/2→1/2) emis...
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society,...
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in...
We report the detection of ADFS-27, a dusty, starbursting major merger at a redshift of z = 5.655, u...
We report new observations toward the hyper-luminous dusty starbursting major merger ADFS-27 (z=5.65...
We present ultrahigh spatial resolution (˜20 mas or 150 pc) ALMA observations of the dust continuum ...
We report the detection of ADFS-27, a dusty, starbursting major merger at a redshift of z=5.655, usi...
Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Arra...
We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using Northern Extend...
Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Arra...
Using the Atacama Large Millimeter/submillimeter Array (ALMA), we report high angular-resolution obs...
We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using NOEMA and ALMA,...
We exploit the continuity equation approach and “main-sequence” star formation timescales to show th...
We report the serendipitous detection of two 3 mm continuum sources found in deep ALMA Band 3 observ...
We report interferometric imaging of [C II](^2 P_(3/2)→^2 P_(1/2)) and OH(^2Π_(1/2)J = 3/2→1/2) emis...
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society,...
Aims. We present the detailed characterisation of a sample of 56 sources serendipitously detected in...