ALMA Band 2 observations of SPT-S J002706-5007.4 at z=3.44 detect multiple molecular lines indicating highly excited dense gas and demonstrate the band's utility for high-redshift spectroscopy.
Physics and Chemistry of Star Formation: The Dynamical ISM Across Time and Spatial Scales , year = 2023, editor =
4 Pith papers cite this work, alongside 12 external citations. Polarity classification is still indexing.
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Involving general users in prioritizing development for scientific software like CASA improves alignment with user needs and benefits both communities despite limited support resources.
The SKA will enable high-resolution, high-sensitivity observations of the thermal SZ effect in massive halos, capturing both pressure substructures and large-scale ICM emission.
The paper presents predictions and observational plans for Zeeman effect measurements with SKA to provide statistical data on magnetic field strengths across scales in molecular clouds.
citing papers explorer
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ALMA Band 2 line survey of a $z = 3.44$ clumpy strongly-lensed submillimetre galaxy
ALMA Band 2 observations of SPT-S J002706-5007.4 at z=3.44 detect multiple molecular lines indicating highly excited dense gas and demonstrate the band's utility for high-redshift spectroscopy.
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Role of General Users in the Lifecycle of Scientific Software
Involving general users in prioritizing development for scientific software like CASA improves alignment with user needs and benefits both communities despite limited support resources.
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The SKA View of the Sunyaev-Zeldovich Effect from Massive Cosmic Halos
The SKA will enable high-resolution, high-sensitivity observations of the thermal SZ effect in massive halos, capturing both pressure substructures and large-scale ICM emission.
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Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA
The paper presents predictions and observational plans for Zeeman effect measurements with SKA to provide statistical data on magnetic field strengths across scales in molecular clouds.