GNOSIS is an OH suppression unit to be used in conjunction with existing spectrographs. The OH suppression is achieved using fibre Bragg gratings (FBGs), and will deliver the darkest near-infrared background of any ground-based instrument. Laboratory and on-sky tests demonstrate that FBGs can suppress OH lines by 30dB whilst maintaing > 90% throughput between the lines, resulting in a 4 mag decrease in the background. In the first implementation GNOSIS will feed IRIS2 on the AAT. It will consist of a seven element lenslet array, covering 1.4" on the sky, and will suppress the 103 brightest OH lines between 1.47 and 1.70 μm. Future upgrades will include J-band suppression and implementation on an 8m telescope.10 page(s
We demonstrate the design and fabrication of multichannel fibre Bragg gratings (FBGs) with aperiodic...
We present results from the first on-sky demonstration of a prototype astronomical integrated photon...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
The sky background is over 1000 times brighter in the near-infrared (NIR) than in the visible placin...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
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...
Astronomical near-infrared spectroscopy is made difficult by the extremely bright and variable night...
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 em...
We analyse the near-infrared interline sky background, OH and O2 emission in 19 h of H-band observat...
Ground-based near-infrared (NIR) astronomy is severely hampered by the forest of atmospheric emissio...
This paper describes an OH-airglow Suppressor (OHS) for the infrared Nasmyth focus of the Subaru tel...
Near-infrared emission from atmospheric OH radicals is known to severely affect astronomical observa...
We demonstrate the design and fabrication of multichannel fibre Bragg gratings (FBGs) with aperiodic...
We present results from the first on-sky demonstration of a prototype astronomical integrated photon...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
The sky background is over 1000 times brighter in the near-infrared (NIR) than in the visible placin...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
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...
Astronomical near-infrared spectroscopy is made difficult by the extremely bright and variable night...
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 em...
We analyse the near-infrared interline sky background, OH and O2 emission in 19 h of H-band observat...
Ground-based near-infrared (NIR) astronomy is severely hampered by the forest of atmospheric emissio...
This paper describes an OH-airglow Suppressor (OHS) for the infrared Nasmyth focus of the Subaru tel...
Near-infrared emission from atmospheric OH radicals is known to severely affect astronomical observa...
We demonstrate the design and fabrication of multichannel fibre Bragg gratings (FBGs) with aperiodic...
We present results from the first on-sky demonstration of a prototype astronomical integrated photon...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...