GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc fiber Bragg gratings to suppress the 103 brightest atmospheric hydroxyl emission doublets between 1.47-1.7 μm. The unit is designed to be used at the 3.9-
Near-infrared emission from atmospheric OH radicals is known to severely affect astronomical observa...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
We demonstrate the direct inscription of aperiodic fiber Bragg gratings (AFBGs) for their use as in-...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
GNOSIS is an OH suppression unit to be used in conjunction with existing spectrographs. The OH suppr...
The sky background is over 1000 times brighter in the near-infrared (NIR) than in the visible placin...
The near-infrared is an important part of the spectrum in astronomy, especially in cosmology because...
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric e...
The near-infrared is an important part of the spectrum in astronomy, especially in cosmology because...
Astronomical near-infrared spectroscopy is made difficult by the extremely bright and variable night...
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric em...
Ground-based near-infrared (NIR) astronomy is severely hampered by the forest of atmospheric emissio...
We analyse the near-infrared interline sky background, OH and O2 emission in 19 h of H-band observat...
We demonstrate the design and fabrication of multichannel fibre Bragg gratings (FBGs) with aperiodic...
A long-standing and profound problem in astronomy is the difficulty in obtaining deep near-infrared ...
Near-infrared emission from atmospheric OH radicals is known to severely affect astronomical observa...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
We demonstrate the direct inscription of aperiodic fiber Bragg gratings (AFBGs) for their use as in-...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
GNOSIS is an OH suppression unit to be used in conjunction with existing spectrographs. The OH suppr...
The sky background is over 1000 times brighter in the near-infrared (NIR) than in the visible placin...
The near-infrared is an important part of the spectrum in astronomy, especially in cosmology because...
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric e...
The near-infrared is an important part of the spectrum in astronomy, especially in cosmology because...
Astronomical near-infrared spectroscopy is made difficult by the extremely bright and variable night...
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric em...
Ground-based near-infrared (NIR) astronomy is severely hampered by the forest of atmospheric emissio...
We analyse the near-infrared interline sky background, OH and O2 emission in 19 h of H-band observat...
We demonstrate the design and fabrication of multichannel fibre Bragg gratings (FBGs) with aperiodic...
A long-standing and profound problem in astronomy is the difficulty in obtaining deep near-infrared ...
Near-infrared emission from atmospheric OH radicals is known to severely affect astronomical observa...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
We demonstrate the direct inscription of aperiodic fiber Bragg gratings (AFBGs) for their use as in-...