SOFIA observations provide the first experimental magnetic-dipole hyperfine constants for [13C II] and refined centroid frequency using astronomical data.
Review of Scientific Instruments , year = 1946, month = jul, volume =
3 Pith papers cite this work. Polarity classification is still indexing.
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Compact dual-polarization Schottky barrier diode receivers at 315-650 GHz achieve up to 34 dB cross-polarization isolation, DSB noise temperatures down to 833 K, and Allan stability over 10 s in a single module with shared components.
Comparison of Galactic magnetic field models to polarized synchrotron observations shows good agreement on angles but poor match on intensity, indicating local foreground structures must be incorporated.
citing papers explorer
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Space as a spectroscopic laboratory: High-resolution spectroscopy of the [$^{13}$C II] hyperfine structure with SOFIA/upGREAT
SOFIA observations provide the first experimental magnetic-dipole hyperfine constants for [13C II] and refined centroid frequency using astronomical data.
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Compact Dual-Polarization Schottky Barrier Diode Receivers for Submillimeter Wave Remote Sensing
Compact dual-polarization Schottky barrier diode receivers at 315-650 GHz achieve up to 34 dB cross-polarization isolation, DSB noise temperatures down to 833 K, and Allan stability over 10 s in a single module with shared components.
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A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz
Comparison of Galactic magnetic field models to polarized synchrotron observations shows good agreement on angles but poor match on intensity, indicating local foreground structures must be incorporated.