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- W3102363529 abstract "(Abr.) Laser guide stars employed at astronomical observatories provide artificial wavefront reference sources to help correct (in part) the impact of atmospheric turbulence on astrophysical observations. Following the recent commissioning of the 4 Laser Guide Star Facility (4LGSF) on UT4 at the VLT, we characterize the spectral signature of the uplink beams from the 22W lasers to assess the impact of laser scattering from the 4LGSF on science observations. We use the MUSE optical integral field spectrograph to acquire spectra at a resolution of R~3000 of the uplink laser beams over the wavelength range of 4750AA to 9350AA. We report the first detection of laser-induced Raman scattering by N2, O2, CO2, H2O and (tentatively) CH4 molecules in the atmosphere above the astronomical observatory of Cerro Paranal. In particular, our observations reveal the characteristic spectral signature of laser photons -- but 480AA to 2210AA redder than the original laser wavelength of 5889.959AA -- landing on the 8.2m primary mirror of UT4 after being Raman-scattered on their way up to the sodium layer. Laser-induced Raman scattering is not unique to the observatory of Cerro Paranal, but common to any astronomical telescope employing a laser-guide-star (LGS) system. It is thus essential for any optical spectrograph coupled to a LGS system to handle thoroughly the possibility of a Raman spectral contamination via a proper baffling of the instrument and suitable calibrations procedures. These considerations are particularly applicable for the HARMONI optical spectrograph on the upcoming Extremely Large Telescope. At sites hosting multiple telescopes, laser collision prediction tools also ought to account for the presence of Raman emission from the uplink laser beam(s) to avoid the unintentional contamination of observations acquired with telescopes in the vicinity of a LGS system." @default.
- W3102363529 created "2020-11-23" @default.
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- W3102363529 date "2017-06-22" @default.
- W3102363529 modified "2023-09-27" @default.
- W3102363529 title "Detection and Implications of Laser-Induced Raman Scattering at Astronomical Observatories" @default.
- W3102363529 cites W1966318877 @default.
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- W3102363529 cites W1972804321 @default.
- W3102363529 cites W1973466816 @default.
- W3102363529 cites W1974230254 @default.
- W3102363529 cites W1975827446 @default.
- W3102363529 cites W1976071155 @default.
- W3102363529 cites W1977583522 @default.
- W3102363529 cites W1982181624 @default.
- W3102363529 cites W1983208565 @default.
- W3102363529 cites W1985027493 @default.
- W3102363529 cites W1985573545 @default.
- W3102363529 cites W1993543543 @default.
- W3102363529 cites W1999633912 @default.
- W3102363529 cites W2000958060 @default.
- W3102363529 cites W2005395150 @default.
- W3102363529 cites W2010954276 @default.
- W3102363529 cites W2011301426 @default.
- W3102363529 cites W2018293667 @default.
- W3102363529 cites W2018612296 @default.
- W3102363529 cites W2031022555 @default.
- W3102363529 cites W2032260186 @default.
- W3102363529 cites W2037564791 @default.
- W3102363529 cites W2038539455 @default.
- W3102363529 cites W2040609398 @default.
- W3102363529 cites W2046002177 @default.
- W3102363529 cites W2048772550 @default.
- W3102363529 cites W2048926060 @default.
- W3102363529 cites W2049715109 @default.
- W3102363529 cites W2050092252 @default.
- W3102363529 cites W2050316146 @default.
- W3102363529 cites W2064902323 @default.
- W3102363529 cites W2070873852 @default.
- W3102363529 cites W2071173961 @default.
- W3102363529 cites W2076348439 @default.
- W3102363529 cites W2079065112 @default.
- W3102363529 cites W2079933224 @default.
- W3102363529 cites W2079941944 @default.
- W3102363529 cites W2081220046 @default.
- W3102363529 cites W2085566693 @default.
- W3102363529 cites W2086325498 @default.
- W3102363529 cites W2087849936 @default.
- W3102363529 cites W2092745113 @default.
- W3102363529 cites W2112764428 @default.
- W3102363529 cites W2127847993 @default.
- W3102363529 cites W2132733111 @default.
- W3102363529 cites W2135625048 @default.
- W3102363529 cites W2136610436 @default.
- W3102363529 cites W2136840156 @default.
- W3102363529 cites W2150659820 @default.
- W3102363529 cites W2151987085 @default.
- W3102363529 cites W2161738620 @default.
- W3102363529 cites W2161934282 @default.
- W3102363529 cites W2168821239 @default.
- W3102363529 cites W2475679609 @default.
- W3102363529 cites W2475947974 @default.
- W3102363529 cites W2477500442 @default.
- W3102363529 cites W2493738696 @default.
- W3102363529 cites W2495523141 @default.
- W3102363529 cites W2497276778 @default.
- W3102363529 cites W2502506140 @default.
- W3102363529 cites W2506384788 @default.
- W3102363529 cites W2558075325 @default.
- W3102363529 cites W3095066679 @default.
- W3102363529 cites W3098856404 @default.
- W3102363529 cites W3102084060 @default.
- W3102363529 cites W3103181481 @default.
- W3102363529 cites W3103620604 @default.
- W3102363529 cites W3104858282 @default.
- W3102363529 cites W3106116524 @default.
- W3102363529 cites W3106221283 @default.
- W3102363529 cites W4238072240 @default.
- W3102363529 cites W1992307720 @default.
- W3102363529 doi "https://doi.org/10.1103/physrevx.7.021044" @default.
- W3102363529 hasPublicationYear "2017" @default.
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