We present HCN J = 4 ! 3 and HCO+ J = 4 ! 3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068, IC 342, M82, M83, and NGC 6946, obtained with the James Clerk Maxwell Telescope as part of the MALATANG survey. All galaxies were mapped in the central 2′ � 2′ region at 14′′ (FWHM) resolution (corresponding to linear scales of � 0:
We have obtained three-dimensional maps of the universe in ~200 × 200 × 80 comoving Mpc3 (cMpc3) vol...
The PHANGS program is building the first data set to enable the multiphase, multiscale study of star...
Large-scale structures (LSSs) out to z 0.8, the SFR density is uniformly distributed over all envir...
We present HCN J = 4 ! 3 and HCO+ J = 4 ! 3 maps of six nearby star-forming galaxies, NGC 253, NGC 1...
This is an author-created, un-copyedited version of an article published in The Astrophysical Journa...
We present HCN J = 4→3 and HCO+ J = 4→3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068,...
Abstract We present and maps of six nearby star-forming galaxies, NGC 253, NGC 1068, I...
We present HCN J = 4→3 and HCO+ J = 4→3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068,...
We present HCN J = 4 -> 3 and HCO+ J = 4 -> 3 maps of six nearby star-forming galaxies, NGC 253, NGC...
We present {HCN} J=4\to 3 and {HCO}}+ J=4\to 3 maps of six nearby star-forming galaxies, NGC 253, NG...
The PHANGS program is building the first data set to enable the multiphase, multiscale study of star...
We present a study of the dust-to-gas ratios in five nearby galaxies: NGC 628 (M74), NGC 6503, NGC 7...
We present bright [C ii] 158 mu m line detections from a strongly magnified and multiply imaged (mu ...
We present bright [C ii] 158 μm line detections from a strongly magnified and multiply imaged (μ ∼ 2...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We have obtained three-dimensional maps of the universe in ~200 × 200 × 80 comoving Mpc3 (cMpc3) vol...
The PHANGS program is building the first data set to enable the multiphase, multiscale study of star...
Large-scale structures (LSSs) out to z 0.8, the SFR density is uniformly distributed over all envir...
We present HCN J = 4 ! 3 and HCO+ J = 4 ! 3 maps of six nearby star-forming galaxies, NGC 253, NGC 1...
This is an author-created, un-copyedited version of an article published in The Astrophysical Journa...
We present HCN J = 4→3 and HCO+ J = 4→3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068,...
Abstract We present and maps of six nearby star-forming galaxies, NGC 253, NGC 1068, I...
We present HCN J = 4→3 and HCO+ J = 4→3 maps of six nearby star-forming galaxies, NGC 253, NGC 1068,...
We present HCN J = 4 -> 3 and HCO+ J = 4 -> 3 maps of six nearby star-forming galaxies, NGC 253, NGC...
We present {HCN} J=4\to 3 and {HCO}}+ J=4\to 3 maps of six nearby star-forming galaxies, NGC 253, NG...
The PHANGS program is building the first data set to enable the multiphase, multiscale study of star...
We present a study of the dust-to-gas ratios in five nearby galaxies: NGC 628 (M74), NGC 6503, NGC 7...
We present bright [C ii] 158 mu m line detections from a strongly magnified and multiply imaged (mu ...
We present bright [C ii] 158 μm line detections from a strongly magnified and multiply imaged (μ ∼ 2...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We have obtained three-dimensional maps of the universe in ~200 × 200 × 80 comoving Mpc3 (cMpc3) vol...
The PHANGS program is building the first data set to enable the multiphase, multiscale study of star...
Large-scale structures (LSSs) out to z 0.8, the SFR density is uniformly distributed over all envir...