SwePub - sökning: WFRF:(Odin P)

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1.	Rosqvist, K., et al. (författare) Levodopa effect on non-motor symptoms in late stage Parkinson's disease 2024 Konferensbidrag (refereegranskat)
2.	Rosqvist, K., et al. (författare) Satisfaction with care in late stage Parkinson's disease 2024 Konferensbidrag (refereegranskat)
3.	Persson, Carina, 1964, et al. (författare) From Molecular Oxygen to Primordial Molecules with the Odin Satellite 2008 Ingår i: Proceedings in Astronomical Society of the Pacific Conference Series "Frontiers of Astronomy", NRAO 50th Anniversary Science Symposium, eds. A. Bridle, J. Condon and G. Hunt.. - 9781583816608 ; 395, s. 378- Konferensbidrag (övrigt vetenskapligt/konstnärligt)abstract Odin is a mm/submm-wave-spectroscopy Astronomy and Aeronomy satellite. Its design life time was two years, but it has now operated successfully for more than six years. Its 1.1 m high-precision telescope, with a beam efficiency of 90%, has beamwidths of 10 arcmin and 2 arcmin at mm and submm wavelengths, respectively. It is equipped with a cryogenic receiver package of four tunable, SSB, submm Schottky mixers covering the 486-504 and 541-581 GHz frequency range, and a fixed-tuned HEMT receiver at a frequency of 118-119 GHz.Odin has discovered the elusive oxygen (O2) molecule at 119 GHz - the detection was made in the ρ Oph A molecular-cloud core. The O2 abundance, X(O2), is ≈5×10^{-8} - Larsson et al. (2007: A&A, 466, 999). Odin has also discovered water (H2O) at 557 GHz in the core of the Milky Way Galaxy - the Sgr A CircumNuclear Disk (CND)- and mapped its distribution in the Sgr A Complex including the +20 and +50 km s-1 Molecular Clouds - Sandqvist et al. (2006: J.Phys. Conf.Ser., 54, 72). Furthermore, devoting about 1,100 orbits (each of which contains 1 hour of observable astronomy time) Odin has performed a spectral-line survey of Orion KL in the ranges 487-492 and 542-577 GHz. There are 280 identified spectral lines from 38 species and 64 unidentified lines [Olofsson et al. (2007: A&A, 476, 791) and Persson et al. (2007: A&A, 476, 807)].Odin has searched for emission from the 557 GHz ortho-H2O line in six nearby starburst galaxies yielding three-sigma upper limits to the water abundance relative to H2 (NGC253 -

Persson, Carina, 1964, et al. (författare)
From Molecular Oxygen to Primordial Molecules with the Odin Satellite
2008
Ingår i: Proceedings in Astronomical Society of the Pacific Conference Series "Frontiers of Astronomy", NRAO 50th Anniversary Science Symposium, eds. A. Bridle, J. Condon and G. Hunt.. - 9781583816608 ; 395, s. 378-
Konferensbidrag (övrigt vetenskapligt/konstnärligt)abstract
- Odin is a mm/submm-wave-spectroscopy Astronomy and Aeronomy satellite. Its design life time was two years, but it has now operated successfully for more than six years. Its 1.1 m high-precision telescope, with a beam efficiency of 90%, has beamwidths of 10 arcmin and 2 arcmin at mm and submm wavelengths, respectively. It is equipped with a cryogenic receiver package of four tunable, SSB, submm Schottky mixers covering the 486-504 and 541-581 GHz frequency range, and a fixed-tuned HEMT receiver at a frequency of 118-119 GHz.Odin has discovered the elusive oxygen (O2) molecule at 119 GHz - the detection was made in the ρ Oph A molecular-cloud core. The O2 abundance, X(O2), is ≈5×10^{-8} - Larsson et al. (2007: A&A, 466, 999). Odin has also discovered water (H2O) at 557 GHz in the core of the Milky Way Galaxy - the Sgr A CircumNuclear Disk (CND)- and mapped its distribution in the Sgr A Complex including the +20 and +50 km s-1 Molecular Clouds - Sandqvist et al. (2006: J.Phys. Conf.Ser., 54, 72). Furthermore, devoting about 1,100 orbits (each of which contains 1 hour of observable astronomy time) Odin has performed a spectral-line survey of Orion KL in the ranges 487-492 and 542-577 GHz. There are 280 identified spectral lines from 38 species and 64 unidentified lines [Olofsson et al. (2007: A&A, 476, 791) and Persson et al. (2007: A&A, 476, 807)].Odin has searched for emission from the 557 GHz ortho-H2O line in six nearby starburst galaxies yielding three-sigma upper limits to the water abundance relative to H2 (NGC253 -

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