Add to ORKGThe Near-infrared Integral Field Spectrograph (NIFS) will be Australia's rst Gem-ini instrument. NIFS is a near-infrared, imaging spectrograph that will be used with the ALTAIR facility adaptive optics system on Gemini North to perform near diraction-limited imaging spectroscopy over a 3:
The Euclid mission objective is to understand why the expansion of the Universe is accelerating thro...
The high sensitivity of large format InSb arrays can be used to obtain deep images of the sky at 3–5...
SINFONI, the SINgle Faint Object Near-infrared Investigation, is an instrument for the Very Large Te...
The Near-infrared Integral Field Spectrograph (NIFS) will be Australia's first Gemini instrument. NI...
NIFS is a near-infrared integral field spectrograph designed for near diffraction-limited imaging sp...
In the next few years, the International Gemini Observatory, a program of NSF’s NOIRLab, is pursuing...
At the present time, several new Gemini instruments are being delivered and commissioned. The Near-I...
Flamingos-2 (F-2) is a wide-field, near-infrared imager, and long-slit and multi-object spectrograph...
The Gemini High-Resolution Optical SpecTrograph (GHOST) is the newest instrument being developed for...
We describe CIRPASS which is currently being completed at the Institute of Astronomy in Cambridge. T...
The Euclid mission objective is to understand why the expansion of the Universe is accelerating thro...
The Immersion GRating INfrared Spectrometer (IGRINS) is a cross-dispersed near-infrared spectrograph...
The Gemini-North Multiobject Spectrograph (CMOS) includes a powerful capability for integral field s...
International audienceThe near-Infrared echelle-AOTF spectrometer is one channel of the Atmospheric ...
International audienceThe Euclid mission objective is to map the geometry of the dark Universe. The ...
The Euclid mission objective is to understand why the expansion of the Universe is accelerating thro...
The high sensitivity of large format InSb arrays can be used to obtain deep images of the sky at 3–5...
SINFONI, the SINgle Faint Object Near-infrared Investigation, is an instrument for the Very Large Te...
The Near-infrared Integral Field Spectrograph (NIFS) will be Australia's first Gemini instrument. NI...
NIFS is a near-infrared integral field spectrograph designed for near diffraction-limited imaging sp...
In the next few years, the International Gemini Observatory, a program of NSF’s NOIRLab, is pursuing...
At the present time, several new Gemini instruments are being delivered and commissioned. The Near-I...
Flamingos-2 (F-2) is a wide-field, near-infrared imager, and long-slit and multi-object spectrograph...
The Gemini High-Resolution Optical SpecTrograph (GHOST) is the newest instrument being developed for...
We describe CIRPASS which is currently being completed at the Institute of Astronomy in Cambridge. T...
The Euclid mission objective is to understand why the expansion of the Universe is accelerating thro...
The Immersion GRating INfrared Spectrometer (IGRINS) is a cross-dispersed near-infrared spectrograph...
The Gemini-North Multiobject Spectrograph (CMOS) includes a powerful capability for integral field s...
International audienceThe near-Infrared echelle-AOTF spectrometer is one channel of the Atmospheric ...
International audienceThe Euclid mission objective is to map the geometry of the dark Universe. The ...
The Euclid mission objective is to understand why the expansion of the Universe is accelerating thro...
The high sensitivity of large format InSb arrays can be used to obtain deep images of the sky at 3–5...
SINFONI, the SINgle Faint Object Near-infrared Investigation, is an instrument for the Very Large Te...