The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric emission from hydroxyl molecules. We have built and commissioned a new instrument, the Gemini Near-infrared OH Suppression Integral Field Unit (IFU) SystemGNOSIS was funded by an ARC LIEF grant LE100100164
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
International audienceThe Gemini Planet Imager is a newly commissioned facility instrument designed ...
The Gemini Planet Imager is a newly commissioned facility instrument designed to measure the near-in...
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric e...
GNOSIS is an OH suppression unit to be used in conjunction with existing spectrographs. The OH suppr...
We analyse the near-infrared interline sky background, OH and O2 emission in 19 h of H-band observat...
Astronomical near-infrared spectroscopy is made difficult by the extremely bright and variable night...
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...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
NIFS is a near-infrared integral field spectrograph designed for near diffraction-limited imaging sp...
The near-infrared is an important part of the spectrum in astronomy, especially in cosmology because...
Ground-based near-infrared (NIR) astronomy is severely hampered by the forest of atmospheric emissio...
A long-standing and profound problem in astronomy is the difficulty in obtaining deep near-infrared ...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
International audienceThe Gemini Planet Imager is a newly commissioned facility instrument designed ...
The Gemini Planet Imager is a newly commissioned facility instrument designed to measure the near-in...
The background noise between 1 and 1.8 μm in ground-based instruments is dominated by atmospheric e...
GNOSIS is an OH suppression unit to be used in conjunction with existing spectrographs. The OH suppr...
We analyse the near-infrared interline sky background, OH and O2 emission in 19 h of H-band observat...
Astronomical near-infrared spectroscopy is made difficult by the extremely bright and variable night...
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...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
GNOSIS has provided the first on-telescope demonstration of a concept to utilize complex aperioidc f...
NIFS is a near-infrared integral field spectrograph designed for near diffraction-limited imaging sp...
The near-infrared is an important part of the spectrum in astronomy, especially in cosmology because...
Ground-based near-infrared (NIR) astronomy is severely hampered by the forest of atmospheric emissio...
A long-standing and profound problem in astronomy is the difficulty in obtaining deep near-infrared ...
International audienceA long-standing and profound problem in astronomy is the difficulty in obtaini...
International audienceThe Gemini Planet Imager is a newly commissioned facility instrument designed ...
The Gemini Planet Imager is a newly commissioned facility instrument designed to measure the near-in...